- published: 04 Sep 2015
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"Giovanni" "Domenico Cassini" was an Italian mathematician, astronomer, astrologer and engineer. Cassini was born in Perinaldo, near Imperia, at that time in the County of Nice, part of the Duchy of Savoy. Cassini is known for his work in the fields of astronomy and engineering. Cassini most notably discovered four satellites of the planet Saturn and noted the division of the rings of Saturn . Giovanni Domenico Cassini was also the first of his family to begin work on the project of creating a topographic map of France. Launched in 1997, the Cassini spaceprobe was named after him and became the fourth to visit Saturn and the first to orbit the planet.
Cassini was the son of Jacopo Cassini, a Tuscan, and Julia Crovesi. Cassini accepted a position at the observatory at Panzano, near Bologna, to work with Marquis Cornelio Malvasia, a rich amateur astronomer, in 1648 initiating the first part of Cassini's career. During Cassini's time at the Panzano Observatory, Cassini was able to complete his education under the scientists Giovanni Battista Riccioli and Francesco Maria Grimaldi. In 1650 the senate of Bologna appointed Cassini as the principal chair of astronomy at the University of Bologna. In San Petronio, Bologna, he created an important meridian, which helped settle the debate about whether the universe is geocentric. Cassini remained in Bologna working until Colbert recruited him to come to Paris to help set up the Paris Observatory. Cassini departed from Bologna on 25 February 1669.
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Background Music:
"The Place Inside" by Silent Partner (royalty-free) from YouTube Audio Library.
This video uses material/images from https://en.wikipedia.org/wiki/Giovanni+Domenico+Cassini, which is released under Creative Commons Attribution-Share-Alike License 3.0 http://creativecommons.org/licenses/by-sa/3.0/ . This video is licensed under Creative Commons Attribution-Share-Alike License 3.0 http://creativecommons.org/licenses/by-sa/3.0/ . To reuse/adapt the content in your own work, you must comply with the license terms.
TEMAS TRATADOS: Giovanni Cassini, astrónomo italiano, las frottolas, capítulo de Il piccolo principe. TEMAS MUSICALES. L'appuntamento, Ornella Vanoni, Zingara, Bobby Solo, Las noches de CAbiria(Nino Rotta), VErgine bella frottola de Bartolomeo Tromboncino, La vida es bella(banda de sonido de la pelicula) La lodoiska, de Giovanni Simone Overture, Obertura de Ermione de Rossini.
- published: 05 Jan 2015
- views: 49
SKYVIEWS - FIND IT SOMEDAY - (REPORT BELOW)
CASSINI ON HER MISSION TO SATURN
MARCH 17, 2014
History of Cassini Probe:
Astronomer Giovanni Cassini is associated with a number of scientific discoveries and projects, including the Cassini-Huygens spacecraft that was launched in 1997 and continues to transmit images from Saturn. Born on he was given the name Giovanni Domenico by his parents, Jacopo Cassini and Julia Crovesi.
However he also used the name Gian Domenico Cassini, and after he moved to France as an adult, he changed his name to the French version — Jean-Dominique Cassini. To add to the perplexity, he was the first of the well-known Cassini family of astronomers and is sometimes referred to as Cassini I.
Astronomer Giovanni Cassini is associated with a number of scientific discoveries and projects, including the Cassini-Huygens spacecraft that was launched in 1997 and continues to transmit images from Saturn.
The well-traveled probe won't stop studying Saturn and its many moons anytime soon!!!
Cassini has logged more than 3.8 billion miles (6.1 billion kilometers) since its launch on Oct. 15, 1997, researchers said.
The nearly 12,600-pound (about 5,700 kilograms) spacecraft was hefted off of Earth on Oct. 15, 1997. It went by Venus in April 1998 and June 1999, Earth in August 1999 and Jupiter in December 2000.
Cassini-Huygens is a symbol of the new kind of space exploration and cooperation among different agencies. The spacecraft has spent years circling Saturn and its moons, beaming back pictures and data to teach scientists on Earth more about how the system was formed.
The ambitious mission is also a joint one among several space agencies, which is a contrast from the large NASA probes of the past such as Pioneer and Voyager. In this case, the main participants are NASA, the European Space Agency and Agenzia Spaziale Italiana (the Italian space agency).
While Cassini was supposed to last four years, it's still going strong at more than double its projected mission lifetime.
Since 2004, the Cassini orbiter has studied Saturn and its many natural satellites. Other missions included observing Jupiter, the Heliosphere and testing the theory of relativity. Cassini is the fourth space probe to visit Saturn and the first to enter orbit. It was renamed the Cassini Equinox in 2008 and is currently scheduled to end its mission in 2017.
There are also several craters name for Cassini, including an impact crater on the moon that is located in the Palus Nebularum, and a crater on Mars.
It regularly passes by the moons of Saturn, producing new data and fueling discoveries back on Earth.
NASA's Cassini probe has captured the highest resolution video yet of Saturn's odd, hexagon shaped jet stream that spins around the gas giants north pole.
Cassini-Huygens is a symbol of the new kind of space exploration and cooperation among different agencies. The spacecraft has spent years circling Saturn and its moons, beaming back pictures and data to teach scientists on Earth more about how the system was formed.
As the probe wandered past Saturn's moons, the findings it brought back to Earth revealed new things about their environments and appearances.
On its final orbit In 2017, NASA's Cassini probe will fly between the inner edge of the D ring and the upper atmosphere of the gas giant. It will also fly though an Enceladus plume in the next few years.
Some of the more notable findings include:
• Finding evidence of liquid water on Enceladus, a frozen moon that shoots out icy jets as it is warped by Saturn's gravity;
• Discovering and then pinning down more details about a giant methane lake on Titan;
• 50-mile landslides on Iapetus;
• A close-up view of Rhea, revealing a pockmarked surface;
• A huge ring, 8 million miles away from Saturn, likely made up of debris from Phoebe
Credits Photo: Image Credit: Hubble Legacy Archive, NASA, ESA; Processing & Copyright: Davide Coverta
Last picture credit: The Antennae Galaxies in Collision
Explanation: Two galaxies are squaring off in Corvus and here are the latest pictures. When two galaxies collide, the stars that compose them usually do not. That's because galaxies are mostly empty space and, however bright, stars only take up only a small amount of that space.
During the slow, hundred million year collision, one galaxy can still rip the other apart gravitationally, and dust and gas common to both galaxies does collide. In this clash of the titans, dark dust pillars mark massive molecular clouds are being compressed during the galactic encounter, causing the rapid birth of millions of stars, some of which are gravitationally bound together in massive star clusters.
Musical Audio: Star and Musical Artist: Derek Clegg - Song: Find it Someday www.derekclegg.com
entry submitted by tina marie on March 27, 2014. love and light~tina marie #candotina
- published: 19 Mar 2014
- views: 374
The first scientific map of the Moon, made by Giovanni Cassini in 1679.
This detailed engraving of the surface of the Moon was based on Cassini's own observations made with a telescope.
The features are an accurate representation of the Moon as Cassini saw it -- apart from a mysterious woman's head, which is hidden among the mountains and craters on the engraving.
The Library and Archives of the Royal Astronomical Society contain books, images and documents significant in the development of scientific thought in astronomy, geophysics and related disciplines. In this series of videos RAS Librarian Jenny Higham displays some of the gems of the collection.
- published: 12 Mar 2014
- views: 499
Updated footage in 4K - http://www.youtube.com/watch?v=QNce_8WHTGc&feature;=share
About this footage: "Not-for-profit animated IMAX film in early production by a single filmmaker. Visit the site to make a tax-deductible contribution to support the film. I hope to present this clip at the international IMAX show (GSCA Expo) next month. Visit outsideinthemovie.com/ to donate."
About Cassini: Cassini--Huygens is a joint NASA/ESA/ASI robotic spacecraft mission currently studying the planet Saturn and its many natural satellites. The spacecraft consists of two main elements: the NASA-designed and -constructed Cassini orbiter, named for the Italian-French astronomer Giovanni Domenico Cassini, and the ESA-developed Huygens probe, named for the Dutch astronomer, mathematician and physicist Christiaan Huygens.
The complete Cassini space probe was launched on October 15, 1997, and after a long interplanetary voyage it entered into orbit around Saturn on July 1, 2004. On December 25, 2004, the Huygens probe was separated from the orbiter at approximately 02:00 UTC. It reached Saturn's moon Titan on January 14, 2005, when it descended into Titan's atmosphere, and downward to the surface, radioing scientific information back to the Earth by telemetry. This was the first landing ever accomplished in the outer solar system. On April 18, 2008, NASA announced a two-year extension of the funding for ground operations of this mission, at which point it was renamed to Cassini Equinox Mission.
This was again extended in February 2010 with the mission now continuing until 2017. Cassini is the fourth space probe to visit Saturn and the first to enter orbit.
- published: 14 Mar 2011
- views: 69184
http://www.mekanizmalar.com/menu_linkage.html
This curve known as the lemniscate of Bernoulli. However this curve first investigated by Giovanni Domenico Cassini. Giovanni Cassini was an Italian mathematician and astronomer who studied this curve which is the locus of a point the product of whose distances from two fixed foci is constant.
- published: 09 Jul 2013
- views: 7129
more at http://scitech.quickfound.net/astro/planet_news.html
Titan: Extraterrestrial Land of Lakes
3-D colorized animated view from the Cassini Saturn orbiter spacecraft of methane lakes on Saturn's moon Titan. The animationa was generated from radar images.
Public domain film from NASA-JPL. I have added music created by myself using the Reaper Digital Audio Workstation and the Independence and Proteus VX VST instrument plugins.
http://www.jpl.nasa.gov/news/news.php?release=2013-364
NASA's Cassini spacecraft is providing scientists with key clues about Saturn's moon Titan, and in particular, its hydrocarbon lakes and seas.
Titan is one of the most Earth-like places in the solar system, and the only place other than our planet that has stable liquid on its surface.
Cassini's recent close flybys are bringing into sharper focus a region in Titan's northern hemisphere that sparkles with almost all of the moon's seas and lakes. Scientists working with the spacecraft's radar instrument have put together the most detailed multi-image mosaic of that region to date. The image includes all the seas and most of the major lakes. Some of the flybys tracked over areas that previously were seen at a different angle, so researchers have been able to create a flyover of the area around Titan's largest and second largest seas, known as Kraken Mare and Ligeia Mare, respectively, and some of the nearby lakes...
These new images show Kraken Mare is more extensive and complex than previously thought. They also show nearly all of the lakes on Titan fall into an area covering about 600 miles by 1,100 miles (900 kilometers by 1,800 kilometers). Only 3 percent of the liquid at Titan falls outside of this area...
http://creativecommons.org/licenses/by-sa/3.0/
http://en.wikipedia.org/wiki/Lakes_of_Titan
The lakes of Titan, a moon of Saturn, are bodies of liquid ethane and methane that have been detected by the Cassini--Huygens space probe, and had been suspected long before. The large ones are known as maria (seas) and the small ones as lacūs (lakes).
http://en.wikipedia.org/wiki/Cassini--Huygens
Cassini--Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-class NASA-ESA-ASI robotic spacecraft sent to the Saturn system. It has studied the planet and its many natural satellites since arriving there in 2004, also observing Jupiter, the heliosphere, and testing the theory of relativity. Launched in 1997 after nearly two decades of development, it includes a Saturn orbiter and an atmospheric probe/lander for the moon Titan called Huygens, which entered and landed on Titan in 2005. Cassini is the fourth space probe to visit Saturn and the first to enter orbit, and its mission is ongoing as of 2013. The two-part spacecraft is named after astronomers Giovanni Cassini and Christiaan Huygens...
It launched on October 15, 1997 on a Titan IVB/Centaur and entered into orbit around Saturn on July 1, 2004, after an interplanetary voyage which included flybys of Earth, Venus, and Jupiter. On December 25, 2004, Huygens separated from the orbiter at approximately 02:00 UTC. It reached Saturn's moon Titan on January 14, 2005, when it entered Titan's atmosphere and descended to the surface. It successfully returned data to Earth, using the orbiter as a relay. This was the first landing ever accomplished in the outer Solar System...
- published: 12 Dec 2013
- views: 8269
CassiniHuygens is a joint NASA/ESA robotic spacecraft mission currently studying the planet Saturn and its moons. The spacecraft consists of two main elements: the NASA Cassini orbiter, named after the Italian-French astronomer Giovanni Domenico Cassini, and the ESA Huygens probe, named after the Dutch astronomer, mathematician and physicist Christiaan Huygens.
- published: 03 Feb 2009
- views: 2957
Jápeto
Es uno de los satélites del planeta Saturno. Es el octavo más distante al planeta y el tercero en tamaño, con un diámetro de alrededor de 1500 km, después de los satélites más grandes Titán y Rea. Fue descubierto por Giovanni Cassini en 1671. Tarda en completar una vuelta alrededor de Saturno 79,33 días terrestres, a una distancia media de 3 561 300 km.
Uno de los hemisferios del satélite es mucho más oscuro que el otro, peculiar característica que se podría deber a una composición distinta del material de la superficie, proveniente del interior de la propia luna o bien de materia de otros satélites o anillos. No se conoce con certeza el motivo real, aunque la segunda hipótesis cada vez es más apoyada por evidencias observacionales.
- published: 30 Mar 2016
- views: 4
Saturn's majestic, iconic rings define the planet, but where did they come from?
Kevin Grazier "Saturn's rings, good question. And the answer is different depending on which ring we're discussing."
That's Dr. Kevin Grazier, a planetary scientist who worked on NASA's Cassini mission or over 15 years, studying Saturn's rings extensively.
Mike Brown "Saturn's rings - the strange things about Saturn's rings is that they shouldn't be there, really, in the sense that they don't last for very long. So, if they are just left over from when Saturn was formed, they'd be gone by now. They would slowly work their way into Saturn and burn up and be gone. And yet they're there. So they are either relatively new or somehow continuously regenerated. 'Continuously regenerated' seems strange and 'relatively new' seems also kind of strange. Something broke up - a large moon broke up, or a comet broke up - something had to have happened relatively recently. And by relatively recently, that means hundreds of millions of years ago for someone like me."
And that's Mike Brown, professor of planetary geology at Caltech, who studies many of the icy objects in the Solar System.
Saturn's rings start just 7,000 km above the surface of the planet, and extend out to an altitude of 80,000 km. But they're gossamer thin, just 10 km across at some points.
We've known about Saturn's rings since 1610, when Galileo was the first person to turn a telescope on them. The resolution was primitive, and he thought he saw "handles" attached to Saturn, or perhaps what were big moons on either side.
In 1659, using a better telescope, the Dutch astronomer Christiaan Huygens figured out that these "handles" were actually rings. And finally in the 1670s, the Italian astronomer Giovanni Cassini was able to resolve the rings in more detail, even observed the biggest gap in the rings.
The Cassini mission, named after Giovanni, has been with Saturn for almost a decade, allowing us to view the rings in incredible detail.
Determining the origin and evolution of Saturn's rings has been one of its objectives.
So far, the argument continues:
Kevin Grazier "There's an age-old debate about whether the rings are old or new. And that goes back and forth - it's been going back and forth for ages and it still goes back and forth. Are they old, or have they been there a long period of time? Are they new? I don't know what to think, to be quite honest. I'm not being wishy-washy, I just don't know what to think anymore."
Evidence from NASA's Voyager spacecraft indicated that the material in Saturn's rings was young.
Perhaps a comet shattered one of Saturn's moons within the last few hundred million years, creating the rings we see today.
If that was the case case, what incredible luck that we're here to see the rings in their current form.
But When Cassini arrived, it showed evidence that Saturn's rings are being refreshed, which could explain why they appear so young.
Perhaps they are ancient after all.
Kevin Grazier "If Saturn's rings are old, a moon could have gotten too close to Saturn and been pulled apart by tidal stresses. There could have been a collision of moons. It could have been a pass by a nearby object, since in the early days of planetary formation, there were many objects zooming past Saturn. Saturn probably had a halo of material in it's early days that was loosely bound to the moon."
There is one ring that we know for certain is being refreshed...
Kevin Grazier "The E-Ring, certainly a new ring, because the E-Ring consists of roughly micron-sized ice particles. And micron-sized ice particles don't last in space. They sputter and sublimate - they go away in very short time periods, and we knew that. And so when we went to Saturn with Cassini, we knew to look for a source of materiel because we knew that the individual components of the E-Ring don't last, so it has to be replenished. So the E-Ring stands alone from the established system, and the E-Ring is absolutely new."
In 2005, scientist discovered that Saturn's E-Ring is being constantly replenished by the moon Enceladus. Cryovolcanoes spew water ice into space from a series of fissures at its south pole.
So where did Saturn's rings come from?
We don't know.
Are the new or old? We don't know.
It just another great mystery of the Solar System.
- published: 19 Dec 2013
- views: 12065
This article is about the Italian-born astronomer. For his French-born great-grandson, see Jean-Dominique Cassini.
Giovanni Domenico Cassini (June 8, 1625 – September 14, 1712) was an Italian/French mathematician, astronomer, engineer, and astrologer. Cassini, also known as Gian Domenico Cassini or Jean-Dominique Cassini, was born in Imperia, near Oneglia, at that time in the Republic of Genova.
Cassini was an astronomer at the Panzano Observatory, from 1648 to 1669. He was a professor of astronomy at the University of Bologna and became, in 1671, director of the Paris Observatory. He thoroughly adopted his new country, to the extent that he became interchangeably known as Jean-Dominique Cassini — although that is also the name of his great-grandson, Dominique, comte de Cassini.
Cassini was the first to observe four of Saturn's moons, which he called Sidera Lodoicea, including Iapetus, whose anomalous variations in brightness he correctly ascribed as being due to the presence of dark material on one hemisphere (now called Cassini regio in his honour). In addition he discovered the Cassini Division in the rings of Saturn (1675). He shares with Robert Hooke credit for the discovery of the Great Red Spot on Jupiter (ca. 1665). Around 1690, Cassini was the first to observe differential rotation within Jupiter's atmosphere.
This page contains text from Wikipedia, the Free Encyclopedia -
http://en.wikipedia.org/wiki/Giovanni_Domenico_Cassini
This article is licensed under the Creative Commons Attribution-ShareAlike 3.0 Unported License, which means that you can copy and modify it as long as the entire work (including additions) remains under this license.
This article is licensed under the Creative Commons Attribution-ShareAlike 3.0 Unported License, which means that you can copy and modify it as long as the entire work (including additions) remains under this license.
Michio Kaku (加来 道雄, Kaku Michio?, born January 24, 1947) is an American theoretical physicist, the Henry Semat Professor of Theoretical Physics in the City College of New York of City University of New York, a co-founder of string field theory, a futurist, and a "communicator" and "popularizer" of science. He has written several books about physics and related topics; he has made frequent appearances on radio, television, and film; and he writes extensive online blogs and articles. He has written two New York Times best sellers, Physics of the Impossible (2008) and Physics of the Future (2011). He has hosted several TV specials for BBC-TV, the Discovery Channel, and the Science Channel.
Kaku was born in San Jose, California to Japanese immigrant parents. His grandfather came to the United States to take part in the clean-up operation after the 1906 San Francisco Earthquake[citation needed]. His father was born in California but was educated in Japan and spoke little English. Both his parents were put in the Tule Lake War Relocation Center, where they met and where his two brothers were born.
This page contains text from Wikipedia, the Free Encyclopedia -
http://en.wikipedia.org/wiki/Michio_Kaku
This article is licensed under the Creative Commons Attribution-ShareAlike 3.0 Unported License, which means that you can copy and modify it as long as the entire work (including additions) remains under this license.
This article is licensed under the Creative Commons Attribution-ShareAlike 3.0 Unported License, which means that you can copy and modify it as long as the entire work (including additions) remains under this license.
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2:04Giovanni Domenico Cassini - Video Learning - WizScience.com
Giovanni Domenico Cassini - Video Learning - WizScience.comGiovanni Domenico Cassini - Video Learning - WizScience.com
"Giovanni" "Domenico Cassini" was an Italian mathematician, astronomer, astrologer and engineer. Cassini was born in Perinaldo, near Imperia, at that time in the County of Nice, part of the Duchy of Savoy. Cassini is known for his work in the fields of astronomy and engineering. Cassini most notably discovered four satellites of the planet Saturn and noted the division of the rings of Saturn . Giovanni Domenico Cassini was also the first of his family to begin work on the project of creating a topographic map of France. Launched in 1997, the Cassini spaceprobe was named after him and became the fourth to visit Saturn and the first to orbit the planet. Cassini was the son of Jacopo Cassini, a Tuscan, and Julia Crovesi. Cassini accepted a position at the observatory at Panzano, near Bologna, to work with Marquis Cornelio Malvasia, a rich amateur astronomer, in 1648 initiating the first part of Cassini's career. During Cassini's time at the Panzano Observatory, Cassini was able to complete his education under the scientists Giovanni Battista Riccioli and Francesco Maria Grimaldi. In 1650 the senate of Bologna appointed Cassini as the principal chair of astronomy at the University of Bologna. In San Petronio, Bologna, he created an important meridian, which helped settle the debate about whether the universe is geocentric. Cassini remained in Bologna working until Colbert recruited him to come to Paris to help set up the Paris Observatory. Cassini departed from Bologna on 25 February 1669. Wiz Science™ is "the" learning channel for children and all ages. SUBSCRIBE TODAY Disclaimer: This video is for your information only. The author or publisher does not guarantee the accuracy of the content presented in this video. USE AT YOUR OWN RISK. Background Music: "The Place Inside" by Silent Partner (royalty-free) from YouTube Audio Library. This video uses material/images from https://en.wikipedia.org/wiki/Giovanni+Domenico+Cassini, which is released under Creative Commons Attribution-Share-Alike License 3.0 http://creativecommons.org/licenses/by-sa/3.0/ . This video is licensed under Creative Commons Attribution-Share-Alike License 3.0 http://creativecommons.org/licenses/by-sa/3.0/ . To reuse/adapt the content in your own work, you must comply with the license terms. -
2:07Giovanni Cassini Interview on "Alex in the AM"
Giovanni Cassini Interview on "Alex in the AM"Giovanni Cassini Interview on "Alex in the AM"
A school video project -
7:35thomas astronomy-Giovanni Cassini
thomas astronomy-Giovanni Cassinithomas astronomy-Giovanni Cassini
astronomy -
54:58Mosaico della bell Italia.Prog 48 .Imagen: Giovanni CAssini,de Durangel,1879
Mosaico della bell Italia.Prog 48 .Imagen: Giovanni CAssini,de Durangel,1879Mosaico della bell Italia.Prog 48 .Imagen: Giovanni CAssini,de Durangel,1879
TEMAS TRATADOS: Giovanni Cassini, astrónomo italiano, las frottolas, capítulo de Il piccolo principe. TEMAS MUSICALES. L'appuntamento, Ornella Vanoni, Zingara, Bobby Solo, Las noches de CAbiria(Nino Rotta), VErgine bella frottola de Bartolomeo Tromboncino, La vida es bella(banda de sonido de la pelicula) La lodoiska, de Giovanni Simone Overture, Obertura de Ermione de Rossini. -
4:11FIND IT SOMEDAY - MEET PROBE CASSINI
FIND IT SOMEDAY - MEET PROBE CASSINIFIND IT SOMEDAY - MEET PROBE CASSINI
SKYVIEWS - FIND IT SOMEDAY - (REPORT BELOW) CASSINI ON HER MISSION TO SATURN MARCH 17, 2014 History of Cassini Probe: Astronomer Giovanni Cassini is associated with a number of scientific discoveries and projects, including the Cassini-Huygens spacecraft that was launched in 1997 and continues to transmit images from Saturn. Born on he was given the name Giovanni Domenico by his parents, Jacopo Cassini and Julia Crovesi. However he also used the name Gian Domenico Cassini, and after he moved to France as an adult, he changed his name to the French version — Jean-Dominique Cassini. To add to the perplexity, he was the first of the well-known Cassini family of astronomers and is sometimes referred to as Cassini I. Astronomer Giovanni Cassini is associated with a number of scientific discoveries and projects, including the Cassini-Huygens spacecraft that was launched in 1997 and continues to transmit images from Saturn. The well-traveled probe won't stop studying Saturn and its many moons anytime soon!!! Cassini has logged more than 3.8 billion miles (6.1 billion kilometers) since its launch on Oct. 15, 1997, researchers said. The nearly 12,600-pound (about 5,700 kilograms) spacecraft was hefted off of Earth on Oct. 15, 1997. It went by Venus in April 1998 and June 1999, Earth in August 1999 and Jupiter in December 2000. Cassini-Huygens is a symbol of the new kind of space exploration and cooperation among different agencies. The spacecraft has spent years circling Saturn and its moons, beaming back pictures and data to teach scientists on Earth more about how the system was formed. The ambitious mission is also a joint one among several space agencies, which is a contrast from the large NASA probes of the past such as Pioneer and Voyager. In this case, the main participants are NASA, the European Space Agency and Agenzia Spaziale Italiana (the Italian space agency). While Cassini was supposed to last four years, it's still going strong at more than double its projected mission lifetime. Since 2004, the Cassini orbiter has studied Saturn and its many natural satellites. Other missions included observing Jupiter, the Heliosphere and testing the theory of relativity. Cassini is the fourth space probe to visit Saturn and the first to enter orbit. It was renamed the Cassini Equinox in 2008 and is currently scheduled to end its mission in 2017. There are also several craters name for Cassini, including an impact crater on the moon that is located in the Palus Nebularum, and a crater on Mars. It regularly passes by the moons of Saturn, producing new data and fueling discoveries back on Earth. NASA's Cassini probe has captured the highest resolution video yet of Saturn's odd, hexagon shaped jet stream that spins around the gas giants north pole. Cassini-Huygens is a symbol of the new kind of space exploration and cooperation among different agencies. The spacecraft has spent years circling Saturn and its moons, beaming back pictures and data to teach scientists on Earth more about how the system was formed. As the probe wandered past Saturn's moons, the findings it brought back to Earth revealed new things about their environments and appearances. On its final orbit In 2017, NASA's Cassini probe will fly between the inner edge of the D ring and the upper atmosphere of the gas giant. It will also fly though an Enceladus plume in the next few years. Some of the more notable findings include: • Finding evidence of liquid water on Enceladus, a frozen moon that shoots out icy jets as it is warped by Saturn's gravity; • Discovering and then pinning down more details about a giant methane lake on Titan; • 50-mile landslides on Iapetus; • A close-up view of Rhea, revealing a pockmarked surface; • A huge ring, 8 million miles away from Saturn, likely made up of debris from Phoebe Credits Photo: Image Credit: Hubble Legacy Archive, NASA, ESA; Processing & Copyright: Davide Coverta Last picture credit: The Antennae Galaxies in Collision Explanation: Two galaxies are squaring off in Corvus and here are the latest pictures. When two galaxies collide, the stars that compose them usually do not. That's because galaxies are mostly empty space and, however bright, stars only take up only a small amount of that space. During the slow, hundred million year collision, one galaxy can still rip the other apart gravitationally, and dust and gas common to both galaxies does collide. In this clash of the titans, dark dust pillars mark massive molecular clouds are being compressed during the galactic encounter, causing the rapid birth of millions of stars, some of which are gravitationally bound together in massive star clusters. Musical Audio: Star and Musical Artist: Derek Clegg - Song: Find it Someday www.derekclegg.com entry submitted by tina marie on March 27, 2014. love and light~tina marie #candotina -
1:02Treasures of the RAS: The woman in the Moon - Cassini's lunar map
Treasures of the RAS: The woman in the Moon - Cassini's lunar mapTreasures of the RAS: The woman in the Moon - Cassini's lunar map
The first scientific map of the Moon, made by Giovanni Cassini in 1679. This detailed engraving of the surface of the Moon was based on Cassini's own observations made with a telescope. The features are an accurate representation of the Moon as Cassini saw it -- apart from a mysterious woman's head, which is hidden among the mountains and craters on the engraving. The Library and Archives of the Royal Astronomical Society contain books, images and documents significant in the development of scientific thought in astronomy, geophysics and related disciplines. In this series of videos RAS Librarian Jenny Higham displays some of the gems of the collection. -
2:33Cassini-Huygens - Saturn HD IMAX footage
Cassini-Huygens - Saturn HD IMAX footageCassini-Huygens - Saturn HD IMAX footage
Updated footage in 4K - http://www.youtube.com/watch?v=QNce_8WHTGc&feature;=share About this footage: "Not-for-profit animated IMAX film in early production by a single filmmaker. Visit the site to make a tax-deductible contribution to support the film. I hope to present this clip at the international IMAX show (GSCA Expo) next month. Visit outsideinthemovie.com/ to donate." About Cassini: Cassini--Huygens is a joint NASA/ESA/ASI robotic spacecraft mission currently studying the planet Saturn and its many natural satellites. The spacecraft consists of two main elements: the NASA-designed and -constructed Cassini orbiter, named for the Italian-French astronomer Giovanni Domenico Cassini, and the ESA-developed Huygens probe, named for the Dutch astronomer, mathematician and physicist Christiaan Huygens. The complete Cassini space probe was launched on October 15, 1997, and after a long interplanetary voyage it entered into orbit around Saturn on July 1, 2004. On December 25, 2004, the Huygens probe was separated from the orbiter at approximately 02:00 UTC. It reached Saturn's moon Titan on January 14, 2005, when it descended into Titan's atmosphere, and downward to the surface, radioing scientific information back to the Earth by telemetry. This was the first landing ever accomplished in the outer solar system. On April 18, 2008, NASA announced a two-year extension of the funding for ground operations of this mission, at which point it was renamed to Cassini Equinox Mission. This was again extended in February 2010 with the mission now continuing until 2017. Cassini is the fourth space probe to visit Saturn and the first to enter orbit. -
5:30Four Bar infinitiy Coupler Curve
Four Bar infinitiy Coupler CurveFour Bar infinitiy Coupler Curve
http://www.mekanizmalar.com/menu_linkage.html This curve known as the lemniscate of Bernoulli. However this curve first investigated by Giovanni Domenico Cassini. Giovanni Cassini was an Italian mathematician and astronomer who studied this curve which is the locus of a point the product of whose distances from two fixed foci is constant. -
1:28Titan Methane Lakes Cassini Flyover 2013 NASA-JPL Animation from Saturn Orbiter; JQ Music
Titan Methane Lakes Cassini Flyover 2013 NASA-JPL Animation from Saturn Orbiter; JQ MusicTitan Methane Lakes Cassini Flyover 2013 NASA-JPL Animation from Saturn Orbiter; JQ Music
more at http://scitech.quickfound.net/astro/planet_news.html Titan: Extraterrestrial Land of Lakes 3-D colorized animated view from the Cassini Saturn orbiter spacecraft of methane lakes on Saturn's moon Titan. The animationa was generated from radar images. Public domain film from NASA-JPL. I have added music created by myself using the Reaper Digital Audio Workstation and the Independence and Proteus VX VST instrument plugins. http://www.jpl.nasa.gov/news/news.php?release=2013-364 NASA's Cassini spacecraft is providing scientists with key clues about Saturn's moon Titan, and in particular, its hydrocarbon lakes and seas. Titan is one of the most Earth-like places in the solar system, and the only place other than our planet that has stable liquid on its surface. Cassini's recent close flybys are bringing into sharper focus a region in Titan's northern hemisphere that sparkles with almost all of the moon's seas and lakes. Scientists working with the spacecraft's radar instrument have put together the most detailed multi-image mosaic of that region to date. The image includes all the seas and most of the major lakes. Some of the flybys tracked over areas that previously were seen at a different angle, so researchers have been able to create a flyover of the area around Titan's largest and second largest seas, known as Kraken Mare and Ligeia Mare, respectively, and some of the nearby lakes... These new images show Kraken Mare is more extensive and complex than previously thought. They also show nearly all of the lakes on Titan fall into an area covering about 600 miles by 1,100 miles (900 kilometers by 1,800 kilometers). Only 3 percent of the liquid at Titan falls outside of this area... http://creativecommons.org/licenses/by-sa/3.0/ http://en.wikipedia.org/wiki/Lakes_of_Titan The lakes of Titan, a moon of Saturn, are bodies of liquid ethane and methane that have been detected by the Cassini--Huygens space probe, and had been suspected long before. The large ones are known as maria (seas) and the small ones as lacūs (lakes). http://en.wikipedia.org/wiki/Cassini--Huygens Cassini--Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-class NASA-ESA-ASI robotic spacecraft sent to the Saturn system. It has studied the planet and its many natural satellites since arriving there in 2004, also observing Jupiter, the heliosphere, and testing the theory of relativity. Launched in 1997 after nearly two decades of development, it includes a Saturn orbiter and an atmospheric probe/lander for the moon Titan called Huygens, which entered and landed on Titan in 2005. Cassini is the fourth space probe to visit Saturn and the first to enter orbit, and its mission is ongoing as of 2013. The two-part spacecraft is named after astronomers Giovanni Cassini and Christiaan Huygens... It launched on October 15, 1997 on a Titan IVB/Centaur and entered into orbit around Saturn on July 1, 2004, after an interplanetary voyage which included flybys of Earth, Venus, and Jupiter. On December 25, 2004, Huygens separated from the orbiter at approximately 02:00 UTC. It reached Saturn's moon Titan on January 14, 2005, when it entered Titan's atmosphere and descended to the surface. It successfully returned data to Earth, using the orbiter as a relay. This was the first landing ever accomplished in the outer Solar System... -
4:09Carolyn Porco speaks about the Cassini-Huygens Mission
Carolyn Porco speaks about the Cassini-Huygens MissionCarolyn Porco speaks about the Cassini-Huygens Mission
CassiniHuygens is a joint NASA/ESA robotic spacecraft mission currently studying the planet Saturn and its moons. The spacecraft consists of two main elements: the NASA Cassini orbiter, named after the Italian-French astronomer Giovanni Domenico Cassini, and the ESA Huygens probe, named after the Dutch astronomer, mathematician and physicist Christiaan Huygens. -
4:59Jápeto
JápetoJápeto
Jápeto Es uno de los satélites del planeta Saturno. Es el octavo más distante al planeta y el tercero en tamaño, con un diámetro de alrededor de 1500 km, después de los satélites más grandes Titán y Rea. Fue descubierto por Giovanni Cassini en 1671. Tarda en completar una vuelta alrededor de Saturno 79,33 días terrestres, a una distancia media de 3 561 300 km. Uno de los hemisferios del satélite es mucho más oscuro que el otro, peculiar característica que se podría deber a una composición distinta del material de la superficie, proveniente del interior de la propia luna o bien de materia de otros satélites o anillos. No se conoce con certeza el motivo real, aunque la segunda hipótesis cada vez es más apoyada por evidencias observacionales. -
4:59Where Did Saturn's Rings Come From?
Where Did Saturn's Rings Come From?Where Did Saturn's Rings Come From?
Saturn's majestic, iconic rings define the planet, but where did they come from? Kevin Grazier "Saturn's rings, good question. And the answer is different depending on which ring we're discussing." That's Dr. Kevin Grazier, a planetary scientist who worked on NASA's Cassini mission or over 15 years, studying Saturn's rings extensively. Mike Brown "Saturn's rings - the strange things about Saturn's rings is that they shouldn't be there, really, in the sense that they don't last for very long. So, if they are just left over from when Saturn was formed, they'd be gone by now. They would slowly work their way into Saturn and burn up and be gone. And yet they're there. So they are either relatively new or somehow continuously regenerated. 'Continuously regenerated' seems strange and 'relatively new' seems also kind of strange. Something broke up - a large moon broke up, or a comet broke up - something had to have happened relatively recently. And by relatively recently, that means hundreds of millions of years ago for someone like me." And that's Mike Brown, professor of planetary geology at Caltech, who studies many of the icy objects in the Solar System. Saturn's rings start just 7,000 km above the surface of the planet, and extend out to an altitude of 80,000 km. But they're gossamer thin, just 10 km across at some points. We've known about Saturn's rings since 1610, when Galileo was the first person to turn a telescope on them. The resolution was primitive, and he thought he saw "handles" attached to Saturn, or perhaps what were big moons on either side. In 1659, using a better telescope, the Dutch astronomer Christiaan Huygens figured out that these "handles" were actually rings. And finally in the 1670s, the Italian astronomer Giovanni Cassini was able to resolve the rings in more detail, even observed the biggest gap in the rings. The Cassini mission, named after Giovanni, has been with Saturn for almost a decade, allowing us to view the rings in incredible detail. Determining the origin and evolution of Saturn's rings has been one of its objectives. So far, the argument continues: Kevin Grazier "There's an age-old debate about whether the rings are old or new. And that goes back and forth - it's been going back and forth for ages and it still goes back and forth. Are they old, or have they been there a long period of time? Are they new? I don't know what to think, to be quite honest. I'm not being wishy-washy, I just don't know what to think anymore." Evidence from NASA's Voyager spacecraft indicated that the material in Saturn's rings was young. Perhaps a comet shattered one of Saturn's moons within the last few hundred million years, creating the rings we see today. If that was the case case, what incredible luck that we're here to see the rings in their current form. But When Cassini arrived, it showed evidence that Saturn's rings are being refreshed, which could explain why they appear so young. Perhaps they are ancient after all. Kevin Grazier "If Saturn's rings are old, a moon could have gotten too close to Saturn and been pulled apart by tidal stresses. There could have been a collision of moons. It could have been a pass by a nearby object, since in the early days of planetary formation, there were many objects zooming past Saturn. Saturn probably had a halo of material in it's early days that was loosely bound to the moon." There is one ring that we know for certain is being refreshed... Kevin Grazier "The E-Ring, certainly a new ring, because the E-Ring consists of roughly micron-sized ice particles. And micron-sized ice particles don't last in space. They sputter and sublimate - they go away in very short time periods, and we knew that. And so when we went to Saturn with Cassini, we knew to look for a source of materiel because we knew that the individual components of the E-Ring don't last, so it has to be replenished. So the E-Ring stands alone from the established system, and the E-Ring is absolutely new." In 2005, scientist discovered that Saturn's E-Ring is being constantly replenished by the moon Enceladus. Cryovolcanoes spew water ice into space from a series of fissures at its south pole. So where did Saturn's rings come from? We don't know. Are the new or old? We don't know. It just another great mystery of the Solar System. -
4:08Cassini Enceladus Flyby & Journey to Mars at IAC on This Week @NASA – October 16, 2015 HD
Cassini Enceladus Flyby & Journey to Mars at IAC on This Week @NASA – October 16, 2015 HDCassini Enceladus Flyby & Journey to Mars at IAC on This Week @NASA – October 16, 2015 HD
more at: http://scitech.quickfound.net/astro/nasa_news.html "Published on Oct 16, 2015 - During meetings and public events at the International Astronautical Congress (IAC), Oct. 12-16 in Jerusalem, NASA Administrator Charlie Bolden and several other NASA officials highlighted the agency’s recently released plan to send astronauts to Mars in the 2030’s. They also emphasized the need for international partnerships and cooperation to make a mission of this magnitude a reality, the importance of harnessing enthusiasm for space exploration and the need to encourage young people to develop the skills we’ll need for the Journey to Mars. Also, New American record in space, Flyby of Saturnian moon, Next launch for Cygnus, Access to space for small satellites and more! JPL Open House is a big draw." Public domain film from NASA. http://creativecommons.org/licenses/by-sa/3.0/ https://en.wikipedia.org/wiki/Enceladus Enceladus (pronounced /ɛnˈsɛlədəs/) is the sixth-largest moon of Saturn. It is only 500 kilometers (310 mi) in diameter, about a tenth of that of Saturn's largest moon, Titan. Enceladus is mostly covered by fresh, clean ice, reflecting almost all the sunlight that strikes it and making its surface temperature at noon reach only −198 °C. Enceladus has a wide range of surface features, ranging from old, heavily cratered regions to young, tectonically deformed terrains that formed as recently as 100 million years ago, despite its small size. Enceladus was discovered in 1789 by William Herschel, but little was known about it until the two Voyager spacecraft passed nearby in the early 1980s. In 2005, the Cassini spacecraft started multiple close flybys of Enceladus, revealing its surface and environment in greater detail. In particular, Cassini discovered a water-rich plume venting from the south polar region of Enceladus. Cryovolcanoes near the south pole shoot geyser-like jets of water vapor, other volatiles, and solid material, including sodium chloride crystals and ice particles, into space, totaling approximately 200 kilograms (440 lb) per second. Over 100 geysers have been identified. Some of the water vapor falls back as "snow"; the rest escapes, and supplies most of the material making up Saturn's E ring. According to NASA scientists, the plumes at Enceladus are similar in composition to comets. In 2014, NASA reported that Cassini found evidence for a large south polar subsurface ocean of liquid water within Enceladus with a thickness of around 10 km. These geyser observations, along with the finding of escaping internal heat and very few (if any) impact craters in the south polar region, show that Enceladus is geologically active today. Enceladus is, like many satellites in the extensive systems of giant planets, trapped in an orbital resonance. Its resonance with Dione excites its orbital eccentricity, which tidal forces damp, resulting in tidal heating of its interior, and offering a possible explanation for the geological activity... https://en.wikipedia.org/wiki/Cassini–Huygens Cassini–Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-class NASA–ESA–ASI robotic spacecraft. Cassini is the fourth space probe to visit Saturn and the first to enter orbit, and its mission is ongoing as of 2015. It has studied the planet and its many natural satellites since arriving there in 2004. Development started in the 1980s. Its design includes a Saturn orbiter, and a lander for the moon Titan. The lander, called Huygens, landed on Titan in 2005. The two-part spacecraft is named after astronomers Giovanni Cassini and Christiaan Huygens. The spacecraft launched on October 15, 1997 aboard a Titan IVB/Centaur and entered orbit around Saturn on July 1, 2004, after an interplanetary voyage that included flybys of Earth, Venus, and Jupiter. On December 25, 2004, Huygens separated from the orbiter and reached Saturn's moon Titan on January 14, 2005. It entered Titan's atmosphere and descended to the surface. It successfully returned data to Earth, using the orbiter as a relay. This was the first landing ever accomplished in the outer Solar System... -
5:25Perinaldo-(LoResMobile) The Village
Perinaldo-(LoResMobile) The VillagePerinaldo-(LoResMobile) The Village
Visit Perinaldo, Italy, a medieval hill village above the Italian Riviera. It's the birthplace of Giovanni Cassini, famous 17th century astronomer. It's also the home of the La Riana Boutique Hotel. This is an authentic hill village, not a spruced-up touristified imitation.
- Aerial telescope
- Alma mater
- Asteroid
- Astrologer
- Astrology
- Astronomer
- Astronomy
- Authority control
- Bibcode
- Bologna
- Cassini Division
- Cassini oval
- Cassini Regio
- Cassini's Laws
- Cassini–Huygens
- Cayenne
- Cornelio Malvasia
- Doctoral advisor
- Edmund F. Robertson
- Engineer
- Engineering
- Ephemeris
- Fibonacci number
- Flood
- Fortification
- France
- French Guiana
- Galileo Galilei
- Gemma Frisius
- Giordano Berti
- Great Red Spot
- Holy Orders
- Iapetus (moon)
- Imperia
- Italian language
- Italy
- Jacques Cassini
- Jean Richer
- Jupiter
- Longitude
- Louis XIV of France
- Machine de Marly
- Mars
- Mathematician
- Mathematics
- Name Authority File
- Natural satellite
- Nicolaus Copernicus
- Oneglia
- Panzano Observatory
- Parallax
- Paris
- Paris Observatory
- Perinaldo
- Po River
- Pope Clement IX
- Professor
- Republic of Genova
- Rings of Saturn
- River management
- Robert Hooke
- Satellite
- Saturn
- Sidera Lodoicea
- Solar system
- Topography
- Triangulation
- Wikipedia Persondata
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Giovanni Domenico Cassini - Video Learning - WizScience.com
"Giovanni" "Domenico Cassini" was an Italian mathematician, astronomer, astrologer and engineer. Cassini was born in Perinaldo, near Imperia, at that time in the County of Nice, part of the Duchy of Savoy. Cassini is known for his work in the fields of astronomy and engineering. Cassini most notably discovered four satellites of the planet Saturn and noted the division of the rings of Saturn . Giovanni Domenico Cassini was also the first of his family to begin work on the project of creating a topographic map of France. Launched in 1997, the Cassini spaceprobe was named after him and became the fourth to visit Saturn and the first to orbit the planet. Cassini was the son of Jacopo Cassini, a Tuscan, and Julia Crovesi. Cassini accepted a position at the observatory at Panzano, near Bo... -
Giovanni Cassini Interview on "Alex in the AM"
A school video project -
thomas astronomy-Giovanni Cassini
astronomy -
Mosaico della bell Italia.Prog 48 .Imagen: Giovanni CAssini,de Durangel,1879
TEMAS TRATADOS: Giovanni Cassini, astrónomo italiano, las frottolas, capítulo de Il piccolo principe. TEMAS MUSICALES. L'appuntamento, Ornella Vanoni, Zingara, Bobby Solo, Las noches de CAbiria(Nino Rotta), VErgine bella frottola de Bartolomeo Tromboncino, La vida es bella(banda de sonido de la pelicula) La lodoiska, de Giovanni Simone Overture, Obertura de Ermione de Rossini. -
FIND IT SOMEDAY - MEET PROBE CASSINI
SKYVIEWS - FIND IT SOMEDAY - (REPORT BELOW) CASSINI ON HER MISSION TO SATURN MARCH 17, 2014 History of Cassini Probe: Astronomer Giovanni Cassini is associated with a number of scientific discoveries and projects, including the Cassini-Huygens spacecraft that was launched in 1997 and continues to transmit images from Saturn. Born on he was given the name Giovanni Domenico by his parents, Jacopo Cassini and Julia Crovesi. However he also used the name Gian Domenico Cassini, and after he moved to France as an adult, he changed his name to the French version — Jean-Dominique Cassini. To add to the perplexity, he was the first of the well-known Cassini family of astronomers and is sometimes referred to as Cassini I. Astronomer Giovanni Cassini is associated with a number of scientific ... -
Treasures of the RAS: The woman in the Moon - Cassini's lunar map
The first scientific map of the Moon, made by Giovanni Cassini in 1679. This detailed engraving of the surface of the Moon was based on Cassini's own observations made with a telescope. The features are an accurate representation of the Moon as Cassini saw it -- apart from a mysterious woman's head, which is hidden among the mountains and craters on the engraving. The Library and Archives of the Royal Astronomical Society contain books, images and documents significant in the development of scientific thought in astronomy, geophysics and related disciplines. In this series of videos RAS Librarian Jenny Higham displays some of the gems of the collection. -
Cassini-Huygens - Saturn HD IMAX footage
Updated footage in 4K - http://www.youtube.com/watch?v=QNce_8WHTGc&feature;=share About this footage: "Not-for-profit animated IMAX film in early production by a single filmmaker. Visit the site to make a tax-deductible contribution to support the film. I hope to present this clip at the international IMAX show (GSCA Expo) next month. Visit outsideinthemovie.com/ to donate." About Cassini: Cassini--Huygens is a joint NASA/ESA/ASI robotic spacecraft mission currently studying the planet Saturn and its many natural satellites. The spacecraft consists of two main elements: the NASA-designed and -constructed Cassini orbiter, named for the Italian-French astronomer Giovanni Domenico Cassini, and the ESA-developed Huygens probe, named for the Dutch astronomer, mathematician and physicist Ch... -
Four Bar infinitiy Coupler Curve
http://www.mekanizmalar.com/menu_linkage.html This curve known as the lemniscate of Bernoulli. However this curve first investigated by Giovanni Domenico Cassini. Giovanni Cassini was an Italian mathematician and astronomer who studied this curve which is the locus of a point the product of whose distances from two fixed foci is constant. -
Titan Methane Lakes Cassini Flyover 2013 NASA-JPL Animation from Saturn Orbiter; JQ Music
more at http://scitech.quickfound.net/astro/planet_news.html Titan: Extraterrestrial Land of Lakes 3-D colorized animated view from the Cassini Saturn orbiter spacecraft of methane lakes on Saturn's moon Titan. The animationa was generated from radar images. Public domain film from NASA-JPL. I have added music created by myself using the Reaper Digital Audio Workstation and the Independence and Proteus VX VST instrument plugins. http://www.jpl.nasa.gov/news/news.php?release=2013-364 NASA's Cassini spacecraft is providing scientists with key clues about Saturn's moon Titan, and in particular, its hydrocarbon lakes and seas. Titan is one of the most Earth-like places in the solar system, and the only place other than our planet that has stable liquid on its surface. Cassini's recent c... -
Carolyn Porco speaks about the Cassini-Huygens Mission
CassiniHuygens is a joint NASA/ESA robotic spacecraft mission currently studying the planet Saturn and its moons. The spacecraft consists of two main elements: the NASA Cassini orbiter, named after the Italian-French astronomer Giovanni Domenico Cassini, and the ESA Huygens probe, named after the Dutch astronomer, mathematician and physicist Christiaan Huygens. -
Jápeto
Jápeto Es uno de los satélites del planeta Saturno. Es el octavo más distante al planeta y el tercero en tamaño, con un diámetro de alrededor de 1500 km, después de los satélites más grandes Titán y Rea. Fue descubierto por Giovanni Cassini en 1671. Tarda en completar una vuelta alrededor de Saturno 79,33 días terrestres, a una distancia media de 3 561 300 km. Uno de los hemisferios del satélite es mucho más oscuro que el otro, peculiar característica que se podría deber a una composición distinta del material de la superficie, proveniente del interior de la propia luna o bien de materia de otros satélites o anillos. No se conoce con certeza el motivo real, aunque la segunda hipótesis cada vez es más apoyada por evidencias observacionales. -
Where Did Saturn's Rings Come From?
Saturn's majestic, iconic rings define the planet, but where did they come from? Kevin Grazier "Saturn's rings, good question. And the answer is different depending on which ring we're discussing." That's Dr. Kevin Grazier, a planetary scientist who worked on NASA's Cassini mission or over 15 years, studying Saturn's rings extensively. Mike Brown "Saturn's rings - the strange things about Saturn's rings is that they shouldn't be there, really, in the sense that they don't last for very long. So, if they are just left over from when Saturn was formed, they'd be gone by now. They would slowly work their way into Saturn and burn up and be gone. And yet they're there. So they are either relatively new or somehow continuously regenerated. 'Continuously regenerated' seems strange and 'relativ... -
Cassini Enceladus Flyby & Journey to Mars at IAC on This Week @NASA – October 16, 2015 HD
more at: http://scitech.quickfound.net/astro/nasa_news.html "Published on Oct 16, 2015 - During meetings and public events at the International Astronautical Congress (IAC), Oct. 12-16 in Jerusalem, NASA Administrator Charlie Bolden and several other NASA officials highlighted the agency’s recently released plan to send astronauts to Mars in the 2030’s. They also emphasized the need for international partnerships and cooperation to make a mission of this magnitude a reality, the importance of harnessing enthusiasm for space exploration and the need to encourage young people to develop the skills we’ll need for the Journey to Mars. Also, New American record in space, Flyby of Saturnian moon, Next launch for Cygnus, Access to space for small satellites and more! JPL Open House is a big draw... -
Perinaldo-(LoResMobile) The Village
Visit Perinaldo, Italy, a medieval hill village above the Italian Riviera. It's the birthplace of Giovanni Cassini, famous 17th century astronomer. It's also the home of the La Riana Boutique Hotel. This is an authentic hill village, not a spruced-up touristified imitation. -
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Cassini's laws
Cassini's laws provide a compact description of the motion of the Moon. They were established in 1693 by Giovanni Domenico Cassini, a prominent scientist of his time. Refinements of these laws to include physical librations have been made, and they have been generalized to treat other satellites and planets. Cassini's laws The Moon has a spin–orbit resonance. This means that the rotation–orbit ratio of the Moon is such that the same side of it always faces the Earth. The Moon's rotational axis maintains a constant angle of inclination from the ecliptic plane. The Moon's rotational axis precesses so as to trace out a cone that intersects the ecliptic plane as a circle. A plane formed from a normal to the ecliptic plane and a normal to the Moon's orbital plane will contain th... -
Cassini's laws
Cassini's laws provide a compact description of the motion of the Moon. They were established in 1693 by Giovanni Domenico Cassini, a prominent scientist of his time. Refinements of these laws to include physical librations have been made, and they have been generalized to treat other satellites and planets -
Clues revealed about hidden interior of Uranus
In 1665, Giovanni Cassini performed the first rotational measurement of a giant planet when he tracked the Great Red Spot on Jupiter. Over the last three and a half centuries, astronomers have pinned down essentially the complete circulation of Jupiter and Saturn and about 75 percent for Uranus and Neptune. Karkoschka's new work fills in the remaining 25 percent for Uranus. - For more information visit : http://www.freedawn.co.uk/scientia/2014/11/14/clues-revealed…rior-of-uranus/ -
Saturn's Moon: Iapetus Rotation
Iapetus (pronounced /aɪˈæpɨtəs/, or as Greek Ιαπετός), occasionally Japetus (pronounced /ˈdʒæpɨtəs/), is the third-largest moon of Saturn, and eleventh in the solar system, Iapetus is best known for its dramatic 'two-tone' coloration, but recent discoveries by the Cassini mission have revealed several other unusual physical characteristics, such as an equatorial ridge that runs about halfway around the moon. Iapetus was discovered by Giovanni Domenico Cassini, an Italian/French astronomer, in October 1671. He had discovered the moon on the western side of Saturn and tried viewing it on the eastern side some months later, but was unsuccessful. The pattern continued the following year as he was able to observe it on the western side, but not the eastern side. Cassini finally observed Iapetu... -
Michio Kaku: Opposition to NASA's Cassini Space Probe (1997)
Cassini--Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-class NASA-ESA-ASI robotic spacecraft sent to the Saturn system. It has studied the planet and its many natural satellites since arriving there in 2004, also observing Jupiter, the heliosphere, and testing the theory of relativity. Launched in 1997 after nearly two decades of development, it includes a Saturn orbiter and an atmospheric probe/lander for the moon Titan called Huygens, which entered and landed on Titan in 2005. Cassini is the fourth space probe to visit Saturn and the first to enter orbit, and its mission is ongoing as of 2014. The two-part spacecraft is named after astronomers Giovanni Cassini and Christiaan Huygens. It launched on October 15, 1997 on a Titan IVB/Centaur and entered into ... -
The mysteries of Iapetus, Saturn's satellite
The mysteries of Iapetus, Saturn's satellite http://www.contactoparanormal.us/2014/04/the-mysteries-of-iapetus-saturns.html Iapetus is the eighth satellite of Saturn and the third largest. The Cassini probe, whose name was chosen to commemorate Giovanni Cassini, astronomer of the seventeenth century, among other achievements, he discovered Saturn's satellites Iapetus, Rhea, Dione and Tethys, came to this satellite in 2004 and provided photographic scenes devoted to Iapetus as the strangest solar system body. English: http://www.contactoparanormal.us/ Spanish: http://www.contactoparanormal.org/ Facebook: https://www.facebook.com/ContactoParanormalCP Twitter: https://twitter.com/ParanormalCP -
How to pronounce Giovanni Domenico Cassini (Italian/Italy) - PronounceNames.com
Audio and video pronunciation of Giovanni Domenico Cassini brought to you by Pronounce Names (http://www.PronounceNames.com), a website dedicated to helping people pronounce names correctly. For more information about this name, such as gender, origin, etc., go to http://www.PronounceNames.com/Giovanni Domenico Cassini -
Perinaldo-(LoResMobile) Nearby Sights
When you visit Perinaldo, Italy, there's plenty to see and do nearby. The village itself is home to La Riana Boutique Hotel, and the birthplace of Giovanni Cassini, the famous 17th century astronomer. Many fascinating villages are nearby and abundant natural beauty surrounds Perinaldo. It's also easy to visit Monaco, San Remo, Nice, and even the Alps.
Giovanni Domenico Cassini - Video Learning - WizScience.com
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- Duration: 2:04
- Updated: 04 Sep 2015
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"Giovanni" "Domenico Cassini" was an Italian mathematician, astronomer, astrologer and engineer. Cassini was born in Perinaldo, near Imperia, at that time in ...
"Giovanni" "Domenico Cassini" was an Italian mathematician, astronomer, astrologer and engineer. Cassini was born in Perinaldo, near Imperia, at that time in the County of Nice, part of the Duchy of Savoy. Cassini is known for his work in the fields of astronomy and engineering. Cassini most notably discovered four satellites of the planet Saturn and noted the division of the rings of Saturn . Giovanni Domenico Cassini was also the first of his family to begin work on the project of creating a topographic map of France. Launched in 1997, the Cassini spaceprobe was named after him and became the fourth to visit Saturn and the first to orbit the planet.
Cassini was the son of Jacopo Cassini, a Tuscan, and Julia Crovesi. Cassini accepted a position at the observatory at Panzano, near Bologna, to work with Marquis Cornelio Malvasia, a rich amateur astronomer, in 1648 initiating the first part of Cassini's career. During Cassini's time at the Panzano Observatory, Cassini was able to complete his education under the scientists Giovanni Battista Riccioli and Francesco Maria Grimaldi. In 1650 the senate of Bologna appointed Cassini as the principal chair of astronomy at the University of Bologna. In San Petronio, Bologna, he created an important meridian, which helped settle the debate about whether the universe is geocentric. Cassini remained in Bologna working until Colbert recruited him to come to Paris to help set up the Paris Observatory. Cassini departed from Bologna on 25 February 1669.
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Background Music:
"The Place Inside" by Silent Partner (royalty-free) from YouTube Audio Library.
This video uses material/images from https://en.wikipedia.org/wiki/Giovanni+Domenico+Cassini, which is released under Creative Commons Attribution-Share-Alike License 3.0 http://creativecommons.org/licenses/by-sa/3.0/ . This video is licensed under Creative Commons Attribution-Share-Alike License 3.0 http://creativecommons.org/licenses/by-sa/3.0/ . To reuse/adapt the content in your own work, you must comply with the license terms.
wn.com/Giovanni Domenico Cassini Video Learning Wizscience.Com
"Giovanni" "Domenico Cassini" was an Italian mathematician, astronomer, astrologer and engineer. Cassini was born in Perinaldo, near Imperia, at that time in the County of Nice, part of the Duchy of Savoy. Cassini is known for his work in the fields of astronomy and engineering. Cassini most notably discovered four satellites of the planet Saturn and noted the division of the rings of Saturn . Giovanni Domenico Cassini was also the first of his family to begin work on the project of creating a topographic map of France. Launched in 1997, the Cassini spaceprobe was named after him and became the fourth to visit Saturn and the first to orbit the planet.
Cassini was the son of Jacopo Cassini, a Tuscan, and Julia Crovesi. Cassini accepted a position at the observatory at Panzano, near Bologna, to work with Marquis Cornelio Malvasia, a rich amateur astronomer, in 1648 initiating the first part of Cassini's career. During Cassini's time at the Panzano Observatory, Cassini was able to complete his education under the scientists Giovanni Battista Riccioli and Francesco Maria Grimaldi. In 1650 the senate of Bologna appointed Cassini as the principal chair of astronomy at the University of Bologna. In San Petronio, Bologna, he created an important meridian, which helped settle the debate about whether the universe is geocentric. Cassini remained in Bologna working until Colbert recruited him to come to Paris to help set up the Paris Observatory. Cassini departed from Bologna on 25 February 1669.
Wiz Science™ is "the" learning channel for children and all ages.
SUBSCRIBE TODAY
Disclaimer: This video is for your information only. The author or publisher does not guarantee the accuracy of the content presented in this video. USE AT YOUR OWN RISK.
Background Music:
"The Place Inside" by Silent Partner (royalty-free) from YouTube Audio Library.
This video uses material/images from https://en.wikipedia.org/wiki/Giovanni+Domenico+Cassini, which is released under Creative Commons Attribution-Share-Alike License 3.0 http://creativecommons.org/licenses/by-sa/3.0/ . This video is licensed under Creative Commons Attribution-Share-Alike License 3.0 http://creativecommons.org/licenses/by-sa/3.0/ . To reuse/adapt the content in your own work, you must comply with the license terms.
- published: 04 Sep 2015
- views: 146
Giovanni Cassini Interview on "Alex in the AM"
- Order: Reorder
- Duration: 2:07
- Updated: 20 Mar 2013
- views: 163
A school video project
A school video project
wn.com/Giovanni Cassini Interview On Alex In The Am
A school video project
- published: 20 Mar 2013
- views: 163
thomas astronomy-Giovanni Cassini
- Order: Reorder
- Duration: 7:35
- Updated: 03 Feb 2008
- views: 348
astronomy
astronomy
wn.com/Thomas Astronomy Giovanni Cassini
astronomy
- published: 03 Feb 2008
- views: 348
Mosaico della bell Italia.Prog 48 .Imagen: Giovanni CAssini,de Durangel,1879
- Order: Reorder
- Duration: 54:58
- Updated: 05 Jan 2015
- views: 49
TEMAS TRATADOS: Giovanni Cassini, astrónomo italiano, las frottolas, capítulo de Il piccolo principe. TEMAS MUSICALES. L'appuntamento, Ornella Vanoni, Zingara, ...
TEMAS TRATADOS: Giovanni Cassini, astrónomo italiano, las frottolas, capítulo de Il piccolo principe. TEMAS MUSICALES. L'appuntamento, Ornella Vanoni, Zingara, Bobby Solo, Las noches de CAbiria(Nino Rotta), VErgine bella frottola de Bartolomeo Tromboncino, La vida es bella(banda de sonido de la pelicula) La lodoiska, de Giovanni Simone Overture, Obertura de Ermione de Rossini.
wn.com/Mosaico Della Bell Italia.Prog 48 .Imagen Giovanni Cassini,De Durangel,1879
TEMAS TRATADOS: Giovanni Cassini, astrónomo italiano, las frottolas, capítulo de Il piccolo principe. TEMAS MUSICALES. L'appuntamento, Ornella Vanoni, Zingara, Bobby Solo, Las noches de CAbiria(Nino Rotta), VErgine bella frottola de Bartolomeo Tromboncino, La vida es bella(banda de sonido de la pelicula) La lodoiska, de Giovanni Simone Overture, Obertura de Ermione de Rossini.
- published: 05 Jan 2015
- views: 49
FIND IT SOMEDAY - MEET PROBE CASSINI
- Order: Reorder
- Duration: 4:11
- Updated: 19 Mar 2014
- views: 374
SKYVIEWS - FIND IT SOMEDAY - (REPORT BELOW)
CASSINI ON HER MISSION TO SATURN
MARCH 17, 2014
History of Cassini Probe:
Astronomer Giovanni Cassini is associa...
SKYVIEWS - FIND IT SOMEDAY - (REPORT BELOW)
CASSINI ON HER MISSION TO SATURN
MARCH 17, 2014
History of Cassini Probe:
Astronomer Giovanni Cassini is associated with a number of scientific discoveries and projects, including the Cassini-Huygens spacecraft that was launched in 1997 and continues to transmit images from Saturn. Born on he was given the name Giovanni Domenico by his parents, Jacopo Cassini and Julia Crovesi.
However he also used the name Gian Domenico Cassini, and after he moved to France as an adult, he changed his name to the French version — Jean-Dominique Cassini. To add to the perplexity, he was the first of the well-known Cassini family of astronomers and is sometimes referred to as Cassini I.
Astronomer Giovanni Cassini is associated with a number of scientific discoveries and projects, including the Cassini-Huygens spacecraft that was launched in 1997 and continues to transmit images from Saturn.
The well-traveled probe won't stop studying Saturn and its many moons anytime soon!!!
Cassini has logged more than 3.8 billion miles (6.1 billion kilometers) since its launch on Oct. 15, 1997, researchers said.
The nearly 12,600-pound (about 5,700 kilograms) spacecraft was hefted off of Earth on Oct. 15, 1997. It went by Venus in April 1998 and June 1999, Earth in August 1999 and Jupiter in December 2000.
Cassini-Huygens is a symbol of the new kind of space exploration and cooperation among different agencies. The spacecraft has spent years circling Saturn and its moons, beaming back pictures and data to teach scientists on Earth more about how the system was formed.
The ambitious mission is also a joint one among several space agencies, which is a contrast from the large NASA probes of the past such as Pioneer and Voyager. In this case, the main participants are NASA, the European Space Agency and Agenzia Spaziale Italiana (the Italian space agency).
While Cassini was supposed to last four years, it's still going strong at more than double its projected mission lifetime.
Since 2004, the Cassini orbiter has studied Saturn and its many natural satellites. Other missions included observing Jupiter, the Heliosphere and testing the theory of relativity. Cassini is the fourth space probe to visit Saturn and the first to enter orbit. It was renamed the Cassini Equinox in 2008 and is currently scheduled to end its mission in 2017.
There are also several craters name for Cassini, including an impact crater on the moon that is located in the Palus Nebularum, and a crater on Mars.
It regularly passes by the moons of Saturn, producing new data and fueling discoveries back on Earth.
NASA's Cassini probe has captured the highest resolution video yet of Saturn's odd, hexagon shaped jet stream that spins around the gas giants north pole.
Cassini-Huygens is a symbol of the new kind of space exploration and cooperation among different agencies. The spacecraft has spent years circling Saturn and its moons, beaming back pictures and data to teach scientists on Earth more about how the system was formed.
As the probe wandered past Saturn's moons, the findings it brought back to Earth revealed new things about their environments and appearances.
On its final orbit In 2017, NASA's Cassini probe will fly between the inner edge of the D ring and the upper atmosphere of the gas giant. It will also fly though an Enceladus plume in the next few years.
Some of the more notable findings include:
• Finding evidence of liquid water on Enceladus, a frozen moon that shoots out icy jets as it is warped by Saturn's gravity;
• Discovering and then pinning down more details about a giant methane lake on Titan;
• 50-mile landslides on Iapetus;
• A close-up view of Rhea, revealing a pockmarked surface;
• A huge ring, 8 million miles away from Saturn, likely made up of debris from Phoebe
Credits Photo: Image Credit: Hubble Legacy Archive, NASA, ESA; Processing & Copyright: Davide Coverta
Last picture credit: The Antennae Galaxies in Collision
Explanation: Two galaxies are squaring off in Corvus and here are the latest pictures. When two galaxies collide, the stars that compose them usually do not. That's because galaxies are mostly empty space and, however bright, stars only take up only a small amount of that space.
During the slow, hundred million year collision, one galaxy can still rip the other apart gravitationally, and dust and gas common to both galaxies does collide. In this clash of the titans, dark dust pillars mark massive molecular clouds are being compressed during the galactic encounter, causing the rapid birth of millions of stars, some of which are gravitationally bound together in massive star clusters.
Musical Audio: Star and Musical Artist: Derek Clegg - Song: Find it Someday www.derekclegg.com
entry submitted by tina marie on March 27, 2014. love and light~tina marie #candotina
wn.com/Find It Someday Meet Probe Cassini
SKYVIEWS - FIND IT SOMEDAY - (REPORT BELOW)
CASSINI ON HER MISSION TO SATURN
MARCH 17, 2014
History of Cassini Probe:
Astronomer Giovanni Cassini is associated with a number of scientific discoveries and projects, including the Cassini-Huygens spacecraft that was launched in 1997 and continues to transmit images from Saturn. Born on he was given the name Giovanni Domenico by his parents, Jacopo Cassini and Julia Crovesi.
However he also used the name Gian Domenico Cassini, and after he moved to France as an adult, he changed his name to the French version — Jean-Dominique Cassini. To add to the perplexity, he was the first of the well-known Cassini family of astronomers and is sometimes referred to as Cassini I.
Astronomer Giovanni Cassini is associated with a number of scientific discoveries and projects, including the Cassini-Huygens spacecraft that was launched in 1997 and continues to transmit images from Saturn.
The well-traveled probe won't stop studying Saturn and its many moons anytime soon!!!
Cassini has logged more than 3.8 billion miles (6.1 billion kilometers) since its launch on Oct. 15, 1997, researchers said.
The nearly 12,600-pound (about 5,700 kilograms) spacecraft was hefted off of Earth on Oct. 15, 1997. It went by Venus in April 1998 and June 1999, Earth in August 1999 and Jupiter in December 2000.
Cassini-Huygens is a symbol of the new kind of space exploration and cooperation among different agencies. The spacecraft has spent years circling Saturn and its moons, beaming back pictures and data to teach scientists on Earth more about how the system was formed.
The ambitious mission is also a joint one among several space agencies, which is a contrast from the large NASA probes of the past such as Pioneer and Voyager. In this case, the main participants are NASA, the European Space Agency and Agenzia Spaziale Italiana (the Italian space agency).
While Cassini was supposed to last four years, it's still going strong at more than double its projected mission lifetime.
Since 2004, the Cassini orbiter has studied Saturn and its many natural satellites. Other missions included observing Jupiter, the Heliosphere and testing the theory of relativity. Cassini is the fourth space probe to visit Saturn and the first to enter orbit. It was renamed the Cassini Equinox in 2008 and is currently scheduled to end its mission in 2017.
There are also several craters name for Cassini, including an impact crater on the moon that is located in the Palus Nebularum, and a crater on Mars.
It regularly passes by the moons of Saturn, producing new data and fueling discoveries back on Earth.
NASA's Cassini probe has captured the highest resolution video yet of Saturn's odd, hexagon shaped jet stream that spins around the gas giants north pole.
Cassini-Huygens is a symbol of the new kind of space exploration and cooperation among different agencies. The spacecraft has spent years circling Saturn and its moons, beaming back pictures and data to teach scientists on Earth more about how the system was formed.
As the probe wandered past Saturn's moons, the findings it brought back to Earth revealed new things about their environments and appearances.
On its final orbit In 2017, NASA's Cassini probe will fly between the inner edge of the D ring and the upper atmosphere of the gas giant. It will also fly though an Enceladus plume in the next few years.
Some of the more notable findings include:
• Finding evidence of liquid water on Enceladus, a frozen moon that shoots out icy jets as it is warped by Saturn's gravity;
• Discovering and then pinning down more details about a giant methane lake on Titan;
• 50-mile landslides on Iapetus;
• A close-up view of Rhea, revealing a pockmarked surface;
• A huge ring, 8 million miles away from Saturn, likely made up of debris from Phoebe
Credits Photo: Image Credit: Hubble Legacy Archive, NASA, ESA; Processing & Copyright: Davide Coverta
Last picture credit: The Antennae Galaxies in Collision
Explanation: Two galaxies are squaring off in Corvus and here are the latest pictures. When two galaxies collide, the stars that compose them usually do not. That's because galaxies are mostly empty space and, however bright, stars only take up only a small amount of that space.
During the slow, hundred million year collision, one galaxy can still rip the other apart gravitationally, and dust and gas common to both galaxies does collide. In this clash of the titans, dark dust pillars mark massive molecular clouds are being compressed during the galactic encounter, causing the rapid birth of millions of stars, some of which are gravitationally bound together in massive star clusters.
Musical Audio: Star and Musical Artist: Derek Clegg - Song: Find it Someday www.derekclegg.com
entry submitted by tina marie on March 27, 2014. love and light~tina marie #candotina
- published: 19 Mar 2014
- views: 374
Treasures of the RAS: The woman in the Moon - Cassini's lunar map
- Order: Reorder
- Duration: 1:02
- Updated: 12 Mar 2014
- views: 499
The first scientific map of the Moon, made by Giovanni Cassini in 1679.
This detailed engraving of the surface of the Moon was based on Cassini's own observati...
The first scientific map of the Moon, made by Giovanni Cassini in 1679.
This detailed engraving of the surface of the Moon was based on Cassini's own observations made with a telescope.
The features are an accurate representation of the Moon as Cassini saw it -- apart from a mysterious woman's head, which is hidden among the mountains and craters on the engraving.
The Library and Archives of the Royal Astronomical Society contain books, images and documents significant in the development of scientific thought in astronomy, geophysics and related disciplines. In this series of videos RAS Librarian Jenny Higham displays some of the gems of the collection.
wn.com/Treasures Of The Ras The Woman In The Moon Cassini's Lunar Map
The first scientific map of the Moon, made by Giovanni Cassini in 1679.
This detailed engraving of the surface of the Moon was based on Cassini's own observations made with a telescope.
The features are an accurate representation of the Moon as Cassini saw it -- apart from a mysterious woman's head, which is hidden among the mountains and craters on the engraving.
The Library and Archives of the Royal Astronomical Society contain books, images and documents significant in the development of scientific thought in astronomy, geophysics and related disciplines. In this series of videos RAS Librarian Jenny Higham displays some of the gems of the collection.
- published: 12 Mar 2014
- views: 499
Cassini-Huygens - Saturn HD IMAX footage
- Order: Reorder
- Duration: 2:33
- Updated: 14 Mar 2011
- views: 69184
Updated footage in 4K - http://www.youtube.com/watch?v=QNce_8WHTGc&feature;=share
About this footage: "Not-for-profit animated IMAX film in early production b...
Updated footage in 4K - http://www.youtube.com/watch?v=QNce_8WHTGc&feature;=share
About this footage: "Not-for-profit animated IMAX film in early production by a single filmmaker. Visit the site to make a tax-deductible contribution to support the film. I hope to present this clip at the international IMAX show (GSCA Expo) next month. Visit outsideinthemovie.com/ to donate."
About Cassini: Cassini--Huygens is a joint NASA/ESA/ASI robotic spacecraft mission currently studying the planet Saturn and its many natural satellites. The spacecraft consists of two main elements: the NASA-designed and -constructed Cassini orbiter, named for the Italian-French astronomer Giovanni Domenico Cassini, and the ESA-developed Huygens probe, named for the Dutch astronomer, mathematician and physicist Christiaan Huygens.
The complete Cassini space probe was launched on October 15, 1997, and after a long interplanetary voyage it entered into orbit around Saturn on July 1, 2004. On December 25, 2004, the Huygens probe was separated from the orbiter at approximately 02:00 UTC. It reached Saturn's moon Titan on January 14, 2005, when it descended into Titan's atmosphere, and downward to the surface, radioing scientific information back to the Earth by telemetry. This was the first landing ever accomplished in the outer solar system. On April 18, 2008, NASA announced a two-year extension of the funding for ground operations of this mission, at which point it was renamed to Cassini Equinox Mission.
This was again extended in February 2010 with the mission now continuing until 2017. Cassini is the fourth space probe to visit Saturn and the first to enter orbit.
wn.com/Cassini Huygens Saturn Hd Imax Footage
Updated footage in 4K - http://www.youtube.com/watch?v=QNce_8WHTGc&feature;=share
About this footage: "Not-for-profit animated IMAX film in early production by a single filmmaker. Visit the site to make a tax-deductible contribution to support the film. I hope to present this clip at the international IMAX show (GSCA Expo) next month. Visit outsideinthemovie.com/ to donate."
About Cassini: Cassini--Huygens is a joint NASA/ESA/ASI robotic spacecraft mission currently studying the planet Saturn and its many natural satellites. The spacecraft consists of two main elements: the NASA-designed and -constructed Cassini orbiter, named for the Italian-French astronomer Giovanni Domenico Cassini, and the ESA-developed Huygens probe, named for the Dutch astronomer, mathematician and physicist Christiaan Huygens.
The complete Cassini space probe was launched on October 15, 1997, and after a long interplanetary voyage it entered into orbit around Saturn on July 1, 2004. On December 25, 2004, the Huygens probe was separated from the orbiter at approximately 02:00 UTC. It reached Saturn's moon Titan on January 14, 2005, when it descended into Titan's atmosphere, and downward to the surface, radioing scientific information back to the Earth by telemetry. This was the first landing ever accomplished in the outer solar system. On April 18, 2008, NASA announced a two-year extension of the funding for ground operations of this mission, at which point it was renamed to Cassini Equinox Mission.
This was again extended in February 2010 with the mission now continuing until 2017. Cassini is the fourth space probe to visit Saturn and the first to enter orbit.
- published: 14 Mar 2011
- views: 69184
Four Bar infinitiy Coupler Curve
- Order: Reorder
- Duration: 5:30
- Updated: 09 Jul 2013
- views: 7129
http://www.mekanizmalar.com/menu_linkage.html
This curve known as the lemniscate of Bernoulli. However this curve first investigated by Giovanni Domenico Cassi...
http://www.mekanizmalar.com/menu_linkage.html
This curve known as the lemniscate of Bernoulli. However this curve first investigated by Giovanni Domenico Cassini. Giovanni Cassini was an Italian mathematician and astronomer who studied this curve which is the locus of a point the product of whose distances from two fixed foci is constant.
wn.com/Four Bar Infinitiy Coupler Curve
http://www.mekanizmalar.com/menu_linkage.html
This curve known as the lemniscate of Bernoulli. However this curve first investigated by Giovanni Domenico Cassini. Giovanni Cassini was an Italian mathematician and astronomer who studied this curve which is the locus of a point the product of whose distances from two fixed foci is constant.
- published: 09 Jul 2013
- views: 7129
Titan Methane Lakes Cassini Flyover 2013 NASA-JPL Animation from Saturn Orbiter; JQ Music
- Order: Reorder
- Duration: 1:28
- Updated: 12 Dec 2013
- views: 8269
more at http://scitech.quickfound.net/astro/planet_news.html
Titan: Extraterrestrial Land of Lakes
3-D colorized animated view from the Cassini Saturn orbiter...
more at http://scitech.quickfound.net/astro/planet_news.html
Titan: Extraterrestrial Land of Lakes
3-D colorized animated view from the Cassini Saturn orbiter spacecraft of methane lakes on Saturn's moon Titan. The animationa was generated from radar images.
Public domain film from NASA-JPL. I have added music created by myself using the Reaper Digital Audio Workstation and the Independence and Proteus VX VST instrument plugins.
http://www.jpl.nasa.gov/news/news.php?release=2013-364
NASA's Cassini spacecraft is providing scientists with key clues about Saturn's moon Titan, and in particular, its hydrocarbon lakes and seas.
Titan is one of the most Earth-like places in the solar system, and the only place other than our planet that has stable liquid on its surface.
Cassini's recent close flybys are bringing into sharper focus a region in Titan's northern hemisphere that sparkles with almost all of the moon's seas and lakes. Scientists working with the spacecraft's radar instrument have put together the most detailed multi-image mosaic of that region to date. The image includes all the seas and most of the major lakes. Some of the flybys tracked over areas that previously were seen at a different angle, so researchers have been able to create a flyover of the area around Titan's largest and second largest seas, known as Kraken Mare and Ligeia Mare, respectively, and some of the nearby lakes...
These new images show Kraken Mare is more extensive and complex than previously thought. They also show nearly all of the lakes on Titan fall into an area covering about 600 miles by 1,100 miles (900 kilometers by 1,800 kilometers). Only 3 percent of the liquid at Titan falls outside of this area...
http://creativecommons.org/licenses/by-sa/3.0/
http://en.wikipedia.org/wiki/Lakes_of_Titan
The lakes of Titan, a moon of Saturn, are bodies of liquid ethane and methane that have been detected by the Cassini--Huygens space probe, and had been suspected long before. The large ones are known as maria (seas) and the small ones as lacūs (lakes).
http://en.wikipedia.org/wiki/Cassini--Huygens
Cassini--Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-class NASA-ESA-ASI robotic spacecraft sent to the Saturn system. It has studied the planet and its many natural satellites since arriving there in 2004, also observing Jupiter, the heliosphere, and testing the theory of relativity. Launched in 1997 after nearly two decades of development, it includes a Saturn orbiter and an atmospheric probe/lander for the moon Titan called Huygens, which entered and landed on Titan in 2005. Cassini is the fourth space probe to visit Saturn and the first to enter orbit, and its mission is ongoing as of 2013. The two-part spacecraft is named after astronomers Giovanni Cassini and Christiaan Huygens...
It launched on October 15, 1997 on a Titan IVB/Centaur and entered into orbit around Saturn on July 1, 2004, after an interplanetary voyage which included flybys of Earth, Venus, and Jupiter. On December 25, 2004, Huygens separated from the orbiter at approximately 02:00 UTC. It reached Saturn's moon Titan on January 14, 2005, when it entered Titan's atmosphere and descended to the surface. It successfully returned data to Earth, using the orbiter as a relay. This was the first landing ever accomplished in the outer Solar System...
wn.com/Titan Methane Lakes Cassini Flyover 2013 Nasa Jpl Animation From Saturn Orbiter Jq Music
more at http://scitech.quickfound.net/astro/planet_news.html
Titan: Extraterrestrial Land of Lakes
3-D colorized animated view from the Cassini Saturn orbiter spacecraft of methane lakes on Saturn's moon Titan. The animationa was generated from radar images.
Public domain film from NASA-JPL. I have added music created by myself using the Reaper Digital Audio Workstation and the Independence and Proteus VX VST instrument plugins.
http://www.jpl.nasa.gov/news/news.php?release=2013-364
NASA's Cassini spacecraft is providing scientists with key clues about Saturn's moon Titan, and in particular, its hydrocarbon lakes and seas.
Titan is one of the most Earth-like places in the solar system, and the only place other than our planet that has stable liquid on its surface.
Cassini's recent close flybys are bringing into sharper focus a region in Titan's northern hemisphere that sparkles with almost all of the moon's seas and lakes. Scientists working with the spacecraft's radar instrument have put together the most detailed multi-image mosaic of that region to date. The image includes all the seas and most of the major lakes. Some of the flybys tracked over areas that previously were seen at a different angle, so researchers have been able to create a flyover of the area around Titan's largest and second largest seas, known as Kraken Mare and Ligeia Mare, respectively, and some of the nearby lakes...
These new images show Kraken Mare is more extensive and complex than previously thought. They also show nearly all of the lakes on Titan fall into an area covering about 600 miles by 1,100 miles (900 kilometers by 1,800 kilometers). Only 3 percent of the liquid at Titan falls outside of this area...
http://creativecommons.org/licenses/by-sa/3.0/
http://en.wikipedia.org/wiki/Lakes_of_Titan
The lakes of Titan, a moon of Saturn, are bodies of liquid ethane and methane that have been detected by the Cassini--Huygens space probe, and had been suspected long before. The large ones are known as maria (seas) and the small ones as lacūs (lakes).
http://en.wikipedia.org/wiki/Cassini--Huygens
Cassini--Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-class NASA-ESA-ASI robotic spacecraft sent to the Saturn system. It has studied the planet and its many natural satellites since arriving there in 2004, also observing Jupiter, the heliosphere, and testing the theory of relativity. Launched in 1997 after nearly two decades of development, it includes a Saturn orbiter and an atmospheric probe/lander for the moon Titan called Huygens, which entered and landed on Titan in 2005. Cassini is the fourth space probe to visit Saturn and the first to enter orbit, and its mission is ongoing as of 2013. The two-part spacecraft is named after astronomers Giovanni Cassini and Christiaan Huygens...
It launched on October 15, 1997 on a Titan IVB/Centaur and entered into orbit around Saturn on July 1, 2004, after an interplanetary voyage which included flybys of Earth, Venus, and Jupiter. On December 25, 2004, Huygens separated from the orbiter at approximately 02:00 UTC. It reached Saturn's moon Titan on January 14, 2005, when it entered Titan's atmosphere and descended to the surface. It successfully returned data to Earth, using the orbiter as a relay. This was the first landing ever accomplished in the outer Solar System...
- published: 12 Dec 2013
- views: 8269
Carolyn Porco speaks about the Cassini-Huygens Mission
- Order: Reorder
- Duration: 4:09
- Updated: 03 Feb 2009
- views: 2957
CassiniHuygens is a joint NASA/ESA robotic spacecraft mission currently studying the planet Saturn and its moons. The spacecraft consists of two main elements: ...
CassiniHuygens is a joint NASA/ESA robotic spacecraft mission currently studying the planet Saturn and its moons. The spacecraft consists of two main elements: the NASA Cassini orbiter, named after the Italian-French astronomer Giovanni Domenico Cassini, and the ESA Huygens probe, named after the Dutch astronomer, mathematician and physicist Christiaan Huygens.
wn.com/Carolyn Porco Speaks About The Cassini Huygens Mission
CassiniHuygens is a joint NASA/ESA robotic spacecraft mission currently studying the planet Saturn and its moons. The spacecraft consists of two main elements: the NASA Cassini orbiter, named after the Italian-French astronomer Giovanni Domenico Cassini, and the ESA Huygens probe, named after the Dutch astronomer, mathematician and physicist Christiaan Huygens.
- published: 03 Feb 2009
- views: 2957
Jápeto
- Order: Reorder
- Duration: 4:59
- Updated: 30 Mar 2016
- views: 4
Jápeto
Es uno de los satélites del planeta Saturno. Es el octavo más distante al planeta y el tercero en tamaño, con un diámetro de alrededor de 1500 km, desp...
Jápeto
Es uno de los satélites del planeta Saturno. Es el octavo más distante al planeta y el tercero en tamaño, con un diámetro de alrededor de 1500 km, después de los satélites más grandes Titán y Rea. Fue descubierto por Giovanni Cassini en 1671. Tarda en completar una vuelta alrededor de Saturno 79,33 días terrestres, a una distancia media de 3 561 300 km.
Uno de los hemisferios del satélite es mucho más oscuro que el otro, peculiar característica que se podría deber a una composición distinta del material de la superficie, proveniente del interior de la propia luna o bien de materia de otros satélites o anillos. No se conoce con certeza el motivo real, aunque la segunda hipótesis cada vez es más apoyada por evidencias observacionales.
wn.com/Jápeto
Jápeto
Es uno de los satélites del planeta Saturno. Es el octavo más distante al planeta y el tercero en tamaño, con un diámetro de alrededor de 1500 km, después de los satélites más grandes Titán y Rea. Fue descubierto por Giovanni Cassini en 1671. Tarda en completar una vuelta alrededor de Saturno 79,33 días terrestres, a una distancia media de 3 561 300 km.
Uno de los hemisferios del satélite es mucho más oscuro que el otro, peculiar característica que se podría deber a una composición distinta del material de la superficie, proveniente del interior de la propia luna o bien de materia de otros satélites o anillos. No se conoce con certeza el motivo real, aunque la segunda hipótesis cada vez es más apoyada por evidencias observacionales.
- published: 30 Mar 2016
- views: 4
Where Did Saturn's Rings Come From?
- Order: Reorder
- Duration: 4:59
- Updated: 19 Dec 2013
- views: 12065
Saturn's majestic, iconic rings define the planet, but where did they come from?
Kevin Grazier "Saturn's rings, good question. And the answer is different depe...
Saturn's majestic, iconic rings define the planet, but where did they come from?
Kevin Grazier "Saturn's rings, good question. And the answer is different depending on which ring we're discussing."
That's Dr. Kevin Grazier, a planetary scientist who worked on NASA's Cassini mission or over 15 years, studying Saturn's rings extensively.
Mike Brown "Saturn's rings - the strange things about Saturn's rings is that they shouldn't be there, really, in the sense that they don't last for very long. So, if they are just left over from when Saturn was formed, they'd be gone by now. They would slowly work their way into Saturn and burn up and be gone. And yet they're there. So they are either relatively new or somehow continuously regenerated. 'Continuously regenerated' seems strange and 'relatively new' seems also kind of strange. Something broke up - a large moon broke up, or a comet broke up - something had to have happened relatively recently. And by relatively recently, that means hundreds of millions of years ago for someone like me."
And that's Mike Brown, professor of planetary geology at Caltech, who studies many of the icy objects in the Solar System.
Saturn's rings start just 7,000 km above the surface of the planet, and extend out to an altitude of 80,000 km. But they're gossamer thin, just 10 km across at some points.
We've known about Saturn's rings since 1610, when Galileo was the first person to turn a telescope on them. The resolution was primitive, and he thought he saw "handles" attached to Saturn, or perhaps what were big moons on either side.
In 1659, using a better telescope, the Dutch astronomer Christiaan Huygens figured out that these "handles" were actually rings. And finally in the 1670s, the Italian astronomer Giovanni Cassini was able to resolve the rings in more detail, even observed the biggest gap in the rings.
The Cassini mission, named after Giovanni, has been with Saturn for almost a decade, allowing us to view the rings in incredible detail.
Determining the origin and evolution of Saturn's rings has been one of its objectives.
So far, the argument continues:
Kevin Grazier "There's an age-old debate about whether the rings are old or new. And that goes back and forth - it's been going back and forth for ages and it still goes back and forth. Are they old, or have they been there a long period of time? Are they new? I don't know what to think, to be quite honest. I'm not being wishy-washy, I just don't know what to think anymore."
Evidence from NASA's Voyager spacecraft indicated that the material in Saturn's rings was young.
Perhaps a comet shattered one of Saturn's moons within the last few hundred million years, creating the rings we see today.
If that was the case case, what incredible luck that we're here to see the rings in their current form.
But When Cassini arrived, it showed evidence that Saturn's rings are being refreshed, which could explain why they appear so young.
Perhaps they are ancient after all.
Kevin Grazier "If Saturn's rings are old, a moon could have gotten too close to Saturn and been pulled apart by tidal stresses. There could have been a collision of moons. It could have been a pass by a nearby object, since in the early days of planetary formation, there were many objects zooming past Saturn. Saturn probably had a halo of material in it's early days that was loosely bound to the moon."
There is one ring that we know for certain is being refreshed...
Kevin Grazier "The E-Ring, certainly a new ring, because the E-Ring consists of roughly micron-sized ice particles. And micron-sized ice particles don't last in space. They sputter and sublimate - they go away in very short time periods, and we knew that. And so when we went to Saturn with Cassini, we knew to look for a source of materiel because we knew that the individual components of the E-Ring don't last, so it has to be replenished. So the E-Ring stands alone from the established system, and the E-Ring is absolutely new."
In 2005, scientist discovered that Saturn's E-Ring is being constantly replenished by the moon Enceladus. Cryovolcanoes spew water ice into space from a series of fissures at its south pole.
So where did Saturn's rings come from?
We don't know.
Are the new or old? We don't know.
It just another great mystery of the Solar System.
wn.com/Where Did Saturn's Rings Come From
Saturn's majestic, iconic rings define the planet, but where did they come from?
Kevin Grazier "Saturn's rings, good question. And the answer is different depending on which ring we're discussing."
That's Dr. Kevin Grazier, a planetary scientist who worked on NASA's Cassini mission or over 15 years, studying Saturn's rings extensively.
Mike Brown "Saturn's rings - the strange things about Saturn's rings is that they shouldn't be there, really, in the sense that they don't last for very long. So, if they are just left over from when Saturn was formed, they'd be gone by now. They would slowly work their way into Saturn and burn up and be gone. And yet they're there. So they are either relatively new or somehow continuously regenerated. 'Continuously regenerated' seems strange and 'relatively new' seems also kind of strange. Something broke up - a large moon broke up, or a comet broke up - something had to have happened relatively recently. And by relatively recently, that means hundreds of millions of years ago for someone like me."
And that's Mike Brown, professor of planetary geology at Caltech, who studies many of the icy objects in the Solar System.
Saturn's rings start just 7,000 km above the surface of the planet, and extend out to an altitude of 80,000 km. But they're gossamer thin, just 10 km across at some points.
We've known about Saturn's rings since 1610, when Galileo was the first person to turn a telescope on them. The resolution was primitive, and he thought he saw "handles" attached to Saturn, or perhaps what were big moons on either side.
In 1659, using a better telescope, the Dutch astronomer Christiaan Huygens figured out that these "handles" were actually rings. And finally in the 1670s, the Italian astronomer Giovanni Cassini was able to resolve the rings in more detail, even observed the biggest gap in the rings.
The Cassini mission, named after Giovanni, has been with Saturn for almost a decade, allowing us to view the rings in incredible detail.
Determining the origin and evolution of Saturn's rings has been one of its objectives.
So far, the argument continues:
Kevin Grazier "There's an age-old debate about whether the rings are old or new. And that goes back and forth - it's been going back and forth for ages and it still goes back and forth. Are they old, or have they been there a long period of time? Are they new? I don't know what to think, to be quite honest. I'm not being wishy-washy, I just don't know what to think anymore."
Evidence from NASA's Voyager spacecraft indicated that the material in Saturn's rings was young.
Perhaps a comet shattered one of Saturn's moons within the last few hundred million years, creating the rings we see today.
If that was the case case, what incredible luck that we're here to see the rings in their current form.
But When Cassini arrived, it showed evidence that Saturn's rings are being refreshed, which could explain why they appear so young.
Perhaps they are ancient after all.
Kevin Grazier "If Saturn's rings are old, a moon could have gotten too close to Saturn and been pulled apart by tidal stresses. There could have been a collision of moons. It could have been a pass by a nearby object, since in the early days of planetary formation, there were many objects zooming past Saturn. Saturn probably had a halo of material in it's early days that was loosely bound to the moon."
There is one ring that we know for certain is being refreshed...
Kevin Grazier "The E-Ring, certainly a new ring, because the E-Ring consists of roughly micron-sized ice particles. And micron-sized ice particles don't last in space. They sputter and sublimate - they go away in very short time periods, and we knew that. And so when we went to Saturn with Cassini, we knew to look for a source of materiel because we knew that the individual components of the E-Ring don't last, so it has to be replenished. So the E-Ring stands alone from the established system, and the E-Ring is absolutely new."
In 2005, scientist discovered that Saturn's E-Ring is being constantly replenished by the moon Enceladus. Cryovolcanoes spew water ice into space from a series of fissures at its south pole.
So where did Saturn's rings come from?
We don't know.
Are the new or old? We don't know.
It just another great mystery of the Solar System.
- published: 19 Dec 2013
- views: 12065
Cassini Enceladus Flyby & Journey to Mars at IAC on This Week @NASA – October 16, 2015 HD
- Order: Reorder
- Duration: 4:08
- Updated: 16 Oct 2015
- views: 431
more at: http://scitech.quickfound.net/astro/nasa_news.html
"Published on Oct 16, 2015 - During meetings and public events at the International Astronautical C...
more at: http://scitech.quickfound.net/astro/nasa_news.html
"Published on Oct 16, 2015 - During meetings and public events at the International Astronautical Congress (IAC), Oct. 12-16 in Jerusalem, NASA Administrator Charlie Bolden and several other NASA officials highlighted the agency’s recently released plan to send astronauts to Mars in the 2030’s. They also emphasized the need for international partnerships and cooperation to make a mission of this magnitude a reality, the importance of harnessing enthusiasm for space exploration and the need to encourage young people to develop the skills we’ll need for the Journey to Mars. Also, New American record in space, Flyby of Saturnian moon, Next launch for Cygnus, Access to space for small satellites and more! JPL Open House is a big draw."
Public domain film from NASA.
http://creativecommons.org/licenses/by-sa/3.0/
https://en.wikipedia.org/wiki/Enceladus
Enceladus (pronounced /ɛnˈsɛlədəs/) is the sixth-largest moon of Saturn. It is only 500 kilometers (310 mi) in diameter, about a tenth of that of Saturn's largest moon, Titan. Enceladus is mostly covered by fresh, clean ice, reflecting almost all the sunlight that strikes it and making its surface temperature at noon reach only −198 °C. Enceladus has a wide range of surface features, ranging from old, heavily cratered regions to young, tectonically deformed terrains that formed as recently as 100 million years ago, despite its small size.
Enceladus was discovered in 1789 by William Herschel, but little was known about it until the two Voyager spacecraft passed nearby in the early 1980s. In 2005, the Cassini spacecraft started multiple close flybys of Enceladus, revealing its surface and environment in greater detail. In particular, Cassini discovered a water-rich plume venting from the south polar region of Enceladus. Cryovolcanoes near the south pole shoot geyser-like jets of water vapor, other volatiles, and solid material, including sodium chloride crystals and ice particles, into space, totaling approximately 200 kilograms (440 lb) per second. Over 100 geysers have been identified. Some of the water vapor falls back as "snow"; the rest escapes, and supplies most of the material making up Saturn's E ring. According to NASA scientists, the plumes at Enceladus are similar in composition to comets. In 2014, NASA reported that Cassini found evidence for a large south polar subsurface ocean of liquid water within Enceladus with a thickness of around 10 km.
These geyser observations, along with the finding of escaping internal heat and very few (if any) impact craters in the south polar region, show that Enceladus is geologically active today. Enceladus is, like many satellites in the extensive systems of giant planets, trapped in an orbital resonance. Its resonance with Dione excites its orbital eccentricity, which tidal forces damp, resulting in tidal heating of its interior, and offering a possible explanation for the geological activity...
https://en.wikipedia.org/wiki/Cassini–Huygens
Cassini–Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-class NASA–ESA–ASI robotic spacecraft. Cassini is the fourth space probe to visit Saturn and the first to enter orbit, and its mission is ongoing as of 2015. It has studied the planet and its many natural satellites since arriving there in 2004.
Development started in the 1980s. Its design includes a Saturn orbiter, and a lander for the moon Titan. The lander, called Huygens, landed on Titan in 2005. The two-part spacecraft is named after astronomers Giovanni Cassini and Christiaan Huygens.
The spacecraft launched on October 15, 1997 aboard a Titan IVB/Centaur and entered orbit around Saturn on July 1, 2004, after an interplanetary voyage that included flybys of Earth, Venus, and Jupiter. On December 25, 2004, Huygens separated from the orbiter and reached Saturn's moon Titan on January 14, 2005. It entered Titan's atmosphere and descended to the surface. It successfully returned data to Earth, using the orbiter as a relay. This was the first landing ever accomplished in the outer Solar System...
wn.com/Cassini Enceladus Flyby Journey To Mars At Iac On This Week Nasa – October 16, 2015 Hd
more at: http://scitech.quickfound.net/astro/nasa_news.html
"Published on Oct 16, 2015 - During meetings and public events at the International Astronautical Congress (IAC), Oct. 12-16 in Jerusalem, NASA Administrator Charlie Bolden and several other NASA officials highlighted the agency’s recently released plan to send astronauts to Mars in the 2030’s. They also emphasized the need for international partnerships and cooperation to make a mission of this magnitude a reality, the importance of harnessing enthusiasm for space exploration and the need to encourage young people to develop the skills we’ll need for the Journey to Mars. Also, New American record in space, Flyby of Saturnian moon, Next launch for Cygnus, Access to space for small satellites and more! JPL Open House is a big draw."
Public domain film from NASA.
http://creativecommons.org/licenses/by-sa/3.0/
https://en.wikipedia.org/wiki/Enceladus
Enceladus (pronounced /ɛnˈsɛlədəs/) is the sixth-largest moon of Saturn. It is only 500 kilometers (310 mi) in diameter, about a tenth of that of Saturn's largest moon, Titan. Enceladus is mostly covered by fresh, clean ice, reflecting almost all the sunlight that strikes it and making its surface temperature at noon reach only −198 °C. Enceladus has a wide range of surface features, ranging from old, heavily cratered regions to young, tectonically deformed terrains that formed as recently as 100 million years ago, despite its small size.
Enceladus was discovered in 1789 by William Herschel, but little was known about it until the two Voyager spacecraft passed nearby in the early 1980s. In 2005, the Cassini spacecraft started multiple close flybys of Enceladus, revealing its surface and environment in greater detail. In particular, Cassini discovered a water-rich plume venting from the south polar region of Enceladus. Cryovolcanoes near the south pole shoot geyser-like jets of water vapor, other volatiles, and solid material, including sodium chloride crystals and ice particles, into space, totaling approximately 200 kilograms (440 lb) per second. Over 100 geysers have been identified. Some of the water vapor falls back as "snow"; the rest escapes, and supplies most of the material making up Saturn's E ring. According to NASA scientists, the plumes at Enceladus are similar in composition to comets. In 2014, NASA reported that Cassini found evidence for a large south polar subsurface ocean of liquid water within Enceladus with a thickness of around 10 km.
These geyser observations, along with the finding of escaping internal heat and very few (if any) impact craters in the south polar region, show that Enceladus is geologically active today. Enceladus is, like many satellites in the extensive systems of giant planets, trapped in an orbital resonance. Its resonance with Dione excites its orbital eccentricity, which tidal forces damp, resulting in tidal heating of its interior, and offering a possible explanation for the geological activity...
https://en.wikipedia.org/wiki/Cassini–Huygens
Cassini–Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-class NASA–ESA–ASI robotic spacecraft. Cassini is the fourth space probe to visit Saturn and the first to enter orbit, and its mission is ongoing as of 2015. It has studied the planet and its many natural satellites since arriving there in 2004.
Development started in the 1980s. Its design includes a Saturn orbiter, and a lander for the moon Titan. The lander, called Huygens, landed on Titan in 2005. The two-part spacecraft is named after astronomers Giovanni Cassini and Christiaan Huygens.
The spacecraft launched on October 15, 1997 aboard a Titan IVB/Centaur and entered orbit around Saturn on July 1, 2004, after an interplanetary voyage that included flybys of Earth, Venus, and Jupiter. On December 25, 2004, Huygens separated from the orbiter and reached Saturn's moon Titan on January 14, 2005. It entered Titan's atmosphere and descended to the surface. It successfully returned data to Earth, using the orbiter as a relay. This was the first landing ever accomplished in the outer Solar System...
- published: 16 Oct 2015
- views: 431
Perinaldo-(LoResMobile) The Village
- Order: Reorder
- Duration: 5:25
- Updated: 16 Jun 2011
- views: 3448
Visit Perinaldo, Italy, a medieval hill village above the Italian Riviera. It's the birthplace of Giovanni Cassini, famous 17th century astronomer. It's also ...
Visit Perinaldo, Italy, a medieval hill village above the Italian Riviera. It's the birthplace of Giovanni Cassini, famous 17th century astronomer. It's also the home of the La Riana Boutique Hotel. This is an authentic hill village, not a spruced-up touristified imitation.
wn.com/Perinaldo (Loresmobile) The Village
Visit Perinaldo, Italy, a medieval hill village above the Italian Riviera. It's the birthplace of Giovanni Cassini, famous 17th century astronomer. It's also the home of the La Riana Boutique Hotel. This is an authentic hill village, not a spruced-up touristified imitation.
- published: 16 Jun 2011
- views: 3448
SP010 - Giovanni Agugiaro - Nowhere EP (Incl Massimo Cassini Remix)
- Order: Reorder
- Duration: 8:01
- Updated: 20 Jan 2016
- views: 88
Cassini's laws
- Order: Reorder
- Duration: 2:35
- Updated: 17 Feb 2016
- views: 2
Cassini's laws provide a compact description of the motion of the Moon. They were established in 1693 by Giovanni Domenico Cassini, a prominent scientist of his...
Cassini's laws provide a compact description of the motion of the Moon. They were established in 1693 by Giovanni Domenico Cassini, a prominent scientist of his time.
Refinements of these laws to include physical librations have been made, and they have been generalized to treat other satellites and planets.
Cassini's laws
The Moon has a spin–orbit resonance. This means that the rotation–orbit ratio of the Moon is such that the same side of it always faces the Earth.
The Moon's rotational axis maintains a constant angle of inclination from the ecliptic plane. The Moon's rotational axis precesses so as to trace out a cone that intersects the ecliptic plane as a circle.
A plane formed from a normal to the ecliptic plane and a normal to the Moon's orbital plane will contain the Moon's rotational axis.
In the case of the Moon, its rotational axis always points some 1.5 degrees away from the North ecliptic pole. The normal to the orbital plane and the rotational axis are always in opposite sides of the normal to the ecliptic.
Therefore, both the normal to the orbital plane and the Moon's rotational axis precess around the Ecliptic pole with the same period. The period is about 18.6 years and the motion is retrograde.
wn.com/Cassini's Laws
Cassini's laws provide a compact description of the motion of the Moon. They were established in 1693 by Giovanni Domenico Cassini, a prominent scientist of his time.
Refinements of these laws to include physical librations have been made, and they have been generalized to treat other satellites and planets.
Cassini's laws
The Moon has a spin–orbit resonance. This means that the rotation–orbit ratio of the Moon is such that the same side of it always faces the Earth.
The Moon's rotational axis maintains a constant angle of inclination from the ecliptic plane. The Moon's rotational axis precesses so as to trace out a cone that intersects the ecliptic plane as a circle.
A plane formed from a normal to the ecliptic plane and a normal to the Moon's orbital plane will contain the Moon's rotational axis.
In the case of the Moon, its rotational axis always points some 1.5 degrees away from the North ecliptic pole. The normal to the orbital plane and the rotational axis are always in opposite sides of the normal to the ecliptic.
Therefore, both the normal to the orbital plane and the Moon's rotational axis precess around the Ecliptic pole with the same period. The period is about 18.6 years and the motion is retrograde.
- published: 17 Feb 2016
- views: 2
Cassini's laws
- Order: Reorder
- Duration: 0:58
- Updated: 29 Jan 2016
- views: 1
Cassini's laws provide a compact description of the motion of the Moon. They were established in 1693 by Giovanni Domenico Cassini, a prominent scientist of his...
Cassini's laws provide a compact description of the motion of the Moon. They were established in 1693 by Giovanni Domenico Cassini, a prominent scientist of his time.
Refinements of these laws to include physical librations have been made, and they have been generalized to treat other satellites and planets
wn.com/Cassini's Laws
Cassini's laws provide a compact description of the motion of the Moon. They were established in 1693 by Giovanni Domenico Cassini, a prominent scientist of his time.
Refinements of these laws to include physical librations have been made, and they have been generalized to treat other satellites and planets
- published: 29 Jan 2016
- views: 1
Clues revealed about hidden interior of Uranus
- Order: Reorder
- Duration: 0:45
- Updated: 14 Nov 2014
- views: 246
In 1665, Giovanni Cassini performed the first rotational measurement of a giant planet when he tracked the Great Red Spot on Jupiter. Over the last three and a ...
In 1665, Giovanni Cassini performed the first rotational measurement of a giant planet when he tracked the Great Red Spot on Jupiter. Over the last three and a half centuries, astronomers have pinned down essentially the complete circulation of Jupiter and Saturn and about 75 percent for Uranus and Neptune. Karkoschka's new work fills in the remaining 25 percent for Uranus. - For more information visit : http://www.freedawn.co.uk/scientia/2014/11/14/clues-revealed…rior-of-uranus/
wn.com/Clues Revealed About Hidden Interior Of Uranus
In 1665, Giovanni Cassini performed the first rotational measurement of a giant planet when he tracked the Great Red Spot on Jupiter. Over the last three and a half centuries, astronomers have pinned down essentially the complete circulation of Jupiter and Saturn and about 75 percent for Uranus and Neptune. Karkoschka's new work fills in the remaining 25 percent for Uranus. - For more information visit : http://www.freedawn.co.uk/scientia/2014/11/14/clues-revealed…rior-of-uranus/
- published: 14 Nov 2014
- views: 246
Saturn's Moon: Iapetus Rotation
- Order: Reorder
- Duration: 1:36
- Updated: 09 Jan 2010
- views: 8854
Iapetus (pronounced /aɪˈæpɨtəs/, or as Greek Ιαπετός), occasionally Japetus (pronounced /ˈdʒæpɨtəs/), is the third-largest moon of Saturn, and eleventh in the s...
Iapetus (pronounced /aɪˈæpɨtəs/, or as Greek Ιαπετός), occasionally Japetus (pronounced /ˈdʒæpɨtəs/), is the third-largest moon of Saturn, and eleventh in the solar system, Iapetus is best known for its dramatic 'two-tone' coloration, but recent discoveries by the Cassini mission have revealed several other unusual physical characteristics, such as an equatorial ridge that runs about halfway around the moon.
Iapetus was discovered by Giovanni Domenico Cassini, an Italian/French astronomer, in October 1671. He had discovered the moon on the western side of Saturn and tried viewing it on the eastern side some months later, but was unsuccessful. The pattern continued the following year as he was able to observe it on the western side, but not the eastern side. Cassini finally observed Iapetus on the eastern side in 1705 with the help of an improved telescope, finding it two magnitudes dimmer on that side.
Cassini correctly surmised that Iapetus has a bright hemisphere and a dark hemisphere, and that it is tidally locked, always keeping the same face towards Saturn. This means that the bright hemisphere is visible from Earth when Iapetus is on the western side of Saturn, and that the dark hemisphere is visible when Iapetus is on the eastern side. The dark hemisphere was later named Cassini Regio in his honour. Iapetus is named after the Titan Iapetus from Greek mythology. In fact, all Saturnian moons are named after Titans. The name was suggested by John Herschel (son of William Herschel, discoverer of Mimas and Enceladus) in his 1847 publication Results of Astronomical Observations made at the Cape of Good Hope, in which he advocated naming the moons of Saturn after the Titans, sisters and brothers of the Titan Cronus (whom the Romans equated with their god Saturn). When first discovered, Iapetus was among four Saturnian moons labelled the Sidera Lodoicea by their discoverer Giovanni Cassini after King Louis XIV (the other three were Tethys, Dione and Rhea). However, astronomers fell into the habit of referring to them using Roman numerals, with Iapetus being Saturn V. Once Mimas and Enceladus were discovered in 1789, the numbering scheme was extended and Iapetus became Saturn VII. And with the discovery of Hyperion in 1848, Iapetus became Saturn VIII, which it is still known by today (see naming of natural satellites). Geological features on Iapetus are named after characters and places from the French epic poem The Song of Roland. Examples of names used include the craters Charlemagne and Baligant, and the northern bright region, Roncevaux Terra. The one exception is Cassini Regio, the dark region of the moon, named after the region's discoverer, Giovanni Cassini. The low density of Iapetus indicates that it is mostly composed of ice, with only a small (~20%) amount of rocky materials.
Unlike most moons, its overall shape is neither spherical nor ellipsoid, but has a bulging waistline and squashed poles; also, its unique equatorial ridge (see below) is so high that it visibly distorts the moon's shape even when viewed from a distance. These features often lead it to be characterized as walnut-shaped.
Iapetus is heavily cratered, and Cassini images have revealed large impact basins in the dark region, at least five of which are over 350 km wide. The largest, Turgis, has a diameter of 580 km; its rim is extremely steep and includes a scarp about 15 km high.
Discovered by G. D. Cassini
Discovery date October 25, 1671
Designations
Alternate name Saturn VIII
Adjective Iapetian, Japetian
Orbital characteristics
Semi-major axis 3 560 820 km
Eccentricity 0.028 612 5
Orbital period 79.321 5 d
Inclination 17.28° (to the ecliptic)
15.47° (to Saturn's equator)
8.13° (to Laplace plane)
Satellite of Saturn
Physical characteristics
Dimensions 1494.8×1424.8 km
Mean radius 735.60 ± 3 km
Surface area 6 700 000 km²
Mass (1.805 635 ± 0.000 375) × 1021 kg
Mean density 1.083 0 ± 0.006 6 g/cm³
Equatorial surface gravity 0.223 m/s2
Escape velocity 0.572 km/s
Rotation period 79.321 5 d
(synchronous)
Axial tilt zero
Albedo 0.05-0.5
Apparent magnitude 10.2-11.9
wn.com/Saturn's Moon Iapetus Rotation
Iapetus (pronounced /aɪˈæpɨtəs/, or as Greek Ιαπετός), occasionally Japetus (pronounced /ˈdʒæpɨtəs/), is the third-largest moon of Saturn, and eleventh in the solar system, Iapetus is best known for its dramatic 'two-tone' coloration, but recent discoveries by the Cassini mission have revealed several other unusual physical characteristics, such as an equatorial ridge that runs about halfway around the moon.
Iapetus was discovered by Giovanni Domenico Cassini, an Italian/French astronomer, in October 1671. He had discovered the moon on the western side of Saturn and tried viewing it on the eastern side some months later, but was unsuccessful. The pattern continued the following year as he was able to observe it on the western side, but not the eastern side. Cassini finally observed Iapetus on the eastern side in 1705 with the help of an improved telescope, finding it two magnitudes dimmer on that side.
Cassini correctly surmised that Iapetus has a bright hemisphere and a dark hemisphere, and that it is tidally locked, always keeping the same face towards Saturn. This means that the bright hemisphere is visible from Earth when Iapetus is on the western side of Saturn, and that the dark hemisphere is visible when Iapetus is on the eastern side. The dark hemisphere was later named Cassini Regio in his honour. Iapetus is named after the Titan Iapetus from Greek mythology. In fact, all Saturnian moons are named after Titans. The name was suggested by John Herschel (son of William Herschel, discoverer of Mimas and Enceladus) in his 1847 publication Results of Astronomical Observations made at the Cape of Good Hope, in which he advocated naming the moons of Saturn after the Titans, sisters and brothers of the Titan Cronus (whom the Romans equated with their god Saturn). When first discovered, Iapetus was among four Saturnian moons labelled the Sidera Lodoicea by their discoverer Giovanni Cassini after King Louis XIV (the other three were Tethys, Dione and Rhea). However, astronomers fell into the habit of referring to them using Roman numerals, with Iapetus being Saturn V. Once Mimas and Enceladus were discovered in 1789, the numbering scheme was extended and Iapetus became Saturn VII. And with the discovery of Hyperion in 1848, Iapetus became Saturn VIII, which it is still known by today (see naming of natural satellites). Geological features on Iapetus are named after characters and places from the French epic poem The Song of Roland. Examples of names used include the craters Charlemagne and Baligant, and the northern bright region, Roncevaux Terra. The one exception is Cassini Regio, the dark region of the moon, named after the region's discoverer, Giovanni Cassini. The low density of Iapetus indicates that it is mostly composed of ice, with only a small (~20%) amount of rocky materials.
Unlike most moons, its overall shape is neither spherical nor ellipsoid, but has a bulging waistline and squashed poles; also, its unique equatorial ridge (see below) is so high that it visibly distorts the moon's shape even when viewed from a distance. These features often lead it to be characterized as walnut-shaped.
Iapetus is heavily cratered, and Cassini images have revealed large impact basins in the dark region, at least five of which are over 350 km wide. The largest, Turgis, has a diameter of 580 km; its rim is extremely steep and includes a scarp about 15 km high.
Discovered by G. D. Cassini
Discovery date October 25, 1671
Designations
Alternate name Saturn VIII
Adjective Iapetian, Japetian
Orbital characteristics
Semi-major axis 3 560 820 km
Eccentricity 0.028 612 5
Orbital period 79.321 5 d
Inclination 17.28° (to the ecliptic)
15.47° (to Saturn's equator)
8.13° (to Laplace plane)
Satellite of Saturn
Physical characteristics
Dimensions 1494.8×1424.8 km
Mean radius 735.60 ± 3 km
Surface area 6 700 000 km²
Mass (1.805 635 ± 0.000 375) × 1021 kg
Mean density 1.083 0 ± 0.006 6 g/cm³
Equatorial surface gravity 0.223 m/s2
Escape velocity 0.572 km/s
Rotation period 79.321 5 d
(synchronous)
Axial tilt zero
Albedo 0.05-0.5
Apparent magnitude 10.2-11.9
- published: 09 Jan 2010
- views: 8854
Michio Kaku: Opposition to NASA's Cassini Space Probe (1997)
- Order: Reorder
- Duration: 69:40
- Updated: 25 Jun 2014
- views: 1464
Cassini--Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-class NASA-ESA-ASI robotic spacecraft sent to the Saturn system. It has s...
Cassini--Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-class NASA-ESA-ASI robotic spacecraft sent to the Saturn system. It has studied the planet and its many natural satellites since arriving there in 2004, also observing Jupiter, the heliosphere, and testing the theory of relativity. Launched in 1997 after nearly two decades of development, it includes a Saturn orbiter and an atmospheric probe/lander for the moon Titan called Huygens, which entered and landed on Titan in 2005. Cassini is the fourth space probe to visit Saturn and the first to enter orbit, and its mission is ongoing as of 2014. The two-part spacecraft is named after astronomers Giovanni Cassini and Christiaan Huygens.
It launched on October 15, 1997 on a Titan IVB/Centaur and entered into orbit around Saturn on July 1, 2004, after an interplanetary voyage which included flybys of Earth, Venus, and Jupiter. On December 25, 2004, Huygens separated from the orbiter at approximately 02:00 UTC. It reached Saturn's moon Titan on January 14, 2005, when it entered Titan's atmosphere and descended to the surface. It successfully returned data to Earth, using the orbiter as a relay. This was the first landing ever accomplished in the outer Solar System.
On April 3, 2014, NASA reported that evidence for a large underground ocean of liquid water on Enceladus, a moon of Saturn, had been found by Cassini. According to the scientists, evidence of an underground ocean suggests that Enceladus is one of the most likely places in the solar system to "host microbial life."
Sixteen European countries and the United States make up the team responsible for designing, building, flying and collecting data from the Cassini orbiter and Huygens probe. The mission is managed by NASA's Jet Propulsion Laboratory in the United States, where the orbiter was assembled. Huygens was developed by the European Space Research and Technology Centre. The Centre's prime contractor, Aérospatiale of France (now Thales Alenia Space), assembled the probe with equipment and instruments supplied by many European countries (Huygens' batteries and two scientific instruments by the United States). The Italian Space Agency (ASI) provided the Cassini orbiter's high-gain radio antenna, with the incorporation of a low-gain antenna (that ensure telecommunications with the Earth for the entire duration of the mission), a compact and lightweight radar, which also uses the high-gain antenna and serves as a synthetic aperture radar, a radar altimeter, a radiometer, the radio science subsystem (RSS), the visible channel portion VIMS-V of VIMS spectrometer (the VIMS-IR counterpart was provided by NASA, as well as Main Electronic Assembly, which includes electronic subassemblies provided by CNES of France).
On April 16, 2008, NASA announced a two-year extension of the funding for ground operations of this mission, at which point it was renamed to the Cassini Equinox Mission. This was again extended in February 2010 with the Cassini Solstice Mission.
http://en.wikipedia.org/wiki/Cassini_space_probe
wn.com/Michio Kaku Opposition To Nasa's Cassini Space Probe (1997)
Cassini--Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-class NASA-ESA-ASI robotic spacecraft sent to the Saturn system. It has studied the planet and its many natural satellites since arriving there in 2004, also observing Jupiter, the heliosphere, and testing the theory of relativity. Launched in 1997 after nearly two decades of development, it includes a Saturn orbiter and an atmospheric probe/lander for the moon Titan called Huygens, which entered and landed on Titan in 2005. Cassini is the fourth space probe to visit Saturn and the first to enter orbit, and its mission is ongoing as of 2014. The two-part spacecraft is named after astronomers Giovanni Cassini and Christiaan Huygens.
It launched on October 15, 1997 on a Titan IVB/Centaur and entered into orbit around Saturn on July 1, 2004, after an interplanetary voyage which included flybys of Earth, Venus, and Jupiter. On December 25, 2004, Huygens separated from the orbiter at approximately 02:00 UTC. It reached Saturn's moon Titan on January 14, 2005, when it entered Titan's atmosphere and descended to the surface. It successfully returned data to Earth, using the orbiter as a relay. This was the first landing ever accomplished in the outer Solar System.
On April 3, 2014, NASA reported that evidence for a large underground ocean of liquid water on Enceladus, a moon of Saturn, had been found by Cassini. According to the scientists, evidence of an underground ocean suggests that Enceladus is one of the most likely places in the solar system to "host microbial life."
Sixteen European countries and the United States make up the team responsible for designing, building, flying and collecting data from the Cassini orbiter and Huygens probe. The mission is managed by NASA's Jet Propulsion Laboratory in the United States, where the orbiter was assembled. Huygens was developed by the European Space Research and Technology Centre. The Centre's prime contractor, Aérospatiale of France (now Thales Alenia Space), assembled the probe with equipment and instruments supplied by many European countries (Huygens' batteries and two scientific instruments by the United States). The Italian Space Agency (ASI) provided the Cassini orbiter's high-gain radio antenna, with the incorporation of a low-gain antenna (that ensure telecommunications with the Earth for the entire duration of the mission), a compact and lightweight radar, which also uses the high-gain antenna and serves as a synthetic aperture radar, a radar altimeter, a radiometer, the radio science subsystem (RSS), the visible channel portion VIMS-V of VIMS spectrometer (the VIMS-IR counterpart was provided by NASA, as well as Main Electronic Assembly, which includes electronic subassemblies provided by CNES of France).
On April 16, 2008, NASA announced a two-year extension of the funding for ground operations of this mission, at which point it was renamed to the Cassini Equinox Mission. This was again extended in February 2010 with the Cassini Solstice Mission.
http://en.wikipedia.org/wiki/Cassini_space_probe
- published: 25 Jun 2014
- views: 1464
The mysteries of Iapetus, Saturn's satellite
- Order: Reorder
- Duration: 0:15
- Updated: 01 May 2014
- views: 116
The mysteries of Iapetus, Saturn's satellite
http://www.contactoparanormal.us/2014/04/the-mysteries-of-iapetus-saturns.html
Iapetus is the eighth satellite of...
The mysteries of Iapetus, Saturn's satellite
http://www.contactoparanormal.us/2014/04/the-mysteries-of-iapetus-saturns.html
Iapetus is the eighth satellite of Saturn and the third largest. The Cassini probe, whose name was chosen to commemorate Giovanni Cassini, astronomer of the seventeenth century, among other achievements, he discovered Saturn's satellites Iapetus, Rhea, Dione and Tethys, came to this satellite in 2004 and provided photographic scenes devoted to Iapetus as the strangest solar system body.
English: http://www.contactoparanormal.us/
Spanish: http://www.contactoparanormal.org/
Facebook: https://www.facebook.com/ContactoParanormalCP
Twitter: https://twitter.com/ParanormalCP
wn.com/The Mysteries Of Iapetus, Saturn's Satellite
The mysteries of Iapetus, Saturn's satellite
http://www.contactoparanormal.us/2014/04/the-mysteries-of-iapetus-saturns.html
Iapetus is the eighth satellite of Saturn and the third largest. The Cassini probe, whose name was chosen to commemorate Giovanni Cassini, astronomer of the seventeenth century, among other achievements, he discovered Saturn's satellites Iapetus, Rhea, Dione and Tethys, came to this satellite in 2004 and provided photographic scenes devoted to Iapetus as the strangest solar system body.
English: http://www.contactoparanormal.us/
Spanish: http://www.contactoparanormal.org/
Facebook: https://www.facebook.com/ContactoParanormalCP
Twitter: https://twitter.com/ParanormalCP
- published: 01 May 2014
- views: 116
How to pronounce Giovanni Domenico Cassini (Italian/Italy) - PronounceNames.com
- Order: Reorder
- Duration: 0:28
- Updated: 07 Feb 2014
- views: 122
Audio and video pronunciation of Giovanni Domenico Cassini brought to you by Pronounce Names (http://www.PronounceNames.com), a website dedicated to helping peo...
Audio and video pronunciation of Giovanni Domenico Cassini brought to you by Pronounce Names (http://www.PronounceNames.com), a website dedicated to helping people pronounce names correctly. For more information about this name, such as gender, origin, etc., go to http://www.PronounceNames.com/Giovanni Domenico Cassini
wn.com/How To Pronounce Giovanni Domenico Cassini (Italian Italy) Pronouncenames.Com
Audio and video pronunciation of Giovanni Domenico Cassini brought to you by Pronounce Names (http://www.PronounceNames.com), a website dedicated to helping people pronounce names correctly. For more information about this name, such as gender, origin, etc., go to http://www.PronounceNames.com/Giovanni Domenico Cassini
- published: 07 Feb 2014
- views: 122
Perinaldo-(LoResMobile) Nearby Sights
- Order: Reorder
- Duration: 4:07
- Updated: 22 Dec 2013
- views: 61
When you visit Perinaldo, Italy, there's plenty to see and do nearby. The village itself is home to La Riana Boutique Hotel, and the birthplace of Giovanni Cas...
When you visit Perinaldo, Italy, there's plenty to see and do nearby. The village itself is home to La Riana Boutique Hotel, and the birthplace of Giovanni Cassini, the famous 17th century astronomer. Many fascinating villages are nearby and abundant natural beauty surrounds Perinaldo. It's also easy to visit Monaco, San Remo, Nice, and even the Alps.
wn.com/Perinaldo (Loresmobile) Nearby Sights
When you visit Perinaldo, Italy, there's plenty to see and do nearby. The village itself is home to La Riana Boutique Hotel, and the birthplace of Giovanni Cassini, the famous 17th century astronomer. Many fascinating villages are nearby and abundant natural beauty surrounds Perinaldo. It's also easy to visit Monaco, San Remo, Nice, and even the Alps.
- published: 22 Dec 2013
- views: 61
-
Sun and Earth Distance in Hanuman Chalisa
Distance between Sun and Earth is given in Hindu Prayer Hanuman Chalisa. Hanuman challisa was written by Goswami Tulasidas in Awadhi language who belongs to 15th century. According to Records, For the first time in the year of 1672, Jean Richer and Giovanni Domenico Cassini measured the distance between Earth and Sun. The distance between Sun and earth in Hanuman Chalisa has been calculated much more accurately than the 17th century scientists even before two centuries. -
Giovanni Monti Interview - Ciao Radio - 14 May 2014
Giovanni Monti interview @ Ciao Radio - 14 May 2014 in studio: Tony Farietti dj - Toz Antonio Piretti -
Cassini–Huygens
Cassini–Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-class NASA-ESA-ASI robotic spacecraft sent to the Saturn system. It has studied the planet and its many natural satellites since arriving there in 2004, also observing Jupiter, the heliosphere, and testing the theory of relativity. Launched in 1997 after nearly two decades of development, it includes a Saturn orbiter and an atmospheric probe/lander for the moon Titan called Huygens, which entered and landed on Titan in 2005. Cassini is the fourth space probe to visit Saturn and the first to enter orbit, and its mission is ongoing as of 2014. The two-part spacecraft is named after astronomers Giovanni Cassini and Christiaan Huygens. The spacecraft launched on October 15, 1997 aboard a Titan IVB/Centaur and... -
EGU2014: Jean Dominique Cassini Medal Lecture by Stamatios M. Krimigis (ML3)
Medal Lecture at the 2014 General Assembly of the European Geosciences Union, which took place in Vienna from 27 April to 2 May 2014. Session details: http://meetingorganizer.copernicus.org/EGU2014/session/16243 (Credit: EGU) The European Geosciences Union (http://www.egu.eu) is Europe’s premier geosciences union, dedicated to the pursuit of excellence in the Earth, planetary, and space sciences for the benefit of humanity, worldwide. It is a non-profit interdisciplinary learned association of scientists founded in 2002. The EGU has a current portfolio of 16 diverse scientific journals, which use an innovative open access format, and organises a number of topical meetings, and education and outreach activities. Its annual General Assembly is the largest and most prominent European geoscie... -
Zum Verkaufen: Stadthaus im historischen ligurischen Bergdorf Perinaldo
Dieses schöne Haus liegt im Zentrum des mittelalterlichen Ortes und wird zur Zeit als Studio genutzt. Die Gesamtfläche ist 192 qm. Die Eingangsetage ist renoviert und hat eine Fläche von 120 qm. es gibt 2 Räume mit Balkonen, 1 x mit Lage zur Via Maraldi. Der größere Balkon ist an der Seite mit Blick in die Alpen. Einige Räume haben sehr schöne Kreuzgewölbe. Der Keller, mit historischen Gewölben, ist 72 qm groß und muss noch renoviert werden. Es gibt im Keller 2 Räume mit großen Fenstern und Blick in die Alpen. Das Haus kann direkt mit dem Auto angefahren werden und hat auch eine Garage für ein kleineres Auto. Insgesamt kann das Anwesen als Wohnhaus, Ristorante (da gibt es bereits Pläne) und/oder Studio genutzt werden. -
Hotel La Riana, Perinaldo (Hotel for sale or to rent)
11 rooms (3 single rooms, 2 double rooms on the village site, 6 double rooms to the seasite with balcony, 2 terasses with view to the sea, parking place, large room for events, Kitchen, several storage rooms -
Perinaldo ( Im )
Immagini di Roberto Fadda -
Sun and Earth Distance in Hanuman Chalisa
- Order: Reorder
- Duration: 2:39
- Updated: 14 Nov 2014
- views: 4741
Distance between Sun and Earth is given in Hindu Prayer Hanuman Chalisa. Hanuman challisa was written by Goswami Tulasidas in Awadhi language who belongs to 15t...
Distance between Sun and Earth is given in Hindu Prayer Hanuman Chalisa. Hanuman challisa was written by Goswami Tulasidas in Awadhi language who belongs to 15th century. According to Records, For the first time in the year of 1672, Jean Richer and Giovanni Domenico Cassini measured the distance between Earth and Sun. The distance between Sun and earth in Hanuman Chalisa has been calculated much more accurately than the 17th century scientists even before two centuries.
wn.com/Sun And Earth Distance In Hanuman Chalisa
Distance between Sun and Earth is given in Hindu Prayer Hanuman Chalisa. Hanuman challisa was written by Goswami Tulasidas in Awadhi language who belongs to 15th century. According to Records, For the first time in the year of 1672, Jean Richer and Giovanni Domenico Cassini measured the distance between Earth and Sun. The distance between Sun and earth in Hanuman Chalisa has been calculated much more accurately than the 17th century scientists even before two centuries.
- published: 14 Nov 2014
- views: 4741
Giovanni Monti Interview - Ciao Radio - 14 May 2014
- Order: Reorder
- Duration: 3:57
- Updated: 15 May 2014
- views: 12
Giovanni Monti interview
@ Ciao Radio - 14 May 2014
in studio: Tony Farietti dj - Toz Antonio Piretti
Giovanni Monti interview
@ Ciao Radio - 14 May 2014
in studio: Tony Farietti dj - Toz Antonio Piretti
wn.com/Giovanni Monti Interview Ciao Radio 14 May 2014
Giovanni Monti interview
@ Ciao Radio - 14 May 2014
in studio: Tony Farietti dj - Toz Antonio Piretti
- published: 15 May 2014
- views: 12
Cassini–Huygens
- Order: Reorder
- Duration: 45:40
- Updated: 04 Aug 2014
- views: 192
Cassini–Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-class NASA-ESA-ASI robotic spacecraft sent to the Saturn system. It has st...
Cassini–Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-class NASA-ESA-ASI robotic spacecraft sent to the Saturn system. It has studied the planet and its many natural satellites since arriving there in 2004, also observing Jupiter, the heliosphere, and testing the theory of relativity. Launched in 1997 after nearly two decades of development, it includes a Saturn orbiter and an atmospheric probe/lander for the moon Titan called Huygens, which entered and landed on Titan in 2005. Cassini is the fourth space probe to visit Saturn and the first to enter orbit, and its mission is ongoing as of 2014. The two-part spacecraft is named after astronomers Giovanni Cassini and Christiaan Huygens.
The spacecraft launched on October 15, 1997 aboard a Titan IVB/Centaur and entered orbit around Saturn on July 1, 2004, after an interplanetary voyage which included flybys of Earth, Venus, and Jupiter. On December 25, 2004, Huygens separated from the orbiter at approximately 02:00 UTC. It reached Saturn's moon Titan on January 14, 2005, when it entered Titan's atmosphere and descended to the surface. It successfully returned data to Earth, using the orbiter as a relay. This was the first landing ever accomplished in the outer Solar System.
This video is targeted to blind users.
Attribution:
Article text available under CC-BY-SA
Creative Commons image source in video
wn.com/Cassini–Huygens
Cassini–Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-class NASA-ESA-ASI robotic spacecraft sent to the Saturn system. It has studied the planet and its many natural satellites since arriving there in 2004, also observing Jupiter, the heliosphere, and testing the theory of relativity. Launched in 1997 after nearly two decades of development, it includes a Saturn orbiter and an atmospheric probe/lander for the moon Titan called Huygens, which entered and landed on Titan in 2005. Cassini is the fourth space probe to visit Saturn and the first to enter orbit, and its mission is ongoing as of 2014. The two-part spacecraft is named after astronomers Giovanni Cassini and Christiaan Huygens.
The spacecraft launched on October 15, 1997 aboard a Titan IVB/Centaur and entered orbit around Saturn on July 1, 2004, after an interplanetary voyage which included flybys of Earth, Venus, and Jupiter. On December 25, 2004, Huygens separated from the orbiter at approximately 02:00 UTC. It reached Saturn's moon Titan on January 14, 2005, when it entered Titan's atmosphere and descended to the surface. It successfully returned data to Earth, using the orbiter as a relay. This was the first landing ever accomplished in the outer Solar System.
This video is targeted to blind users.
Attribution:
Article text available under CC-BY-SA
Creative Commons image source in video
- published: 04 Aug 2014
- views: 192
EGU2014: Jean Dominique Cassini Medal Lecture by Stamatios M. Krimigis (ML3)
- Order: Reorder
- Duration: 50:15
- Updated: 03 Feb 2015
- views: 27
Medal Lecture at the 2014 General Assembly of the European Geosciences Union, which took place in Vienna from 27 April to 2 May 2014. Session details: http://me...
Medal Lecture at the 2014 General Assembly of the European Geosciences Union, which took place in Vienna from 27 April to 2 May 2014. Session details: http://meetingorganizer.copernicus.org/EGU2014/session/16243 (Credit: EGU)
The European Geosciences Union (http://www.egu.eu) is Europe’s premier geosciences union, dedicated to the pursuit of excellence in the Earth, planetary, and space sciences for the benefit of humanity, worldwide. It is a non-profit interdisciplinary learned association of scientists founded in 2002. The EGU has a current portfolio of 16 diverse scientific journals, which use an innovative open access format, and organises a number of topical meetings, and education and outreach activities. Its annual General Assembly is the largest and most prominent European geosciences event, attracting over 12,000 scientists from all over the world. The meeting’s sessions cover a wide range of topics, including volcanology, planetary exploration, the Earth’s internal structure and atmosphere, climate, energy, and resources. The EGU 2015 General Assembly is taking place in Vienna, Austria, from 12 to 17 April 2015.
wn.com/Egu2014 Jean Dominique Cassini Medal Lecture By Stamatios M. Krimigis (Ml3)
Medal Lecture at the 2014 General Assembly of the European Geosciences Union, which took place in Vienna from 27 April to 2 May 2014. Session details: http://meetingorganizer.copernicus.org/EGU2014/session/16243 (Credit: EGU)
The European Geosciences Union (http://www.egu.eu) is Europe’s premier geosciences union, dedicated to the pursuit of excellence in the Earth, planetary, and space sciences for the benefit of humanity, worldwide. It is a non-profit interdisciplinary learned association of scientists founded in 2002. The EGU has a current portfolio of 16 diverse scientific journals, which use an innovative open access format, and organises a number of topical meetings, and education and outreach activities. Its annual General Assembly is the largest and most prominent European geosciences event, attracting over 12,000 scientists from all over the world. The meeting’s sessions cover a wide range of topics, including volcanology, planetary exploration, the Earth’s internal structure and atmosphere, climate, energy, and resources. The EGU 2015 General Assembly is taking place in Vienna, Austria, from 12 to 17 April 2015.
- published: 03 Feb 2015
- views: 27
Zum Verkaufen: Stadthaus im historischen ligurischen Bergdorf Perinaldo
- Order: Reorder
- Duration: 6:15
- Updated: 28 Jun 2015
- views: 52
Dieses schöne Haus liegt im Zentrum des mittelalterlichen Ortes und wird zur Zeit als Studio genutzt. Die Gesamtfläche ist 192 qm. Die Eingangsetage ist renovie...
Dieses schöne Haus liegt im Zentrum des mittelalterlichen Ortes und wird zur Zeit als Studio genutzt. Die Gesamtfläche ist 192 qm. Die Eingangsetage ist renoviert und hat eine Fläche von 120 qm. es gibt 2 Räume mit Balkonen, 1 x mit Lage zur Via Maraldi. Der größere Balkon ist an der Seite mit Blick in die Alpen. Einige Räume haben sehr schöne Kreuzgewölbe. Der Keller, mit historischen Gewölben, ist 72 qm groß und muss noch renoviert werden. Es gibt im Keller 2 Räume mit großen Fenstern und Blick in die Alpen. Das Haus kann direkt mit dem Auto angefahren werden und hat auch eine Garage für ein kleineres Auto. Insgesamt kann das Anwesen als Wohnhaus, Ristorante (da gibt es bereits Pläne) und/oder Studio genutzt werden.
wn.com/Zum Verkaufen Stadthaus Im Historischen Ligurischen Bergdorf Perinaldo
Dieses schöne Haus liegt im Zentrum des mittelalterlichen Ortes und wird zur Zeit als Studio genutzt. Die Gesamtfläche ist 192 qm. Die Eingangsetage ist renoviert und hat eine Fläche von 120 qm. es gibt 2 Räume mit Balkonen, 1 x mit Lage zur Via Maraldi. Der größere Balkon ist an der Seite mit Blick in die Alpen. Einige Räume haben sehr schöne Kreuzgewölbe. Der Keller, mit historischen Gewölben, ist 72 qm groß und muss noch renoviert werden. Es gibt im Keller 2 Räume mit großen Fenstern und Blick in die Alpen. Das Haus kann direkt mit dem Auto angefahren werden und hat auch eine Garage für ein kleineres Auto. Insgesamt kann das Anwesen als Wohnhaus, Ristorante (da gibt es bereits Pläne) und/oder Studio genutzt werden.
- published: 28 Jun 2015
- views: 52
Hotel La Riana, Perinaldo (Hotel for sale or to rent)
- Order: Reorder
- Duration: 10:10
- Updated: 18 Jul 2015
- views: 140
11 rooms (3 single rooms, 2 double rooms on the village site, 6 double rooms to the seasite with balcony, 2 terasses with view to the sea, parking place, large ...
11 rooms (3 single rooms, 2 double rooms on the village site, 6 double rooms to the seasite with balcony, 2 terasses with view to the sea, parking place, large room for events, Kitchen, several storage rooms
wn.com/Hotel La Riana, Perinaldo (Hotel For Sale Or To Rent)
11 rooms (3 single rooms, 2 double rooms on the village site, 6 double rooms to the seasite with balcony, 2 terasses with view to the sea, parking place, large room for events, Kitchen, several storage rooms
- published: 18 Jul 2015
- views: 140
Perinaldo ( Im )
- Order: Reorder
- Duration: 9:25
- Updated: 26 Sep 2015
- views: 35
Immagini di Roberto Fadda
Immagini di Roberto Fadda
wn.com/Perinaldo ( Im )
SOLD: Elazaro (King Kolibri x Voltaire)
- Order: Reorder
- Duration: 1:51
- Updated: 16 Mar 2014
- views: 1030
http://www.wendyscholten.nl - Sporthorses for sale - 5 year old gelding Elazaro (King Kolibri x Voltaire x Joost).
http://www.wendyscholten.nl - Sporthorses for sale - 5 year old gelding Elazaro (King Kolibri x Voltaire x Joost).
wn.com/Sold Elazaro (King Kolibri X Voltaire)
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2:04
Giovanni Domenico Cassini - Video Learning - WizScience.com
"Giovanni" "Domenico Cassini" was an Italian mathematician, astronomer, astrologer and e...
published: 04 Sep 2015
Giovanni Domenico Cassini - Video Learning - WizScience.com
Giovanni Domenico Cassini - Video Learning - WizScience.com
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- published: 04 Sep 2015
- views: 146
2:07
Giovanni Cassini Interview on "Alex in the AM"
A school video project
published: 20 Mar 2013
Giovanni Cassini Interview on "Alex in the AM"
Giovanni Cassini Interview on "Alex in the AM"
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- published: 20 Mar 2013
- views: 163
7:35
thomas astronomy-Giovanni Cassini
astronomy
published: 03 Feb 2008
thomas astronomy-Giovanni Cassini
thomas astronomy-Giovanni Cassini
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- published: 03 Feb 2008
- views: 348
54:58
Mosaico della bell Italia.Prog 48 .Imagen: Giovanni CAssini,de Durangel,1879
TEMAS TRATADOS: Giovanni Cassini, astrónomo italiano, las frottolas, capítulo de Il piccol...
published: 05 Jan 2015
Mosaico della bell Italia.Prog 48 .Imagen: Giovanni CAssini,de Durangel,1879
Mosaico della bell Italia.Prog 48 .Imagen: Giovanni CAssini,de Durangel,1879
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- published: 05 Jan 2015
- views: 49
4:11
FIND IT SOMEDAY - MEET PROBE CASSINI
SKYVIEWS - FIND IT SOMEDAY - (REPORT BELOW)
CASSINI ON HER MISSION TO SATURN
MARCH 17, 20...
published: 19 Mar 2014
FIND IT SOMEDAY - MEET PROBE CASSINI
FIND IT SOMEDAY - MEET PROBE CASSINI
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- published: 19 Mar 2014
- views: 374
1:02
Treasures of the RAS: The woman in the Moon - Cassini's lunar map
The first scientific map of the Moon, made by Giovanni Cassini in 1679.
This detailed eng...
published: 12 Mar 2014
Treasures of the RAS: The woman in the Moon - Cassini's lunar map
Treasures of the RAS: The woman in the Moon - Cassini's lunar map
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- published: 12 Mar 2014
- views: 499
2:33
Cassini-Huygens - Saturn HD IMAX footage
Updated footage in 4K - http://www.youtube.com/watch?v=QNce_8WHTGc&feature;=share
About t...
published: 14 Mar 2011
Cassini-Huygens - Saturn HD IMAX footage
Cassini-Huygens - Saturn HD IMAX footage
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- published: 14 Mar 2011
- views: 69184
5:30
Four Bar infinitiy Coupler Curve
http://www.mekanizmalar.com/menu_linkage.html
This curve known as the lemniscate of Bernou...
published: 09 Jul 2013
Four Bar infinitiy Coupler Curve
Four Bar infinitiy Coupler Curve
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- published: 09 Jul 2013
- views: 7129
1:28
Titan Methane Lakes Cassini Flyover 2013 NASA-JPL Animation from Saturn Orbiter; JQ Music
more at http://scitech.quickfound.net/astro/planet_news.html
Titan: Extraterrestrial Land...
published: 12 Dec 2013
Titan Methane Lakes Cassini Flyover 2013 NASA-JPL Animation from Saturn Orbiter; JQ Music
Titan Methane Lakes Cassini Flyover 2013 NASA-JPL Animation from Saturn Orbiter; JQ Music
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- published: 12 Dec 2013
- views: 8269
4:09
Carolyn Porco speaks about the Cassini-Huygens Mission
CassiniHuygens is a joint NASA/ESA robotic spacecraft mission currently studying the plane...
published: 03 Feb 2009
Carolyn Porco speaks about the Cassini-Huygens Mission
Carolyn Porco speaks about the Cassini-Huygens Mission
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- published: 03 Feb 2009
- views: 2957
4:59
Jápeto
Jápeto
Es uno de los satélites del planeta Saturno. Es el octavo más distante al planeta...
published: 30 Mar 2016
Jápeto
Jápeto
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- published: 30 Mar 2016
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4:59
Where Did Saturn's Rings Come From?
Saturn's majestic, iconic rings define the planet, but where did they come from?
Kevin Gr...
published: 19 Dec 2013
Where Did Saturn's Rings Come From?
Where Did Saturn's Rings Come From?
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4:08
Cassini Enceladus Flyby & Journey to Mars at IAC on This Week @NASA – October 16, 2015 HD
more at: http://scitech.quickfound.net/astro/nasa_news.html
"Published on Oct 16, 2015 - ...
published: 16 Oct 2015
Cassini Enceladus Flyby & Journey to Mars at IAC on This Week @NASA – October 16, 2015 HD
Cassini Enceladus Flyby & Journey to Mars at IAC on This Week @NASA – October 16, 2015 HD
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- published: 16 Oct 2015
- views: 431
5:25
Perinaldo-(LoResMobile) The Village
Visit Perinaldo, Italy, a medieval hill village above the Italian Riviera. It's the birth...
published: 16 Jun 2011
Perinaldo-(LoResMobile) The Village
Perinaldo-(LoResMobile) The Village
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2:39
Sun and Earth Distance in Hanuman Chalisa
Distance between Sun and Earth is given in Hindu Prayer Hanuman Chalisa. Hanuman challisa ...
published: 14 Nov 2014
Sun and Earth Distance in Hanuman Chalisa
Sun and Earth Distance in Hanuman Chalisa
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- published: 14 Nov 2014
- views: 4741
3:57
Giovanni Monti Interview - Ciao Radio - 14 May 2014
Giovanni Monti interview
@ Ciao Radio - 14 May 2014
in studio: Tony Farietti dj - Toz Anto...
published: 15 May 2014
Giovanni Monti Interview - Ciao Radio - 14 May 2014
Giovanni Monti Interview - Ciao Radio - 14 May 2014
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- published: 15 May 2014
- views: 12
45:40
Cassini–Huygens
Cassini–Huygens is an unmanned spacecraft sent to the planet Saturn. It is a flagship-clas...
published: 04 Aug 2014
Cassini–Huygens
Cassini–Huygens
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- published: 04 Aug 2014
- views: 192
50:15
EGU2014: Jean Dominique Cassini Medal Lecture by Stamatios M. Krimigis (ML3)
Medal Lecture at the 2014 General Assembly of the European Geosciences Union, which took p...
published: 03 Feb 2015
EGU2014: Jean Dominique Cassini Medal Lecture by Stamatios M. Krimigis (ML3)
EGU2014: Jean Dominique Cassini Medal Lecture by Stamatios M. Krimigis (ML3)
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- published: 03 Feb 2015
- views: 27
6:15
Zum Verkaufen: Stadthaus im historischen ligurischen Bergdorf Perinaldo
Dieses schöne Haus liegt im Zentrum des mittelalterlichen Ortes und wird zur Zeit als Stud...
published: 28 Jun 2015
Zum Verkaufen: Stadthaus im historischen ligurischen Bergdorf Perinaldo
Zum Verkaufen: Stadthaus im historischen ligurischen Bergdorf Perinaldo
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- published: 28 Jun 2015
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10:10
Hotel La Riana, Perinaldo (Hotel for sale or to rent)
11 rooms (3 single rooms, 2 double rooms on the village site, 6 double rooms to the seasit...
published: 18 Jul 2015
Hotel La Riana, Perinaldo (Hotel for sale or to rent)
Hotel La Riana, Perinaldo (Hotel for sale or to rent)
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- published: 18 Jul 2015
- views: 140
9:25
Perinaldo ( Im )
Immagini di Roberto Fadda
published: 26 Sep 2015
Perinaldo ( Im )
Perinaldo ( Im )
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- published: 26 Sep 2015
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1:51
SOLD: Elazaro (King Kolibri x Voltaire)
http://www.wendyscholten.nl - Sporthorses for sale - 5 year old gelding Elazaro (King Koli...
published: 16 Mar 2014
SOLD: Elazaro (King Kolibri x Voltaire)
SOLD: Elazaro (King Kolibri x Voltaire)
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- published: 16 Mar 2014
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Sun and Earth Distance in Hanuman Chalisa...
Giovanni Monti Interview - Ciao Radio - 14 May 201...
Cassini–Huygens...
EGU2014: Jean Dominique Cassini Medal Lecture by S...
Zum Verkaufen: Stadthaus im historischen ligurisch...
Hotel La Riana, Perinaldo (Hotel for sale or to re...
Perinaldo ( Im )...
SOLD: Elazaro (King Kolibri x Voltaire)...
photo: WN / Aruna Mirasdar
Porn and the Threat to Virility
Edit Time Magazine 31 Mar 2016
Noah Church is a 26-year-old part-time wildland firefighter in Portland, Ore. When he was 9, he found naked pictures on the Internet. He learned how to download explicit videos. When he was 15, streaming videos arrived, and he watched those. Often. Several times a day, doing that which people often do while watching that genre by themselves ... After the appeal of those waned, he moved on to the next level, more intense, often more violent ... ....
photo: Twitter
Kim Kardashian, Emily Ratajkowski post topless bathroom pic
Edit New York Daily News 30 Mar 2016
Kim Kardashian has added a friend to her set of scandalous selfies ... ....
photo: WN / Bhaskar Mallick
India bridge collapse: Kolkata rescue efforts under way
Edit Al Jazeera 01 Apr 2016
Emergency workers in Kolkata continued to search for survivors underneath a collapsed overpass in a congested area of the eastern city, as the construction firm building the flyover was being investigated. At least 21 people were killed and over a dozens were still trapped under the rubble of the under-construction overpass that collapsed on Thursday ... "The condition is pathetic ... And the flyover is built in between residential buildings....
photo: AP / Bikas Das
At Least 21 Confirmed Dead, Scores Injured, Missing In Kolkata Overpass Collapse
Edit WorldNews.com 31 Mar 2016
Rescuers in Kolkata used saws, small cranes and bare hands to dig through the wreckage after a long section of a road overpass under construction collapsed in a crowded Indian neighborhood Thursday killing 21 people and leave scores of injured, the Belfast Telegraph reported Thursday ... “[It] came down with a huge crashing sound. I left my cup of tea and ran. I was crying at the spot.” – Yogesh Sharma, eyewitness to the overpass collapse....
photo: Creative Commons
On 55 Cancri e., It's Always Summer. Super-Earth A 'Cool' 2,060º At Night
Edit WorldNews.com 31 Mar 2016
Scientists have made a scorching hot discovery involving a “super-Earth” exo-planet 40 light years from Earth.The exo-planet, known as 55 Cancri e, is a bit warmer than originally thought – how much warmer? – well, dayside temperatures are about 4,400 degrees Fahrenheit, while nightside temperatures are a “brisk” 2,060 degrees Fahrenheit, CNN reports ... They can be made of gas, rock or a combination of both....
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Principal in North Haledon hands in resignation
Edit North Jersey 01 Apr 2016
High Mountain School Principal Giovanni Giancaspro's resignation was formally accepted by the North Haledon Board of Education on March 17 in a resolution voted on unanimously by the board ... ....
Tenaris Files Annual Report 2015 and Convenes Annual General Meetings of Shareholders (Tenaris SA)
Edit Public Technologies 01 Apr 2016
(Source. Tenaris SA). The Financial and Operational Information Contained in this Press Release Is Based on Audited Consolidated Financial Statements Presented in U.S. Dollars and Prepared in Accordance With International Financial Reporting Standards as Issued by the International Accounting Standard Board and Adopted by the European Union, or IFRS. LUXEMBOURG -- (Marketwired) -- 02/24/16 -- Tenaris S.A. (NYSE. TS) (BAE ... Giovanni Sardagna....
COMPLETION OF DISCLOSEABLE TRANSACTION: ACQUISITION OF 51% INTEREST IN THE TARGET (M Dream Inworld Limited)
Edit Public Technologies 31 Mar 2016
(Source. M Dream Inworld Limited) E161356A_GET Holdings 1..2 ... GET HOLDINGS LIMITED. 智 易 控 股 有 限 公 司*. (Incorporated in the Cayman Islands and continued in Bermuda with limited liability). (Stock Code. 8100). COMPLETION OF DISCLOSEABLE TRANSACTION. ACQUISITION OF 51% INTEREST IN THE TARGET ... On behalf of the Board GET Holdings Limited Kuang Hao Kun Giovanni Chairman. Hong Kong, 31 March 2016 ... Kuang Hao Kun Giovanni and Mr ... Original Document.....
Riverside cops
Edit Chicago Tribune 31 Mar 2016
A Chicago man whose recent gunshot leg wounds hampered an attempt to run away from police was arrested last week by Riverside police, who said was he trying "to sell cannabis to anyone he encountered on the street.". Giovanni Castrejon, 23, of the 700 block of West 71st Street, was charged with drug... ....
RIP CURL GROMSEARCH STARTS THE 2016 ITALIAN JUNIOR CIRCUIT FISURF (ISA - International Surfing Association)
Edit Public Technologies 31 Mar 2016
(Source. ISA - International Surfing Association). 'All's well that ends well' says an Italian proverb. The Italian event of the European Rip Curl Gromsearch was also the start of the 2016 FISURF Italian Junior Circuit. The local organizers in Levanto, one of the most famous Italian waves, called the contest on due to a 3 to 4 feet swell from south-west, set to arrive on march 28th ... 3° GIOVANNI DELL'OVO ... UNDER 14 ... 5° GIOVANNI CARDINALI....
Intesa Sanpaolo: submission of first list of candidates for appointment to Board of Directors and Management Control Committee (Intesa Sanpaolo SpA)
Edit Public Technologies 31 Mar 2016
(Source. Intesa Sanpaolo SpA) DRAFT PRESS RELEASE. PRESS RELEASE. INTESA SANPAOLO. SUBMISSION OF FIRST LIST OF CANDIDATES FOR APPOINTMENT TO BOARD OF DIRECTORS AND MANAGEMENT CONTROL COMMITTEE ... The appointment of Board Directors and Management Control Committee members is on the agenda at the Ordinary Shareholders' Meeting to take place on 27 April 2016 ... The list consists of two separate sections ... Giovanni Costa ... Giovanni Gorno Tempini ... 2....
Viking's Choice: Pinkwash, 'Burning Too'
Edit National Public Radio 31 Mar 2016
i. Pinkwash. Amy June Breesman/Courtesy of the artist hide caption. toggle caption Amy June Breesman/Courtesy of the artist. Pinkwash. Amy June Breesman/Courtesy of the artist ... YouTube. Collective Sigh comes out May 13 on Don Giovanni. ....
Arms and the man: how a culture of warfare shapes masculinity (University of Cambridge)
Edit Public Technologies 31 Mar 2016
The license in question was granted to a painter called Maestro Giovanni Fiammingo Pittore ... It is interesting that Maestro Giovanni was a painter and, as such, attuned to the powerful symbolism of arms and armour ... In a letter written in 1572, Antonio Serguidi noted that Duke Cosimo I wept with pride when he saw his youngest son Giovanni kitted out in armour, and holding a pike and mace....
European funding to study the Paleolithic sites in Croatia (Università di Pisa)
Edit Public Technologies 31 Mar 2016
(Source. Università di Pisa) ... The project entitled 'Mend the Gap ... The archaeologists from the University of Pisa involved in the project are Giovanni Boschian and Damiano Marchi, the geologist is Marta Pappalardo ... In the project, Giovanni Boschian deals with geoarchaeology, or rather paleoenvironmental reconstruction and human behavior through the geological study of sediments from archaeological sites, especially caves ... (noodl....
JCU Professor Stefan Sorgner Participates in Roma Tre University's Conference "Politics and Aesthetics" (John Cabot University)
Edit Public Technologies 31 Mar 2016
(Source. John Cabot University). March 31, 2016. Professor of Philosophy Stefan Lorenz Sorgner will present a paper during Roma Tre University's two-day conference 'Politics and Aesthetics' on April 4-6, 2016. Prof. Sorgner is one of the world's leading post- and transhumanist philosophers ... During the conference, Prof ... The presentations will be moderated by Giovanni Sampaolo and Marco Federici ... (noodl....
Enceladus’ geysers may persist for millions of years
Edit Ars Technica 30 Mar 2016
(credit. Cassini Imaging Team, SSI, JPL, ESA, NASA). Saturn's moon Enceladus is a relatively small body, only a bit over 500km across ... This implies that the geysers, and the E-ring of Saturn that they create, are a very temporary phenomenon, and we're lucky to have sent Cassini there while the geysers were active....
War reporter Di Giovanni on her ‘Dispatches from Syria’
Edit France24 30 Mar 2016
Veteran war reporter Janine Di Giovanni arrived in Damascus in the spring of 2012, when the conflict in Syria was barely a year old. What she witnessed next is that moment when everything suddenly changes from normal to extremely abnormal ... "Dispatches From Syria. The Morning They Came For Us". Di Giovanni paints a harrowing picture of a nation on the brink of unravelling, and of individual resilience ... ....
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