9:32
Hubble's Universe: Extrasolar Planets
facebook.com ... Hubble's Universe Unfiltered (Episode 7): Eye Spy A Planet (Part 2/2)...
published: 05 May 2010
Author: ScienceMagazine
Hubble's Universe: Extrasolar Planets
facebook.com ... Hubble's Universe Unfiltered (Episode 7): Eye Spy A Planet (Part 2/2) - Extrasolar Planets. Up until the 1990s, we only knew of the planets in our own solar system. Since then, we have discovered over 300 planets orbiting other stars (extrasolar planets, exoplanets). However, most of these planets were found when scientists observed the effect of the planet's gravity upon their host stars. Astronomers could not show the world what we wanted most: a visible light picture of a planet around a star like the Sun. That situation changed in November 2008 with a discovery by the Hubble Space Telescope. Join us for the story that begins a new era in our knowledge of planetary systems. --- Please SUBSCRIBE to Science & Reason: • www.youtube.com • www.youtube.com • www.youtube.com • www.youtube.com --- Hubble Directly Observes Planet Orbiting Fomalhaut hubblesite.org --- Notes - Note that Hubble's discovery of Fomalhaut b is billed as the "first visible-light snapshot of a planet orbiting another star." It is important to note that the first direct detection of a planet will likely turn out to be the planet known as 2M1207 b. However, the host, 2M1207, is not a full-fledged star, but a brown dwarf (see below). In addition, pictures of three planets around HR 8799, released the same day as the Fomalhaut discovery, were taken in the infrared. - Let me clarify about 2M1207. It has less than 3% the mass of our Sun, roughly 25 times the mass of Jupiter. That mass places <b>...</b>
5:48
Eye Spy A Planet: Our Solar System
facebook.com ...Hubble's Universe Unfiltered (Episode 7): Eye Spy A Planet (Part 1/2) ...
published: 30 Apr 2010
Author: ScienceMagazine
Eye Spy A Planet: Our Solar System
facebook.com ...Hubble's Universe Unfiltered (Episode 7): Eye Spy A Planet (Part 1/2) - Our Solar System. Up until the 1990s, we only knew of the planets in our own solar system. Since then, we have discovered over 300 planets orbiting other stars (extrasolar planets, exoplanets). However, most of these planets were found when scientists observed the effect of the planet's gravity upon their host stars. Astronomers could not show the world what we wanted most: a visible light picture of a planet around a star like the Sun. That situation changed in November 2008 with a discovery by the Hubble Space Telescope. Join us for the story that begins a new era in our knowledge of planetary systems. --- Please SUBSCRIBE to Science & Reason: • www.youtube.com • www.youtube.com • www.youtube.com • www.youtube.com --- Hubble press release: Hubble Directly Observes Planet Orbiting Fomalhaut hubblesite.org --- Notes - Note that Hubble's discovery of Fomalhaut b is billed as the "first visible-light snapshot of a planet orbiting another star." It is important to note that the first direct detection of a planet will likely turn out to be the planet known as 2M1207 b. However, the host, 2M1207, is not a full-fledged star, but a brown dwarf (see below). In addition, pictures of three planets around HR 8799, released the same day as the Fomalhaut discovery, were taken in the infrared. - Let me clarify about 2M1207. It has less than 3% the mass of our Sun, roughly 25 times the mass of <b>...</b>
6:34
Eye Spy A Planet: Our Solar System,good
Beautiful orrery(solar system model) avaiable in : www.orrerystore.com .Science & Reas...
published: 07 Dec 2011
Author: notbadastro
Eye Spy A Planet: Our Solar System,good
Beautiful orrery(solar system model) avaiable in : www.orrerystore.com .Science & Reason on Facebook: tinyurl.com Universe Unfiltered (Episode 7): Eye Spy A Planet (Part 1/2) - Our Solar System.Up until the 1990s, we only knew of the planets in our own solar system. Since then, we have discovered over 300 planets orbiting other stars (extrasolar planets, exoplanets). However, most of these planets were found when scientists observed the effect of the planet's gravity upon their host stars.Astronomers could not show the world what we wanted most: a visible light picture of a planet around a star like the Sun. That situation changed in November 2008 with a discovery by the Hubble Space Telescope. Join us for the story that begins a new era in our knowledge of planetary systems.---Please subscribe to Science & Reason:• www.youtube.com www.youtube.com www.youtube.com www.youtube.com press release:Hubble Directly Observes Planet Orbiting Fomalhauthubblesite.org Note that Hubble's discovery of Fomalhaut b is billed as the "first visible-light snapshot of a planet orbiting another star." It is important to note that the first direct detection of a planet will likely turn out to be the planet known as 2M1207 b. However, the host, 2M1207, is not a full-fledged star, but a brown dwarf (see below). In addition, pictures of three planets around HR 8799, released the same day as the Fomalhaut discovery, were taken in the infrared.- Let me clarify about 2M1207. It has less than <b>...</b>
7:18
A Space Opera
Science & Reason on Facebook: tinyurl.com ESO VLT Space Opera. Starring: Helix Nebula,...
published: 25 Dec 2009
Author: FFreeThinker
A Space Opera
Science & Reason on Facebook: tinyurl.com ESO VLT Space Opera. Starring: Helix Nebula, Gliese 667, stellar cluster NGC 2467, R Coronae Austrinae, protostar HH34 (Orion), Chamaeleon I complex, Eagle Nebula, Lagoon Nebula, southern Milky Way band, Trifid Nebula, the first image of an exoplanet (2M1207 system). --- Please subscribe to Science & Reason: • www.YouTube.com • www.YouTube.com • www.YouTube.com • www.YouTube.com --- The Very Large Telescope (VLT) is made up of four separate optical telescopes (the Antu telescope, the Kueyen telescope, the Melipal telescope, and the Yepun telescope) organized in an array formation, built and operated by the European Southern Observatory (ESO) at the Paranal Observatory on Cerro Paranal, a 2635 m high mountain in the Atacama desert in northern Chile. The array is complemented by four movable Auxiliary Telescopes. Working together in so-called interferometric mode, the telescopes can achieve an angular resolution of around 1 milliarcsecond, equivalent to the gap between the headlights of a car as observed from the same distance as between the Earth to the Moon. en.wikipedia.org --- Very Large Telescope - The world's most advanced visible-light astronomical observatory The Very Large Telescope array (VLT) is the flagship facility for ESO's ground-based astronomy at the beginning of the third Millennium. It is the worlds most advanced optical instrument, consisting of four Unit Telescopes with main mirrors of 8.2 m diameter and four <b>...</b>
8:04
A Space Opera,good
Beautiful orrery(solar system model) avaiable in : www.orrerystore.com .Science & Reas...
published: 28 Dec 2011
Author: astrospace100
A Space Opera,good
Beautiful orrery(solar system model) avaiable in : www.orrerystore.com .Science & Reason on Facebook: tinyurl.com VLT Space Opera.Starring: Helix Nebula, Gliese 667, stellar cluster NGC 2467, R Coronae Austrinae, protostar HH34 (Orion), Chamaeleon I complex, Eagle Nebula, Lagoon Nebula, southern Milky Way band, Trifid Nebula, the first image of an exoplanet (2M1207 system).---Please subscribe to Science & Reason:• www.YouTube.com www.YouTube.com www.YouTube.com www.YouTube.com Very Large Telescope (VLT) is made up of four separate optical telescopes (the Antu telescope, the Kueyen telescope, the Melipal telescope, and the Yepun telescope) organized in an array formation, built and operated by the European Southern Observatory (ESO) at the Paranal Observatory on Cerro Paranal, a 2635 m high mountain in the Atacama desert in northern Chile.The array is complemented by four movable Auxiliary Telescopes. Working together in so-called interferometric mode, the telescopes can achieve an angular resolution of around 1 milliarcsecond, equivalent to the gap between the headlights of a car as observed from the same distance as between the Earth to the Moon.en.wikipedia.org Large Telescope - The world's most advanced visible-light astronomical observatoryThe Very Large Telescope array (VLT) is the flagship facility for ESO's ground-based astronomy at the beginning of the third Millennium. It is the worlds most advanced optical instrument, consisting of four Unit Telescopes <b>...</b>
Vimeo results:
2:54
Could this really be Planet X ? 2010-03-18 Update
Quote from jcattera's channel on http://www.youtube.com/user/jcattera#p/a
"jcattera - Mar...
published: 09 Apr 2010
Author: manchildminister
Could this really be Planet X ? 2010-03-18 Update
Quote from jcattera's channel on http://www.youtube.com/user/jcattera#p/a
"jcattera - March 18 2010 - Coordinates confirmed w/Meade LX200-ACF Telescope on three separate nights in conjunction with my IR camera to locate this object. I also confirmed with four of my astronomy friends. We all know where Mars is located. The coordinates for this object are no where near Mars.
http://www.nasa.gov/mission_pages/WISE/multimedia/pia12462.html
Planet X?? (also referred to as Nibiru, The Destroyer, or just Brown Dwarf).
This planet or failed star supposedly comes around Earth every 3500 years and creates destruction on Earth and is due to come around in 2012.
So, I've very been interested in capturing an Infrared video of this very large orange object which is visible right now just to the upper left of the star constellation, "Orion the Hunter". This bright orange planet or star is not on any star map, and Mars is over by the "Cancer" star constellation, so it isn't Mars.
Just to point out, Brown dwarfs are too cool to give off much visible light but they do emit substantial amounts of infrared radiation, but they are detectable by ground-based and space borne infrared telescopes.
So, that being the case, I wanted to see how bright the infrared video would be on my Yukon IR camera. After capturing this video, I came to the conclusion that this planet or star is actually giving off a lot of infrared radiation. As you can in the video, I scanned other parts of the sky to show how bright this object really is compared to the other stars.
With that, I'm going to continue monitoring and recording video of this object on every clear night to see if this is getting bigger by the day or week. If it is getting bigger, that would clue us in that this could be Nibiru and is coming closer to us.
Also, an important thing to remember, one of the air shafts in the king's chamber in the great pyramid of Eygpt points to the first star on the left of Orion's belt. That is very close to the location of this orange bright object. My question is, were they trying to tell us that Nibiru will be aligned with this 1st star on Orion's belt in 2012?
Anyways, I'll continue giving updates when I can...
Brown dwarfs are sub-stellar objects which are too low in mass to sustain stable hydrogen fusion. Their mass is below that necessary to maintain hydrogen-burning nuclear fusion reactions in their cores, as do stars on the main sequence, but which have fully convective surfaces and interiors, with no chemical differentiation by depth. Brown dwarfs occupy the mass range between that of large gas giant planets and the lowest mass stars; this upper limit is between 75[1] and 80 Jupiter masses (MJ). Currently there is some debate as to what criterion to use to define the separation between a brown dwarf from a giant planet at very low brown dwarf masses (~13 MJ ), and whether brown dwarfs are required to have experienced fusion at some point in their history. In any event, brown dwarfs heavier than 13 MJ do fuse deuterium and those above ~65 MJ also fuse lithium. The only planets known to orbit brown dwarfs are 2M1207b and MOA-2007-BLG-192Lb
http://www.space.com/scienceastronomy/nemesis-comets-earth-am-100311.html
3:50
Possible Brown Dwarf (Planet X) very close to Orion's Belt
Quote from jcattera's channel on http://www.youtube.com/user/jcattera#p/a
"jcattera - Mar...
published: 09 Apr 2010
Author: manchildminister
Possible Brown Dwarf (Planet X) very close to Orion's Belt
Quote from jcattera's channel on http://www.youtube.com/user/jcattera#p/a
"jcattera - March 18 2010 - Coordinates confirmed w/Meade LX200-ACF Telescope on three separate nights in conjunction with my IR camera to locate this object. I also confirmed with four of my astronomy friends. We all know where Mars is located. The coordinates for this object are no where near Mars.
http://www.nasa.gov/mission_pages/WISE/multimedia/pia12462.html
Planet X?? (also referred to as Nibiru, The Destroyer, or just Brown Dwarf).
This planet or failed star supposedly comes around Earth every 3500 years and creates destruction on Earth and is due to come around in 2012.
So, I've very been interested in capturing an Infrared video of this very large orange object which is visible right now just to the upper left of the star constellation, "Orion the Hunter". This bright orange planet or star is not on any star map, and Mars is over by the "Cancer" star constellation, so it isn't Mars.
Just to point out, Brown dwarfs are too cool to give off much visible light but they do emit substantial amounts of infrared radiation, but they are detectable by ground-based and space borne infrared telescopes.
So, that being the case, I wanted to see how bright the infrared video would be on my Yukon IR camera. After capturing this video, I came to the conclusion that this planet or star is actually giving off a lot of infrared radiation. As you can in the video, I scanned other parts of the sky to show how bright this object really is compared to the other stars.
With that, I'm going to continue monitoring and recording video of this object on every clear night to see if this is getting bigger by the day or week. If it is getting bigger, that would clue us in that this could be Nibiru and is coming closer to us.
Also, an important thing to remember, one of the air shafts in the king's chamber in the great pyramid of Eygpt points to the first star on the left of Orion's belt. That is very close to the location of this orange bright object. My question is, were they trying to tell us that Nibiru will be aligned with this 1st star on Orion's belt in 2012?
Anyways, I'll continue giving updates when I can...
Brown dwarfs are sub-stellar objects which are too low in mass to sustain stable hydrogen fusion. Their mass is below that necessary to maintain hydrogen-burning nuclear fusion reactions in their cores, as do stars on the main sequence, but which have fully convective surfaces and interiors, with no chemical differentiation by depth. Brown dwarfs occupy the mass range between that of large gas giant planets and the lowest mass stars; this upper limit is between 75[1] and 80 Jupiter masses (MJ). Currently there is some debate as to what criterion to use to define the separation between a brown dwarf from a giant planet at very low brown dwarf masses (~13 MJ ), and whether brown dwarfs are required to have experienced fusion at some point in their history. In any event, brown dwarfs heavier than 13 MJ do fuse deuterium and those above ~65 MJ also fuse lithium. The only planets known to orbit brown dwarfs are 2M1207b and MOA-2007-BLG-192Lb
http://www.space.com/scienceastronomy/nemesis-comets-earth-am-100311.html