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Vesto Slipher
Vesto Slipher
Robin Danderkindt
℗ 2015 Robin Danderkindt
Released on: 2015-04-28
Auto-generated by YouTube.
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Vesto Slipher.
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Laird Thompson: Expanding Universe Conference (http://www.lowell.edu/workshops/slipher)
Title: Vesto Slipher and the development of nebular spectrographs Abstract: While the earliest attempts to detect photographic spectra of galaxies—by Huggins...
-
Cosmic Time Mechanism, Part 1 Gravitational Time Dilation, by Dimitri Metz
The logical explanation for: - The Accelerating Growth of the Universe, - Hubble's Law, - The Galaxy Orbit Speed Discrepancies, - Galaxy Spiral Arms, - The M...
-
Slipher Expanding Universe P.01 Daniel Armstrong
Conference on Origins of the Expanding Universe: 1912-1932 Sep 14-15, 2012 - Lowell Observatory Presentation P.01 Daniel Armstrong Spectral Shifts A visual a...
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El Universo: Bin Bang, la gran explosión 3/5
La teoría del Big Bang se desarrolló a partir de observaciones y avances teóricos. Por medio de observaciones, en la década de 1910, el astrónomo estadounide...
-
Teach Astronomy - Discovery of Galaxy Redshifts
http://www.teachastronomy.com/ In 1912 Vesto Slipher working at the Lowell Observatory began a project to observe spectra of spiral nebulae. He was working u...
-
Dr Hubble's Mistake: A Difficult Diagnosis [Shorter Version]
This video examines the teachings of 4 pioneer cosmologists Henrietta Leavitt, Vesto Slipher, Georges Lemaitre and Edwin Hubble and suggests an anomaly in th...
-
Mysteries of a Dark Universe
Cosmology, the study of the universe as a whole, has been turned on its head by a stunning discovery that the universe is flying apart in all directions at a...
-
Nebula
A nebula is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the Andromeda Nebula before the true nature of galaxies was confirmed in the early 20th century by Vesto Slipher, Edwin Hubble and others. Nebulae are
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Nebula
A nebula (from Latin: "cloud"; pl. nebulae or nebulæ, with ligature, or nebulas) is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the Andromeda Nebula (and spiral galaxies in general as "spiral nebulae") before
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The Universe- Dark Energy | Full Documentary HD
advexontube.com Seosan TV DOCUMENTARY HD ( WORLD BEST DOCUMENTARIES AROUND THE WORLD )
For thousands of years, astronomers wrestled with basic questions about the size and age of the universe. Does the universe go on forever, or does it have an edge somewhere? Has it always existed, or did it come to being some time in the past? In 1929, Edwin Hubble, an astronomer at Caltech, made a critical d
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video youtube3
A nebula (from Latin: "cloud";[1] pl. nebulae or nebulæ, with ligature, or nebulas) is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the Andromeda Nebula (and spiral galaxies in general as "spiral nebulae") bef
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NEBULA - Hubble probes distant Nebula.
A nebula is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, inclu...
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Nebula - Video Learning - WizScience.com
A "nebula" is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, "nebula" was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the "Andromeda Nebula" before the true nature of galaxies was confirmed in the early 20th century by Vesto Slipher, Edwin Hubble and others.
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How colourful clouds of gas get their hue
A nebula (from Latin: "cloud";[1] pl. nebulae or nebulæ, with ligature, or nebulas) is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the Andromeda Nebula (and spiral galaxies in general as "spiral nebulae") bef
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Teach Astronomy - Discovery of Active Galaxies
http://www.teachastronomy.com/ Active galaxies were discovered even before we knew the distance to galaxies. In 1908, Edward Fath discovered strong emission ...
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Edwin Hubble - History channel
Edwin Powell Hubble (November 20, 1889 – September 28, 1953) was an American astronomer who played a crucial role in establishing the field of extragalactic astronomy and is generally regarded as one of the most important observational cosmologists of the 20th century. Hubble is known for showing that the recessional velocity of a galaxy increases with its distance from the earth, implying the Uni
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Physical cosmology
Physical cosmology is the study of the largest-scale structures and dynamics of the Universe and is concerned with fundamental questions about its origin, structure, evolution, and ultimate fate. For most of human history, it was a branch of metaphysics and religion. Cosmology as a science originated with the Copernican principle, which implies that celestial bodies obey identical physical laws to
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Edwin Hubble - Video Learning - WizScience.com
"Edwin Powell Hubble" was an American astronomer who played a crucial role in establishing the field of extragalactic astronomy and is generally regarded as one of the most important observational cosmologists of the 20th century. Hubble is known for showing that the recessional velocity of a galaxy increases with its distance from the earth, implying the universe is expanding, known as "Hubble'
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Tired light - Video Learning - WizScience.com
"Tired light" is a class of hypothetical redshift mechanisms that was proposed as an alternative explanation for the redshift-distance relationship. These models have been proposed as alternatives to the metric expansion of space of which the Big Bang and the Steady State cosmologies are the most famous examples. The concept was first proposed in 1929 by Fritz Zwicky, who suggested that if photons
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What Is The Evidence For The Big Bang?
Almost all astronomers agree on the theory of the Big Bang, that the entire Universe is spreading apart, with distant galaxies speeding away from us in all d...
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Perseid meteor shower will help astronomers get a better view of space
As sky-watchers marvel at the beauty of the annual Perseid meteor shower — set to peak late Sunday and early Monday — astronomers will be thanking their shoo...
Vesto Slipher
Vesto Slipher
Robin Danderkindt
℗ 2015 Robin Danderkindt
Released on: 2015-04-28
Auto-generated by YouTube....
Vesto Slipher
Robin Danderkindt
℗ 2015 Robin Danderkindt
Released on: 2015-04-28
Auto-generated by YouTube.
wn.com/Vesto Slipher
Vesto Slipher
Robin Danderkindt
℗ 2015 Robin Danderkindt
Released on: 2015-04-28
Auto-generated by YouTube.
- published: 01 May 2015
- views: 5
Laird Thompson: Expanding Universe Conference (http://www.lowell.edu/workshops/slipher)
Title: Vesto Slipher and the development of nebular spectrographs Abstract: While the earliest attempts to detect photographic spectra of galaxies—by Huggins......
Title: Vesto Slipher and the development of nebular spectrographs Abstract: While the earliest attempts to detect photographic spectra of galaxies—by Huggins...
wn.com/Laird Thompson Expanding Universe Conference (Http Www.Lowell.Edu Workshops Slipher)
Title: Vesto Slipher and the development of nebular spectrographs Abstract: While the earliest attempts to detect photographic spectra of galaxies—by Huggins...
Cosmic Time Mechanism, Part 1 Gravitational Time Dilation, by Dimitri Metz
The logical explanation for: - The Accelerating Growth of the Universe, - Hubble's Law, - The Galaxy Orbit Speed Discrepancies, - Galaxy Spiral Arms, - The M......
The logical explanation for: - The Accelerating Growth of the Universe, - Hubble's Law, - The Galaxy Orbit Speed Discrepancies, - Galaxy Spiral Arms, - The M...
wn.com/Cosmic Time Mechanism, Part 1 Gravitational Time Dilation, By Dimitri Metz
The logical explanation for: - The Accelerating Growth of the Universe, - Hubble's Law, - The Galaxy Orbit Speed Discrepancies, - Galaxy Spiral Arms, - The M...
Slipher Expanding Universe P.01 Daniel Armstrong
Conference on Origins of the Expanding Universe: 1912-1932 Sep 14-15, 2012 - Lowell Observatory Presentation P.01 Daniel Armstrong Spectral Shifts A visual a......
Conference on Origins of the Expanding Universe: 1912-1932 Sep 14-15, 2012 - Lowell Observatory Presentation P.01 Daniel Armstrong Spectral Shifts A visual a...
wn.com/Slipher Expanding Universe P.01 Daniel Armstrong
Conference on Origins of the Expanding Universe: 1912-1932 Sep 14-15, 2012 - Lowell Observatory Presentation P.01 Daniel Armstrong Spectral Shifts A visual a...
El Universo: Bin Bang, la gran explosión 3/5
La teoría del Big Bang se desarrolló a partir de observaciones y avances teóricos. Por medio de observaciones, en la década de 1910, el astrónomo estadounide......
La teoría del Big Bang se desarrolló a partir de observaciones y avances teóricos. Por medio de observaciones, en la década de 1910, el astrónomo estadounide...
wn.com/El Universo Bin Bang, La Gran Explosión 3 5
La teoría del Big Bang se desarrolló a partir de observaciones y avances teóricos. Por medio de observaciones, en la década de 1910, el astrónomo estadounide...
Teach Astronomy - Discovery of Galaxy Redshifts
http://www.teachastronomy.com/ In 1912 Vesto Slipher working at the Lowell Observatory began a project to observe spectra of spiral nebulae. He was working u......
http://www.teachastronomy.com/ In 1912 Vesto Slipher working at the Lowell Observatory began a project to observe spectra of spiral nebulae. He was working u...
wn.com/Teach Astronomy Discovery Of Galaxy Redshifts
http://www.teachastronomy.com/ In 1912 Vesto Slipher working at the Lowell Observatory began a project to observe spectra of spiral nebulae. He was working u...
Dr Hubble's Mistake: A Difficult Diagnosis [Shorter Version]
This video examines the teachings of 4 pioneer cosmologists Henrietta Leavitt, Vesto Slipher, Georges Lemaitre and Edwin Hubble and suggests an anomaly in th......
This video examines the teachings of 4 pioneer cosmologists Henrietta Leavitt, Vesto Slipher, Georges Lemaitre and Edwin Hubble and suggests an anomaly in th...
wn.com/Dr Hubble's Mistake A Difficult Diagnosis Shorter Version
This video examines the teachings of 4 pioneer cosmologists Henrietta Leavitt, Vesto Slipher, Georges Lemaitre and Edwin Hubble and suggests an anomaly in th...
Mysteries of a Dark Universe
Cosmology, the study of the universe as a whole, has been turned on its head by a stunning discovery that the universe is flying apart in all directions at a......
Cosmology, the study of the universe as a whole, has been turned on its head by a stunning discovery that the universe is flying apart in all directions at a...
wn.com/Mysteries Of A Dark Universe
Cosmology, the study of the universe as a whole, has been turned on its head by a stunning discovery that the universe is flying apart in all directions at a...
- published: 13 Oct 2011
- views: 628561
-
author: SpaceRip
Nebula
A nebula is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, includi...
A nebula is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the Andromeda Nebula before the true nature of galaxies was confirmed in the early 20th century by Vesto Slipher, Edwin Hubble and others. Nebulae are often star-forming regions, such as in the Eagle Nebula. This nebula is depicted in one of NASA's most famous images, the "Pillars of Creation". In these regions the formations of gas, dust, and other materials "clump" together to form larger masses, which attract further matter, and eventually will become massive enough to form stars. The remaining materials are then believed to form planets, and other planetary system objects.
This video targeted to blind users.
Attribution:
Article text available under CC-BY-SA
Public domain image source in video
wn.com/Nebula
A nebula is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the Andromeda Nebula before the true nature of galaxies was confirmed in the early 20th century by Vesto Slipher, Edwin Hubble and others. Nebulae are often star-forming regions, such as in the Eagle Nebula. This nebula is depicted in one of NASA's most famous images, the "Pillars of Creation". In these regions the formations of gas, dust, and other materials "clump" together to form larger masses, which attract further matter, and eventually will become massive enough to form stars. The remaining materials are then believed to form planets, and other planetary system objects.
This video targeted to blind users.
Attribution:
Article text available under CC-BY-SA
Public domain image source in video
- published: 12 May 2014
- views: 0
Nebula
A nebula (from Latin: "cloud"; pl. nebulae or nebulæ, with ligature, or nebulas) is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Ori...
A nebula (from Latin: "cloud"; pl. nebulae or nebulæ, with ligature, or nebulas) is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the Andromeda Nebula (and spiral galaxies in general as "spiral nebulae") before the true nature of galaxies was confirmed in the early 20th century by Vesto Slipher, Edwin Hubble and others. Nebulae are often star-forming regions, such as in the Eagle Nebula. This nebula is depicted in one of NASA's most famous images, the "Pillars of Creation". In these regions the formations of gas, dust, and other materials "clump" together to form larger masses, which attract further matter, and eventually will become massive enough to form stars. The remaining materials are then believed to form planets, and other planetary system objects.
This video is targeted to blind users.
Attribution:
Article text available under CC-BY-SA
Creative Commons image source in video
wn.com/Nebula
A nebula (from Latin: "cloud"; pl. nebulae or nebulæ, with ligature, or nebulas) is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the Andromeda Nebula (and spiral galaxies in general as "spiral nebulae") before the true nature of galaxies was confirmed in the early 20th century by Vesto Slipher, Edwin Hubble and others. Nebulae are often star-forming regions, such as in the Eagle Nebula. This nebula is depicted in one of NASA's most famous images, the "Pillars of Creation". In these regions the formations of gas, dust, and other materials "clump" together to form larger masses, which attract further matter, and eventually will become massive enough to form stars. The remaining materials are then believed to form planets, and other planetary system objects.
This video is targeted to blind users.
Attribution:
Article text available under CC-BY-SA
Creative Commons image source in video
- published: 31 Jul 2014
- views: 1
The Universe- Dark Energy | Full Documentary HD
advexontube.com Seosan TV DOCUMENTARY HD ( WORLD BEST DOCUMENTARIES AROUND THE WORLD )
For thousands of years, astronomers wrestled with basic questions abou...
advexontube.com Seosan TV DOCUMENTARY HD ( WORLD BEST DOCUMENTARIES AROUND THE WORLD )
For thousands of years, astronomers wrestled with basic questions about the size and age of the universe. Does the universe go on forever, or does it have an edge somewhere? Has it always existed, or did it come to being some time in the past? In 1929, Edwin Hubble, an astronomer at Caltech, made a critical discovery that soon led to scientific answers for these questions: he discovered that the universe is expanding.
The ancient Greeks recognized that it was difficult to imagine what an infinite universe might look like. But they also wondered that if the universe were finite, and you stuck out your hand at the edge, where would your hand go? The Greeks' two problems with the universe represented a paradox - the universe had to be either finite or infinite, and both alternatives presented problems.
After the rise of modern astronomy, another paradox began to puzzle astronomers. In the early 1800s, German astronomer Heinrich Olbers argued that the universe must be finite. If the Universe were infinite and contained stars throughout, Olbers said, then if you looked in any particular direction, your line-of-sight would eventually fall on the surface of a star. Although the apparent size of a star in the sky becomes smaller as the distance to the star increases, the brightness of this smaller surface remains a constant. Therefore, if the Universe were infinite, the whole surface of the night sky should be as bright as a star. Obviously, there are dark areas in the sky, so the universe must be finite.
But, when Isaac Newton discovered the law of gravity, he realized that gravity is always attractive. Every object in the universe attracts every other object. If the universe truly were finite, the attractive forces of all the objects in the universe should have caused the entire universe to collapse on itself. This clearly had not happened, and so astronomers were presented with a paradox.
When Einstein developed his theory of gravity in the General Theory of Relativity, he thought he ran into the same problem that Newton did: his equations said that the universe should be either expanding or collapsing, yet he assumed that the universe was static. His original solution contained a constant term, called the cosmological constant, which cancelled the effects of gravity on very large scales, and led to a static universe. After Hubble discovered that the universe was expanding, Einstein called the cosmological constant his "greatest blunder."
At around the same time, larger telescopes were being built that were able to accurately measure the spectra, or the intensity of light as a function of wavelength, of faint objects. Using these new data, astronomers tried to understand the plethora of faint, nebulous objects they were observing. Between 1912 and 1922, astronomer Vesto Slipher at the Lowell Observatory in Arizona discovered that the spectra of light from many of these objects was systematically shifted to longer wavelengths, or redshifted. A short time later, other astronomers showed that these nebulous objects were distant galaxies.
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Thank You for watching!
Please don't forget to subscribe!!
God Bless You!
Documentary #DocumentaryChannel #History&Reserch; #Space #Documentary #BestDocumentary #Explore #Discover #Advance #Technology #DocumentaryHd #AsiaTravel #DicoverSpace #Discover #UnitedStates #Ukraine #ISIS #Israel #Palestine #WW3 #Worldsbest #Sighseeing #whattodo #howto #Amazing #Cool #Best #top #America #UnitedNations #EuropeanUnion#human#SafeLife
wn.com/The Universe Dark Energy | Full Documentary Hd
advexontube.com Seosan TV DOCUMENTARY HD ( WORLD BEST DOCUMENTARIES AROUND THE WORLD )
For thousands of years, astronomers wrestled with basic questions about the size and age of the universe. Does the universe go on forever, or does it have an edge somewhere? Has it always existed, or did it come to being some time in the past? In 1929, Edwin Hubble, an astronomer at Caltech, made a critical discovery that soon led to scientific answers for these questions: he discovered that the universe is expanding.
The ancient Greeks recognized that it was difficult to imagine what an infinite universe might look like. But they also wondered that if the universe were finite, and you stuck out your hand at the edge, where would your hand go? The Greeks' two problems with the universe represented a paradox - the universe had to be either finite or infinite, and both alternatives presented problems.
After the rise of modern astronomy, another paradox began to puzzle astronomers. In the early 1800s, German astronomer Heinrich Olbers argued that the universe must be finite. If the Universe were infinite and contained stars throughout, Olbers said, then if you looked in any particular direction, your line-of-sight would eventually fall on the surface of a star. Although the apparent size of a star in the sky becomes smaller as the distance to the star increases, the brightness of this smaller surface remains a constant. Therefore, if the Universe were infinite, the whole surface of the night sky should be as bright as a star. Obviously, there are dark areas in the sky, so the universe must be finite.
But, when Isaac Newton discovered the law of gravity, he realized that gravity is always attractive. Every object in the universe attracts every other object. If the universe truly were finite, the attractive forces of all the objects in the universe should have caused the entire universe to collapse on itself. This clearly had not happened, and so astronomers were presented with a paradox.
When Einstein developed his theory of gravity in the General Theory of Relativity, he thought he ran into the same problem that Newton did: his equations said that the universe should be either expanding or collapsing, yet he assumed that the universe was static. His original solution contained a constant term, called the cosmological constant, which cancelled the effects of gravity on very large scales, and led to a static universe. After Hubble discovered that the universe was expanding, Einstein called the cosmological constant his "greatest blunder."
At around the same time, larger telescopes were being built that were able to accurately measure the spectra, or the intensity of light as a function of wavelength, of faint objects. Using these new data, astronomers tried to understand the plethora of faint, nebulous objects they were observing. Between 1912 and 1922, astronomer Vesto Slipher at the Lowell Observatory in Arizona discovered that the spectra of light from many of these objects was systematically shifted to longer wavelengths, or redshifted. A short time later, other astronomers showed that these nebulous objects were distant galaxies.
=====================================
Thank You for watching!
Please don't forget to subscribe!!
God Bless You!
Documentary #DocumentaryChannel #History&Reserch; #Space #Documentary #BestDocumentary #Explore #Discover #Advance #Technology #DocumentaryHd #AsiaTravel #DicoverSpace #Discover #UnitedStates #Ukraine #ISIS #Israel #Palestine #WW3 #Worldsbest #Sighseeing #whattodo #howto #Amazing #Cool #Best #top #America #UnitedNations #EuropeanUnion#human#SafeLife
- published: 25 Apr 2015
- views: 1
video youtube3
A nebula (from Latin: "cloud";[1] pl. nebulae or nebulæ, with ligature, or nebulas) is an interstellar cloud of dust, hydrogen, helium and other ionized gases. ...
A nebula (from Latin: "cloud";[1] pl. nebulae or nebulæ, with ligature, or nebulas) is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the Andromeda Nebula (and spiral galaxies in general as "spiral nebulae") before the true nature of galaxies was confirmed in the early 20th century by Vesto Slipher, Edwin Hubble and others. Nebulae are often star-forming regions, such as in the Eagle Nebula. This nebula is depicted in one of NASA's most famous images, the "Pillars of Creation". In these regions the formations of gas, dust, and other materials "clump" together to form larger masses, which attract further matter, and eventually will become massive enough to form stars. The remaining materials are then believed to form planets, and other planetary system objects.
wn.com/Video Youtube3
A nebula (from Latin: "cloud";[1] pl. nebulae or nebulæ, with ligature, or nebulas) is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the Andromeda Nebula (and spiral galaxies in general as "spiral nebulae") before the true nature of galaxies was confirmed in the early 20th century by Vesto Slipher, Edwin Hubble and others. Nebulae are often star-forming regions, such as in the Eagle Nebula. This nebula is depicted in one of NASA's most famous images, the "Pillars of Creation". In these regions the formations of gas, dust, and other materials "clump" together to form larger masses, which attract further matter, and eventually will become massive enough to form stars. The remaining materials are then believed to form planets, and other planetary system objects.
- published: 03 Aug 2014
- views: 8
NEBULA - Hubble probes distant Nebula.
A nebula is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, inclu......
A nebula is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, inclu...
wn.com/Nebula Hubble Probes Distant Nebula.
A nebula is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, inclu...
Nebula - Video Learning - WizScience.com
A "nebula" is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, "nebula" was a name for any diffuse astronomical object, i...
A "nebula" is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, "nebula" was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the "Andromeda Nebula" before the true nature of galaxies was confirmed in the early 20th century by Vesto Slipher, Edwin Hubble and others.
Most nebulae are of vast size, even hundreds of light years in diameter. Although denser than the space surrounding them, most nebulae are far less dense than any vacuum created in an Earthen environment - a nebular cloud the size of the Earth would have a total mass of only a few kilograms.
Nebulae are often star-forming regions, such as in the "Pillars of Creation" in the Eagle Nebula. In these regions the formations of gas, dust, and other materials "clump" together to form larger masses, which attract further matter, and eventually will become massive enough to form stars. The remaining materials are then believed to form planets and other planetary system objects.
Around 150 AD, Claudius Ptolemaeus recorded, in books VII-VIII of his "Almagest", five stars that appeared nebulous. He also noted a region of nebulosity between the constellations Ursa Major and Leo that was not associated with any star. The first true nebula, as distinct from a star cluster, was mentioned by the Persian/Muslim astronomer, Abd al-Rahman al-Sufi, in his "Book of Fixed Stars" . He noted "a little cloud" where the Andromeda Galaxy is located. He also cataloged the Omicron Velorum star cluster as a "nebulous star" and other nebulous objects, such as Brocchi's Cluster. The supernova that created the Crab Nebula, the SN 1054, was observed by Arabic and Chinese astronomers in 1054.
Wiz Science™ is "the" learning channel for children and all ages.
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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/Nebula, 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/Nebula Video Learning Wizscience.Com
A "nebula" is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, "nebula" was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the "Andromeda Nebula" before the true nature of galaxies was confirmed in the early 20th century by Vesto Slipher, Edwin Hubble and others.
Most nebulae are of vast size, even hundreds of light years in diameter. Although denser than the space surrounding them, most nebulae are far less dense than any vacuum created in an Earthen environment - a nebular cloud the size of the Earth would have a total mass of only a few kilograms.
Nebulae are often star-forming regions, such as in the "Pillars of Creation" in the Eagle Nebula. In these regions the formations of gas, dust, and other materials "clump" together to form larger masses, which attract further matter, and eventually will become massive enough to form stars. The remaining materials are then believed to form planets and other planetary system objects.
Around 150 AD, Claudius Ptolemaeus recorded, in books VII-VIII of his "Almagest", five stars that appeared nebulous. He also noted a region of nebulosity between the constellations Ursa Major and Leo that was not associated with any star. The first true nebula, as distinct from a star cluster, was mentioned by the Persian/Muslim astronomer, Abd al-Rahman al-Sufi, in his "Book of Fixed Stars" . He noted "a little cloud" where the Andromeda Galaxy is located. He also cataloged the Omicron Velorum star cluster as a "nebulous star" and other nebulous objects, such as Brocchi's Cluster. The supernova that created the Crab Nebula, the SN 1054, was observed by Arabic and Chinese astronomers in 1054.
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/Nebula, 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: 08 Sep 2015
- views: 1
How colourful clouds of gas get their hue
A nebula (from Latin: "cloud";[1] pl. nebulae or nebulæ, with ligature, or nebulas) is an interstellar cloud of dust, hydrogen, helium and other ionized gases. ...
A nebula (from Latin: "cloud";[1] pl. nebulae or nebulæ, with ligature, or nebulas) is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the Andromeda Nebula (and spiral galaxies in general as "spiral nebulae") before the true nature of galaxies was confirmed in the early 20th century by Vesto Slipher, Edwin Hubble, et al.
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wn.com/How Colourful Clouds Of Gas Get Their Hue
A nebula (from Latin: "cloud";[1] pl. nebulae or nebulæ, with ligature, or nebulas) is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the Andromeda Nebula (and spiral galaxies in general as "spiral nebulae") before the true nature of galaxies was confirmed in the early 20th century by Vesto Slipher, Edwin Hubble, et al.
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- published: 15 Sep 2013
- views: 1
Teach Astronomy - Discovery of Active Galaxies
http://www.teachastronomy.com/ Active galaxies were discovered even before we knew the distance to galaxies. In 1908, Edward Fath discovered strong emission ......
http://www.teachastronomy.com/ Active galaxies were discovered even before we knew the distance to galaxies. In 1908, Edward Fath discovered strong emission ...
wn.com/Teach Astronomy Discovery Of Active Galaxies
http://www.teachastronomy.com/ Active galaxies were discovered even before we knew the distance to galaxies. In 1908, Edward Fath discovered strong emission ...
Edwin Hubble - History channel
Edwin Powell Hubble (November 20, 1889 – September 28, 1953) was an American astronomer who played a crucial role in establishing the field of extragalactic ast...
Edwin Powell Hubble (November 20, 1889 – September 28, 1953) was an American astronomer who played a crucial role in establishing the field of extragalactic astronomy and is generally regarded as one of the most important observational cosmologists of the 20th century. Hubble is known for showing that the recessional velocity of a galaxy increases with its distance from the earth, implying the Universe is expanding. Known as "Hubble's law", this relation had been discovered previously by Georges Lemaître, a Belgian priest/astronomer who published his work in a less visible journal. There is still much controversy surrounding the issue, and some argue that it should be referred to as "Lemaître's law", although this change has not taken hold in the astronomy community.
Edwin Hubble is also known for providing substantial evidence that many objects then classified as "nebulae" were actually galaxies beyond the Milky Way. American astronomer Vesto Slipher provided the first evidence for this argument almost a decade before.
Edwin Hubble supported the Doppler shift interpretation of the observed redshift that had been proposed earlier by Slipher, and that led to the theory of the metric expansion of space. He tended to believe that the frequency of light could, by some so far unknown means, decrease the longer light travels through space.
wn.com/Edwin Hubble History Channel
Edwin Powell Hubble (November 20, 1889 – September 28, 1953) was an American astronomer who played a crucial role in establishing the field of extragalactic astronomy and is generally regarded as one of the most important observational cosmologists of the 20th century. Hubble is known for showing that the recessional velocity of a galaxy increases with its distance from the earth, implying the Universe is expanding. Known as "Hubble's law", this relation had been discovered previously by Georges Lemaître, a Belgian priest/astronomer who published his work in a less visible journal. There is still much controversy surrounding the issue, and some argue that it should be referred to as "Lemaître's law", although this change has not taken hold in the astronomy community.
Edwin Hubble is also known for providing substantial evidence that many objects then classified as "nebulae" were actually galaxies beyond the Milky Way. American astronomer Vesto Slipher provided the first evidence for this argument almost a decade before.
Edwin Hubble supported the Doppler shift interpretation of the observed redshift that had been proposed earlier by Slipher, and that led to the theory of the metric expansion of space. He tended to believe that the frequency of light could, by some so far unknown means, decrease the longer light travels through space.
- published: 25 Feb 2015
- views: 1
Physical cosmology
Physical cosmology is the study of the largest-scale structures and dynamics of the Universe and is concerned with fundamental questions about its origin, struc...
Physical cosmology is the study of the largest-scale structures and dynamics of the Universe and is concerned with fundamental questions about its origin, structure, evolution, and ultimate fate. For most of human history, it was a branch of metaphysics and religion. Cosmology as a science originated with the Copernican principle, which implies that celestial bodies obey identical physical laws to those on Earth, and Newtonian mechanics, which first allowed us to understand those physical laws.
Physical cosmology, as it is now understood, began with the development in 1915 of Albert Einstein's general theory of relativity, followed by major observational discoveries in the 1920s: first, Edwin Hubble discovered that the universe contains a huge number of external galaxies beyond our own Milky Way; then, work by Vesto Slipher and others showed that the universe is expanding. These advances made it possible to speculate about the origin of the universe, and allowed the establishment of the Big Bang Theory, by Georges Lemaitre, as the leading cosmological model. A few researchers still advocate a handful of alternative cosmologies; however, most cosmologists agree that the Big Bang theory explains the observations better.
This video is targeted to blind users.
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Article text available under CC-BY-SA
Creative Commons image source in video
wn.com/Physical Cosmology
Physical cosmology is the study of the largest-scale structures and dynamics of the Universe and is concerned with fundamental questions about its origin, structure, evolution, and ultimate fate. For most of human history, it was a branch of metaphysics and religion. Cosmology as a science originated with the Copernican principle, which implies that celestial bodies obey identical physical laws to those on Earth, and Newtonian mechanics, which first allowed us to understand those physical laws.
Physical cosmology, as it is now understood, began with the development in 1915 of Albert Einstein's general theory of relativity, followed by major observational discoveries in the 1920s: first, Edwin Hubble discovered that the universe contains a huge number of external galaxies beyond our own Milky Way; then, work by Vesto Slipher and others showed that the universe is expanding. These advances made it possible to speculate about the origin of the universe, and allowed the establishment of the Big Bang Theory, by Georges Lemaitre, as the leading cosmological model. A few researchers still advocate a handful of alternative cosmologies; however, most cosmologists agree that the Big Bang theory explains the observations better.
This video is targeted to blind users.
Attribution:
Article text available under CC-BY-SA
Creative Commons image source in video
- published: 02 Nov 2015
- views: 5
Edwin Hubble - Video Learning - WizScience.com
"Edwin Powell Hubble" was an American astronomer who played a crucial role in establishing the field of extragalactic astronomy and is generally regarded as o...
"Edwin Powell Hubble" was an American astronomer who played a crucial role in establishing the field of extragalactic astronomy and is generally regarded as one of the most important observational cosmologists of the 20th century. Hubble is known for showing that the recessional velocity of a galaxy increases with its distance from the earth, implying the universe is expanding, known as "Hubble's law" although this relation had been discovered previously by Georges Lemaître, who published his work in a less visible journal.
Edwin Hubble is also known for providing substantial evidence that many objects then classified as "nebulae" were actually galaxies beyond the Milky Way. American astronomer Vesto Slipher provided the first evidence for this argument almost a decade before.
Edwin Hubble was born to Virginia Lee James and John Powell Hubble, an insurance executive, in Marshfield, Missouri, and moved to Wheaton, Illinois, in 1900. In his younger days, he was noted more for his athletic prowess than his intellectual abilities, although he did earn good grades in every subject except for spelling. Edwin was a gifted athlete playing baseball, football, basketball, and he ran track in both high school and college. He played a variety of positions on the basketball court from center to shooting guard. In fact Hubble even led the University of Chicago's basketball team to their first conference title in 1907. He won seven first places and a third place in a single high school track and field meet in 1906.
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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/Edwin+Hubble, 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/Edwin Hubble Video Learning Wizscience.Com
"Edwin Powell Hubble" was an American astronomer who played a crucial role in establishing the field of extragalactic astronomy and is generally regarded as one of the most important observational cosmologists of the 20th century. Hubble is known for showing that the recessional velocity of a galaxy increases with its distance from the earth, implying the universe is expanding, known as "Hubble's law" although this relation had been discovered previously by Georges Lemaître, who published his work in a less visible journal.
Edwin Hubble is also known for providing substantial evidence that many objects then classified as "nebulae" were actually galaxies beyond the Milky Way. American astronomer Vesto Slipher provided the first evidence for this argument almost a decade before.
Edwin Hubble was born to Virginia Lee James and John Powell Hubble, an insurance executive, in Marshfield, Missouri, and moved to Wheaton, Illinois, in 1900. In his younger days, he was noted more for his athletic prowess than his intellectual abilities, although he did earn good grades in every subject except for spelling. Edwin was a gifted athlete playing baseball, football, basketball, and he ran track in both high school and college. He played a variety of positions on the basketball court from center to shooting guard. In fact Hubble even led the University of Chicago's basketball team to their first conference title in 1907. He won seven first places and a third place in a single high school track and field meet in 1906.
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/Edwin+Hubble, 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: 24 Sep 2015
- views: 1
Tired light - Video Learning - WizScience.com
"Tired light" is a class of hypothetical redshift mechanisms that was proposed as an alternative explanation for the redshift-distance relationship. These model...
"Tired light" is a class of hypothetical redshift mechanisms that was proposed as an alternative explanation for the redshift-distance relationship. These models have been proposed as alternatives to the metric expansion of space of which the Big Bang and the Steady State cosmologies are the most famous examples. The concept was first proposed in 1929 by Fritz Zwicky, who suggested that if photons lost energy over time through collisions with other particles in a regular way, the more distant objects would appear redder than more nearby ones. Zwicky himself acknowledged that any sort of scattering of light would blur the images of distant objects more than what is seen. Additionally, the surface brightness of galaxies evolving with time, time dilation of cosmological sources, and a thermal spectrum of the cosmic microwave background have been observed — these effects should not be present if the cosmological redshift was due to any tired light scattering mechanism. Despite periodic re-examination of the concept, tired light has not been supported by observational tests and has lately been consigned to consideration only in the fringes of astrophysics.
Tired light was an idea that came about due to the observation made by Edwin Hubble that distant galaxies have redshifts proportional to their distance. Redshift is a shift in the spectrum of the emitted electromagnetic radiation from an object toward lower energies and frequencies, associated with the phenomenon of the Doppler Effect. Observers of spiral nebulae such as Vesto Slipher observed that these objects generally exhibited redshift rather than blueshifts independent of where they were located. Since the relation holds in all directions it cannot be attributed to normal movement with respect to a background which would show an assortment of redshifts and blueshifts. Everything is moving "away" from the Milky Way galaxy. Hubble's contribution was to show that the magnitude of the redshift correlated strongly with the distance to the galaxies.
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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/Tired+light, 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/Tired Light Video Learning Wizscience.Com
"Tired light" is a class of hypothetical redshift mechanisms that was proposed as an alternative explanation for the redshift-distance relationship. These models have been proposed as alternatives to the metric expansion of space of which the Big Bang and the Steady State cosmologies are the most famous examples. The concept was first proposed in 1929 by Fritz Zwicky, who suggested that if photons lost energy over time through collisions with other particles in a regular way, the more distant objects would appear redder than more nearby ones. Zwicky himself acknowledged that any sort of scattering of light would blur the images of distant objects more than what is seen. Additionally, the surface brightness of galaxies evolving with time, time dilation of cosmological sources, and a thermal spectrum of the cosmic microwave background have been observed — these effects should not be present if the cosmological redshift was due to any tired light scattering mechanism. Despite periodic re-examination of the concept, tired light has not been supported by observational tests and has lately been consigned to consideration only in the fringes of astrophysics.
Tired light was an idea that came about due to the observation made by Edwin Hubble that distant galaxies have redshifts proportional to their distance. Redshift is a shift in the spectrum of the emitted electromagnetic radiation from an object toward lower energies and frequencies, associated with the phenomenon of the Doppler Effect. Observers of spiral nebulae such as Vesto Slipher observed that these objects generally exhibited redshift rather than blueshifts independent of where they were located. Since the relation holds in all directions it cannot be attributed to normal movement with respect to a background which would show an assortment of redshifts and blueshifts. Everything is moving "away" from the Milky Way galaxy. Hubble's contribution was to show that the magnitude of the redshift correlated strongly with the distance to the galaxies.
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/Tired+light, 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: 29 Sep 2015
- views: 0
What Is The Evidence For The Big Bang?
Almost all astronomers agree on the theory of the Big Bang, that the entire Universe is spreading apart, with distant galaxies speeding away from us in all d......
Almost all astronomers agree on the theory of the Big Bang, that the entire Universe is spreading apart, with distant galaxies speeding away from us in all d...
wn.com/What Is The Evidence For The Big Bang
Almost all astronomers agree on the theory of the Big Bang, that the entire Universe is spreading apart, with distant galaxies speeding away from us in all d...
- published: 18 Nov 2013
- views: 10276
-
author: Fraser Cain
Perseid meteor shower will help astronomers get a better view of space
As sky-watchers marvel at the beauty of the annual Perseid meteor shower — set to peak late Sunday and early Monday — astronomers will be thanking their shoo......
As sky-watchers marvel at the beauty of the annual Perseid meteor shower — set to peak late Sunday and early Monday — astronomers will be thanking their shoo...
wn.com/Perseid Meteor Shower Will Help Astronomers Get A Better View Of Space
As sky-watchers marvel at the beauty of the annual Perseid meteor shower — set to peak late Sunday and early Monday — astronomers will be thanking their shoo...
- published: 11 Aug 2013
- views: 38
-
author: MMKVID
-
Documentary on Universe HD
For thousands of years, astronomers wrestled with basic questions about the size and age of the universe. Does the universe go on forever, or does it have an edge somewhere? Has it always existed, or did it come to being some time in the past? In 1929, Edwin Hubble, an astronomer at Caltech, made a critical discovery that soon led to scientific answers for these questions: he discovered that the u
-
Physical cosmology
Please give us a THUMBS UP if you like our videos!!!
Source:http://en.wikipedia.org/wiki/Physical_cosmology
Physical cosmology, as it is now understood, began with the development in 1915
of Albert Einstein's general theory of relativity, followed by major
observational discoveries in the 1920s: first, Edwin Hubble discovered that the
Universe contains a huge number of external galaxies beyond
-
Slipher Expanding Universe 1.03 Robert Smith
Conference on Origins of the Expanding Universe: 1912-1932
Sep 14-15, 2012 - Lowell Observatory
Presentation 1.03
Robert Smith
V.M. Slipher: Master of the Spectrograph
For some 15 years in the early years of the twentieth century, V.M. Slipher's mastery of the Lowell spectrograph enabled him to do extremely significant research in a range of areas. It is now generally agreed that his most import
-
Andromeda Galaxy
The Andromeda Galaxy /ænˈdrɒmɨdə/ is a spiral galaxy approximately 2.5 million light-years (2.4×1019 km) from Earth in the Andromeda constellation. Also know...
-
Authors@Google: Anil Ananthaswamy
Anil Ananthaswamy visits Google's San Francisco office to present his book "Edge of Physics". This event took place on March 12, 2010, as part of the Authors...
-
Nobel Laureate Professor Brian Schmidt presents "The Discovery of Cosmic Acceleration"
Find out more at http://ow.ly/wwh4E
Nobel Laureate Professor Brian Schmidt presents "The Discovery of Cosmic Acceleration" at QUT on 11 April, 2014.
From a childhood love of science to being awarded the prestigious Nobel Prize in Physics, Professor Brian Schmidt shares his "fairy-tale of a science story" that led to the startling discovery that the expansion of the universe is not slowing down
-
Galaxy
A galaxy is a massive, gravitationally bound system consisting of stars, stellar remnants, an interstellar medium of gas and dust, and dark matter, an import...
-
Alex Filippenko: "Dark Energy and the Runaway Universe", Talks at Google
We expected the attractive force of gravity to slow down the rate at which the Universe is expanding. But observations of very distant exploding stars (super...
Documentary on Universe HD
For thousands of years, astronomers wrestled with basic questions about the size and age of the universe. Does the universe go on forever, or does it have an ed...
For thousands of years, astronomers wrestled with basic questions about the size and age of the universe. Does the universe go on forever, or does it have an edge somewhere? Has it always existed, or did it come to being some time in the past? In 1929, Edwin Hubble, an astronomer at Caltech, made a critical discovery that soon led to scientific answers for these questions: he discovered that the universe is expanding.
The ancient Greeks recognized that it was difficult to imagine what an infinite universe might look like. But they also wondered that if the universe were finite, and you stuck out your hand at the edge, where would your hand go? The Greeks' two problems with the universe represented a paradox - the universe had to be either finite or infinite, and both alternatives presented problems.
After the rise of modern astronomy, another paradox began to puzzle astronomers. In the early 1800s, German astronomer Heinrich Olbers argued that the universe must be finite. If the Universe were infinite and contained stars throughout, Olbers said, then if you looked in any particular direction, your line-of-sight would eventually fall on the surface of a star. Although the apparent size of a star in the sky becomes smaller as the distance to the star increases, the brightness of this smaller surface remains a constant. Therefore, if the Universe were infinite, the whole surface of the night sky should be as bright as a star. Obviously, there are dark areas in the sky, so the universe must be finite.
But, when Isaac Newton discovered the law of gravity, he realized that gravity is always attractive. Every object in the universe attracts every other object. If the universe truly were finite, the attractive forces of all the objects in the universe should have caused the entire universe to collapse on itself. This clearly had not happened, and so astronomers were presented with a paradox.
When Einstein developed his theory of gravity in the General Theory of Relativity, he thought he ran into the same problem that Newton did: his equations said that the universe should be either expanding or collapsing, yet he assumed that the universe was static. His original solution contained a constant term, called the cosmological constant, which cancelled the effects of gravity on very large scales, and led to a static universe. After Hubble discovered that the universe was expanding, Einstein called the cosmological constant his "greatest blunder."
At around the same time, larger telescopes were being built that were able to accurately measure the spectra, or the intensity of light as a function of wavelength, of faint objects. Using these new data, astronomers tried to understand the plethora of faint, nebulous objects they were observing. Between 1912 and 1922, astronomer Vesto Slipher at the Lowell Observatory in Arizona discovered that the spectra of light from many of these objects was systematically shifted to longer wavelengths, or redshifted. A short time later, other astronomers showed that these nebulous objects were distant galaxies.
wn.com/Documentary On Universe Hd
For thousands of years, astronomers wrestled with basic questions about the size and age of the universe. Does the universe go on forever, or does it have an edge somewhere? Has it always existed, or did it come to being some time in the past? In 1929, Edwin Hubble, an astronomer at Caltech, made a critical discovery that soon led to scientific answers for these questions: he discovered that the universe is expanding.
The ancient Greeks recognized that it was difficult to imagine what an infinite universe might look like. But they also wondered that if the universe were finite, and you stuck out your hand at the edge, where would your hand go? The Greeks' two problems with the universe represented a paradox - the universe had to be either finite or infinite, and both alternatives presented problems.
After the rise of modern astronomy, another paradox began to puzzle astronomers. In the early 1800s, German astronomer Heinrich Olbers argued that the universe must be finite. If the Universe were infinite and contained stars throughout, Olbers said, then if you looked in any particular direction, your line-of-sight would eventually fall on the surface of a star. Although the apparent size of a star in the sky becomes smaller as the distance to the star increases, the brightness of this smaller surface remains a constant. Therefore, if the Universe were infinite, the whole surface of the night sky should be as bright as a star. Obviously, there are dark areas in the sky, so the universe must be finite.
But, when Isaac Newton discovered the law of gravity, he realized that gravity is always attractive. Every object in the universe attracts every other object. If the universe truly were finite, the attractive forces of all the objects in the universe should have caused the entire universe to collapse on itself. This clearly had not happened, and so astronomers were presented with a paradox.
When Einstein developed his theory of gravity in the General Theory of Relativity, he thought he ran into the same problem that Newton did: his equations said that the universe should be either expanding or collapsing, yet he assumed that the universe was static. His original solution contained a constant term, called the cosmological constant, which cancelled the effects of gravity on very large scales, and led to a static universe. After Hubble discovered that the universe was expanding, Einstein called the cosmological constant his "greatest blunder."
At around the same time, larger telescopes were being built that were able to accurately measure the spectra, or the intensity of light as a function of wavelength, of faint objects. Using these new data, astronomers tried to understand the plethora of faint, nebulous objects they were observing. Between 1912 and 1922, astronomer Vesto Slipher at the Lowell Observatory in Arizona discovered that the spectra of light from many of these objects was systematically shifted to longer wavelengths, or redshifted. A short time later, other astronomers showed that these nebulous objects were distant galaxies.
- published: 02 Nov 2014
- views: 20
Physical cosmology
Please give us a THUMBS UP if you like our videos!!!
Source:http://en.wikipedia.org/wiki/Physical_cosmology
Physical cosmology, as it is now understood, began ...
Please give us a THUMBS UP if you like our videos!!!
Source:http://en.wikipedia.org/wiki/Physical_cosmology
Physical cosmology, as it is now understood, began with the development in 1915
of Albert Einstein's general theory of relativity, followed by major
observational discoveries in the 1920s: first, Edwin Hubble discovered that the
Universe contains a huge number of external galaxies beyond our own Milky Way;
then, work by Vesto Slipher and others showed that the universe is expanding.
These advances made it possible to speculate about the origin of the Universe,
and allowed the establishment of the Big Bang Theory, by Fr. Georges Lemaitre,
as the leading cosmological model. A few researchers still advocate a handful of
alternative cosmologies; however, most cosmologists agree that the Big Bang
theory best explains observations.
wn.com/Physical Cosmology
Please give us a THUMBS UP if you like our videos!!!
Source:http://en.wikipedia.org/wiki/Physical_cosmology
Physical cosmology, as it is now understood, began with the development in 1915
of Albert Einstein's general theory of relativity, followed by major
observational discoveries in the 1920s: first, Edwin Hubble discovered that the
Universe contains a huge number of external galaxies beyond our own Milky Way;
then, work by Vesto Slipher and others showed that the universe is expanding.
These advances made it possible to speculate about the origin of the Universe,
and allowed the establishment of the Big Bang Theory, by Fr. Georges Lemaitre,
as the leading cosmological model. A few researchers still advocate a handful of
alternative cosmologies; however, most cosmologists agree that the Big Bang
theory best explains observations.
- published: 03 Apr 2015
- views: 1
Slipher Expanding Universe 1.03 Robert Smith
Conference on Origins of the Expanding Universe: 1912-1932
Sep 14-15, 2012 - Lowell Observatory
Presentation 1.03
Robert Smith
V.M. Slipher: Master of the Spec...
Conference on Origins of the Expanding Universe: 1912-1932
Sep 14-15, 2012 - Lowell Observatory
Presentation 1.03
Robert Smith
V.M. Slipher: Master of the Spectrograph
For some 15 years in the early years of the twentieth century, V.M. Slipher's mastery of the Lowell spectrograph enabled him to do extremely significant research in a range of areas. It is now generally agreed that his most important findings centered on the spectral shifts of spiral nebulae, results that were to be crucial to the development of ideas about the expanding universe. In this talk I will place Slipher’s redshift researches into the context of the contemporary debates on the nebular hypothesis and the nature of the spirals, but I will also briefly examine what brought him to Lowell, his route to mastery of the spectrograph, and briefly discuss some of his findings in other areas in order to better understand his studies of redshifts and their reception.
For more, see
http://www2.lowell.edu/workshops/slipher/
Presentation abstracts and slides at
http://www2.lowell.edu/workshops/slipher/programv2/program.html
wn.com/Slipher Expanding Universe 1.03 Robert Smith
Conference on Origins of the Expanding Universe: 1912-1932
Sep 14-15, 2012 - Lowell Observatory
Presentation 1.03
Robert Smith
V.M. Slipher: Master of the Spectrograph
For some 15 years in the early years of the twentieth century, V.M. Slipher's mastery of the Lowell spectrograph enabled him to do extremely significant research in a range of areas. It is now generally agreed that his most important findings centered on the spectral shifts of spiral nebulae, results that were to be crucial to the development of ideas about the expanding universe. In this talk I will place Slipher’s redshift researches into the context of the contemporary debates on the nebular hypothesis and the nature of the spirals, but I will also briefly examine what brought him to Lowell, his route to mastery of the spectrograph, and briefly discuss some of his findings in other areas in order to better understand his studies of redshifts and their reception.
For more, see
http://www2.lowell.edu/workshops/slipher/
Presentation abstracts and slides at
http://www2.lowell.edu/workshops/slipher/programv2/program.html
- published: 07 Feb 2014
- views: 4
Andromeda Galaxy
The Andromeda Galaxy /ænˈdrɒmɨdə/ is a spiral galaxy approximately 2.5 million light-years (2.4×1019 km) from Earth in the Andromeda constellation. Also know......
The Andromeda Galaxy /ænˈdrɒmɨdə/ is a spiral galaxy approximately 2.5 million light-years (2.4×1019 km) from Earth in the Andromeda constellation. Also know...
wn.com/Andromeda Galaxy
The Andromeda Galaxy /ænˈdrɒmɨdə/ is a spiral galaxy approximately 2.5 million light-years (2.4×1019 km) from Earth in the Andromeda constellation. Also know...
- published: 14 Jul 2014
- views: 32
-
author: Audiopedia
Authors@Google: Anil Ananthaswamy
Anil Ananthaswamy visits Google's San Francisco office to present his book "Edge of Physics". This event took place on March 12, 2010, as part of the Authors......
Anil Ananthaswamy visits Google's San Francisco office to present his book "Edge of Physics". This event took place on March 12, 2010, as part of the Authors...
wn.com/Authors Google Anil Ananthaswamy
Anil Ananthaswamy visits Google's San Francisco office to present his book "Edge of Physics". This event took place on March 12, 2010, as part of the Authors...
Nobel Laureate Professor Brian Schmidt presents "The Discovery of Cosmic Acceleration"
Find out more at http://ow.ly/wwh4E
Nobel Laureate Professor Brian Schmidt presents "The Discovery of Cosmic Acceleration" at QUT on 11 April, 2014.
From a ...
Find out more at http://ow.ly/wwh4E
Nobel Laureate Professor Brian Schmidt presents "The Discovery of Cosmic Acceleration" at QUT on 11 April, 2014.
From a childhood love of science to being awarded the prestigious Nobel Prize in Physics, Professor Brian Schmidt shares his "fairy-tale of a science story" that led to the startling discovery that the expansion of the universe is not slowing down but accelerating, and what that means for us.
wn.com/Nobel Laureate Professor Brian Schmidt Presents The Discovery Of Cosmic Acceleration
Find out more at http://ow.ly/wwh4E
Nobel Laureate Professor Brian Schmidt presents "The Discovery of Cosmic Acceleration" at QUT on 11 April, 2014.
From a childhood love of science to being awarded the prestigious Nobel Prize in Physics, Professor Brian Schmidt shares his "fairy-tale of a science story" that led to the startling discovery that the expansion of the universe is not slowing down but accelerating, and what that means for us.
- published: 07 May 2014
- views: 88
Galaxy
A galaxy is a massive, gravitationally bound system consisting of stars, stellar remnants, an interstellar medium of gas and dust, and dark matter, an import......
A galaxy is a massive, gravitationally bound system consisting of stars, stellar remnants, an interstellar medium of gas and dust, and dark matter, an import...
wn.com/Galaxy
A galaxy is a massive, gravitationally bound system consisting of stars, stellar remnants, an interstellar medium of gas and dust, and dark matter, an import...
- published: 17 Jul 2014
- views: 4
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author: Audiopedia
Alex Filippenko: "Dark Energy and the Runaway Universe", Talks at Google
We expected the attractive force of gravity to slow down the rate at which the Universe is expanding. But observations of very distant exploding stars (super......
We expected the attractive force of gravity to slow down the rate at which the Universe is expanding. But observations of very distant exploding stars (super...
wn.com/Alex Filippenko Dark Energy And The Runaway Universe , Talks At Google
We expected the attractive force of gravity to slow down the rate at which the Universe is expanding. But observations of very distant exploding stars (super...