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Essay of the hubble telescope
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Essay of the hubble telescope
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Astrophysics
Astrophysics in the 20th Century
Hubble's Discoveries:
Edwin Hubble (1889-1953) is a central figure in the development of observational cosmology. From 1922 to 1936 Hubble solved four of the central problems in cosmology.
From 1922 to 1925 Hubble devised a classification system for galaxies by grouping them according to their content, distance, shape, size, and brightness. The galaxy classification system had become the Hubble morphological (The study of form, structure and the like. ) sequence of galaxy types. Previous to this, no satisfactory system existed, thus Hubble's powerful, yet simple scheme was an incredibly important scientific achievement.
By his discovery of Cepheids in 1924 and with parallel work in M33 and M31, Hubble proved decisively that these stars are outside of our galaxy. Thus bringing to a close the debate of whether there are other galaxies in the Universe beyond the Milky Way.
From 1926 to 1936 Hubble spent studying the distribution of galaxies and thus determining them to be homogeneous in distance. Hubble's 1934 paper was so detailed and convincing that it brought the problem of the mean galaxy distribution, which was by then more than 100 years old, to a close. Attempts were then made to measure the radius of curvature of space.
By 1936 Hubble, together with Milton Humason, showed beyond doubt the linear velocity-distance relationship (redshift-distance relationship). This led to the formulation of the Empirical Redshift Distance Law for galaxies, now days known as Hubble's Law.The law states that the greater the distance between any two galaxies, the greater their relative speed of separation ie Recessional Velocity = Hubble's Co...
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...se." Internet WWW page at URL www.pd.astro.it/E-MOSTRA/NEW/A9003DES.HTM
"The pocket Macquarie Dictionary." General Editor: JRL Bernard. NSW, Australia: The Jacaranda Press, 1997.
"The ultimate fate of the Universe." Internet WWW page at URL http://en.wikipedia.org/Ultimate_fate_of_the_Universe
"Will this Universe ever end?." Internet WWW page at URL www.closertotruth.com/topics/universemeaning/213/213transcrips.html
Internet WWW page at URL http://oposite.stsci.edu/pubinfo/spacecraft/Primer/Hubble_Expand.htm
Internet WWW page at URL www.howstuffworks.com
Internet WWW page at URL www.spacetoday.org/History/MillenniumTimeline/20thCenturyLate.html
One of the most electrifying pictures of all, the Hubble Deep Field image began literally as a shot in the dark: the sum of 342 exposures taken with Hubble's Wide Field and Planetary Camera 2 in December 1995 of a black speck of northern sky. Although the Shoemaker-Levy 9 comet impact on Jupiter may have generated a bigger media splash, astronomers still are agog over the Deep Field. Aides to Vice President Al Gore ordered a Deep Field poster from the Space Telescope Science Institute (STScI), which manages the Hubble's science program under contract with NASA. Borrowing a page from Mikulski, Gore plans to use the Deep Field poster to promote scientific research in the next millennium. In an age of cost-cutting and smaller-is-preferred, the $3 billion Hubble has demonstrated that bigger can be better: The telescope attracted 1,298 proposals for observing time during its next annual cycle that began in July, an increase of 30 percent from the previous cycle and more than had been received by any other U.S. telescope or NASA project. Ever.
Two men named Harlow Shapley and Heber Curtis has a debate in 1920 that is still important today for changing how we think about galaxies. They talked about five important things. The first thing they debated was how big our galaxy, the Milky Way, is. Shapley said that the Milky Way was much bigger than we first thought, 100,000 light-years across, and that, because it was that big, it had to be the only one. Curtis said the the Milky Way was smaller than that, and that other galaxies existed past ours. They were both right and both wrong. Shapley was right about the size of the Milky Way, and Curtis was right about there being many more galaxies in the universe.
Kuhn, T. S., 1957. The Copernican Revolution: Planetary Astronomy in the Development of Western Thought. Londen: Harvard University Press.
Waller, William H. The Milky Way: An Insider's Guide. Princeton, N.J: Princeton UP, 2013. 42+. Print.
Hubble, Edwin. 1929, "A Relation between Distance and Radial Velocity among Extra-Galactic Nebulae" Proceedings of the National Academy of Sciences of the United States of America, Volume 15, Issue 3, pp. 168-173
lifetime. Some of Edwin Hubble's greatest accomplishments were: Edwin Hubble proposed a classification system for nebulae, which are fuzzy little patches of light that are up in the sky. He discovered a variable star, called the Cepheid. It is located in the Andromeda Nebulae. Edwin Hubble settled decisively the question of the nature of the galaxies. Edwin Hubble's distribution of galaxies was determined to be homogeneous in distance. Edwin wanted to classify the galaxies according to their content, distance, shape, and pattern of brightness. By observing redshifts Edwin saw that galaxies were moving away from each other at a rate constant to the distance between them (this is known as Hubble's Law).
Albert Einstein’s discoveries and theories have had a positively enormous effect on the world. Some of Einstein’s biggest impacting discoveries and theories are the theories of Special and General relativity, the Theory of Relativity, Brownian motion, the discovery of the photon, and Einstein’s creation of the equation E = MC^2. Perhaps Einstein’s most beneficial discovery is his formulation of E = MC^2 which is crucial for space-flight and can help today’s scientist in gathering knowledge about our universe.
In the article from the official NASA website, NASA gives a list of Hubble’s accomplishments, which gives the reader a comprehensive picture of Hubble’s importance. Hubble has not only given astronomers the most detailed images of outer-space in existence, but also taug...
Carl Sagan: astronomer, astrophysicist, cosmologist, author, skeptic, and visionary. The middle of the twentieth century was clad in scientific advancements that opened up the realm of our universe to the world. At the head of this exploration was Carl Sagan, a pioneer of sorts. Aside from his countless contributions to the scientific community, he backed a new understanding of the cosmos to the more pedestrian population of the world.
Just recently a major discovery was found with the help of a device known as The Hubble Telescope. This telescope has just recently found what many astronomers believe to be a black hole, After being focuses on a star orbiting empty space. Several pictures of various radiation fluctuations and other diverse types of readings that could be read from that area which the black hole is suspected to be in.
The Orion Nebula is a spectacular sight. Consequently, it has been a preferred target of the Hubble Space Telescope (HST) over recent years. The HST has provided a great deal of insight into the complicated process of star formation. In June of 1994, C.
By 1936, astronomers had realized that the hazy balls they sometimes saw in their telescopes, which looked like stars obscured by gas, were actually galaxies (Hibbison).
The Hubble Telescope is the world’s first space-based optical telescope. The Hubble telescope received its name from American astronomer Dr. Edwin P. Hubble. Dr. Hubble confirmed an ever expanding universe which provided the basic foundation of the Big Bang theory. The first concept of the Hubble telescope came from Lyman Spitzer in 1946, who at that time was a professor and researcher at Yale University. In 1946, Professor Spitzer believed that Earth’s atmosphere blurs and distorts light, and a space orbited telescope would be able to overcome this problem.
The first person to ever observe the Milky Way was Greek philosopher, Democritus, who said the galaxy may consist of distant stars. In 1610, Galileo Galilei used a telescope to study the Milky Way and came to the conclusion that it was composed of billions and billions of faint stars. Then, in 1750, Thomas Wright c...