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Test #1
Test #1

... 27) A shift in the direction of an object caused by a change in the position of an observer is called a) parallax, b) precession, c) the Coriolis effect, d) epicycle motion 28) The angular distance of an object from the horizon is its a) latitude, b) declination, c) altitude, d) right ascension 29) ...
A Sense of Scale - Young Scientists Journal
A Sense of Scale - Young Scientists Journal

... black hole could be tens of billions of times as massive. The largest known black hole is at the centre of the OJ 287 galaxy and has a mass estimated at 18 billion solar masses. It can be hard to imagine how large a billion is, but help is at hand; consider that a billion minutes ago the Roman Empir ...
ch16 b - Manasquan Public Schools
ch16 b - Manasquan Public Schools

...  This radiation was predicted by the theory.  The radiation has shown a cooling trend which has allowed scientist to measure the overall temperature of the universe. (2.7 K)  Also the amount hydrogen (most common ...
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07optics_8inch_orion

... • Assuming aperture of 6.5 mm smallest detail eye can possibly resolve due to diffraction limit would be 20”. • Acuity of Eye: Fovea of eye has best resolution (this is what you are using to read), but spacing of ...
Stellar Evolution
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Universal redshift, the Hubble constant The cosmic background
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... decoupled photons allow gravitational collapse and creation of galaxies photons scattered for the last time and continue expanding destiny of some of the photons was to be measured by us One can see it easier – since λM ∼ 1/T , TD/TC = LC /LD CMB is the picture of the Universe when it was 2000 (^3) ...
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... likely companions. With medium resolution (R~5500) GNIRS and NIFS data we estimate effective temperatures, surface gravities and veiling from the relative and absolute depths of photospheric lines. High resolution (R~18,000) spectra of a few late-type stars better constrain temperature, gravity and ...
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Astronomy Study Guide
Astronomy Study Guide

... The apparent motions of the Sun, Moon, Planets, and stars across the sky can be explained by Earth’s rotation and revolution. Earth’s rotation on its axis causes the length of one day to be approximately 24 hours. This rotation also causes the Sun and Moon to appear to rise along the eastern horizo ...
Themes of the Planetarium (PDF:81 KB)
Themes of the Planetarium (PDF:81 KB)

... Best chance to see Saturn in this year will be early summer. You can see the much-loved Saturn's rings with a simple telescope. Why don't you get one and enjoy star-watching. July: "Tanabata" star festival and the Milky Way" The Milkey Way separating "Orihimeboshi (Vega)" and "Hikoboshi (Altair)" in ...
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“Crossroads of Astronomy.” Talk about Five Remarkable
“Crossroads of Astronomy.” Talk about Five Remarkable

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Galileo, Brahe, and Kepler - Pennsylvania State University
Galileo, Brahe, and Kepler - Pennsylvania State University

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Click here to 2016 The Universe Diagnostic Test
Click here to 2016 The Universe Diagnostic Test

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december 2010 - Holt Planetarium
december 2010 - Holt Planetarium

... On December 21 there is a total eclipse of the Moon. The total phase of this eclipse lasts for just over 72 minutes, with the partial umbral eclipse spanning almost 3.5 hours. All stages of the total eclipse of the Moon are visible from North America and the eastern Pacific. South America will see t ...
december 2010 - Holt Planetarium
december 2010 - Holt Planetarium

... On December 21 there is a total eclipse of the Moon. The total phase of this eclipse lasts for just over 72 minutes, with the partial umbral eclipse spanning almost 3.5 hours. All stages of the total eclipse of the Moon are visible from North America and the eastern Pacific. South America will see t ...
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Chapter 6 Telescopes: Portals of Discovery
Chapter 6 Telescopes: Portals of Discovery

... •  Why do we put telescopes into space? –  Forms of light other than radio and visible do not pass through Earth’s atmosphere. –  Also, much sharper images are possible because there is no turbulence. ...
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Stars, Galaxies and the Universe FORM A

... 40. If you were to move the Earth to half its current distance from the Sun (to 0.5 AU), how would the gravitational pull on the Earth by the Sun change? (a) it would be ¼ as strong at 0.5 AU (b) it would be 4x as strong at 0.5 AU (c) it would be ½ as strong at 0.5 AU (d) it would be 2x as strong a ...
Price List Galileo Telescope Makers
Price List Galileo Telescope Makers

... payable at Mumbai. Local cheques are accepted but order will be processed after realization. Bank Transfer: You can directly deposit / transfer the funds to our bank accounts with ICICI / CITI / HDFC/ HSBC banks across the country. Call / email for the bank details. Personal Collect: From our Mumbai ...
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Level :3ASS3-4 School Year: 2009/2010 English

... Our solar system consists of an average star we call the Sun, the planets Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and Pluto. It includes also the satellites of the planets; numerous comets, asteroids, and meteoroids. The moon is the satellite rotating around the Erath and the ...
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... late to resolve “The” comet (at this time, I no longer own the big reflector – had to sell it to buy college supplies for my eldest son many years ago). But the Astroscan did not resolve Mars as I thought it should have. Even with Edmund Scientifics’ bulky Barlow lens, and some very good viewing con ...
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International Ultraviolet Explorer



The International Ultraviolet Explorer (IUE) was an astronomical observatory satellite primarily designed to take ultraviolet spectra. The satellite was a collaborative project between NASA, the UK Science Research Council and the European Space Agency (ESA). The mission was first proposed in early 1964, by a group of scientists in the United Kingdom, and was launched on January 26, 1978 aboard a NASA Delta rocket. The mission lifetime was initially set for 3 years, but in the end it lasted almost 18 years, with the satellite being shut down in 1996. The switch-off occurred for financial reasons, while the telescope was still functioning at near original efficiency.It was the first space observatory to be operated in real time by astronomers who visited the groundstations in the United States and Europe. Astronomers made over 104,000 observations using the IUE, of objects ranging from solar system bodies to distant quasars. Among the significant scientific results from IUE data were the first large scale studies of stellar winds, accurate measurements of the way interstellar dust absorbs light, and measurements of the supernova SN1987A which showed that it defied stellar evolution theories as they then stood. When the mission ended, it was considered the most successful astronomical satellite ever.
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