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Astronomy Chapter 17 – Galaxies A. Main Ideas 1. Discovering
Astronomy Chapter 17 – Galaxies A. Main Ideas 1. Discovering

... use the method of standard candles to measure the distance to distant galaxies. Using the inverse-square law and the known luminosity of Cepheid variables scientists are able to reasonable measurements of the distances involved. • Redshift and the Hubble Law ⇒ In the 1920s, astronomers discovered th ...
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doc

... THE HERTZSPRUNG-RUSSELL DIAGRAM The story may be said to begin at Harvard College Observatory in the 1880s when E. C. Pickering and Annie Cannon began to analyse the emission spectra of the visible stars. The stars they examined were placed into several ‘spectral classes’, each class being designate ...
1 - Piscataway High School
1 - Piscataway High School

... enough, helium fusion begins to make energy, and the temperature rises, but pressure does not increase because the gas is degenerate. The higher temperature increases the helium fusion even further, and the result is a runaway explosion called the helium flash in which, for a few minutes, the core o ...
CELESTIAL MANUAL:CELESTIAL MANUAL
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Introduction to Astrotheology
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it now and get started on your discovery
it now and get started on your discovery

... Edwin Powell Hubble was an American astronomer who helped form the field of extragalactic astronomy, which means studying objects outside the Milky Way galaxy. Hubble’s discovery that things exist outside the Milky Way galaxy was revolutionary but debated. One of his findings, known as “Hubble’s Law ...
Precision age indicators that exploit chemically peculiar stars
Precision age indicators that exploit chemically peculiar stars

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The Vampire Stars - d_smith.lhseducators.com
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Doppler Effect Demo
Doppler Effect Demo

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ppt - SLAC
ppt - SLAC

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the magellanic clouds newsletter - Keele University Astrophysics
the magellanic clouds newsletter - Keele University Astrophysics

... have a binary frequency that decreases towards the core, while the binary frequency for stars of similar mass in NGC 1805 is flat with radius, or perhaps bimodal (with a peak in the core). We show here, through detailed N -body modeling, that both clusters could have formed with the same primordial ...
November, 2015 - The Baton Rouge Astronomical Society
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... One big early surprise (1995) was the ground-based discovery of “hot Jupiters:” gas giants the size of Jupiter in orbits around their parent stars much closer than Venus—or even Mercury—is to the Sun. How does something that massive form so close to a parent star? Would there have been enough materi ...
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“Breakthroughs” of the 20th Century
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... in 1897 and this transformed spectroscopy and introduced plasma and magnetohydrodynamic physics and astro-chemistry. Einstein’s E = mc2, solved the problem of stellar energy generation and spawned the study of elemental nuclear synthesis. Large telescopes led to a boom in astronomical spectroscopic ...
1Barycenter Our solar system consists of the Sun and the
1Barycenter Our solar system consists of the Sun and the

... km below the surface of the Earth. This is because the Earth is far more massive than the Moon and it is this common center of mass around which the Earth and the Moon seem to go around. The International Astronomical Union (IAU) does not consider the Earth-Moon system as a double-planet system, sin ...
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... object with a spectrum much like a dim star high red shift enormous recessional velocity huge distance (from Hubble’s Law) enormously luminous compact physical size powered by supermassive black hole often produce huge jets ...
Question paper - Unit A183/02 - Module P7 - Higher tier
Question paper - Unit A183/02 - Module P7 - Higher tier

... OCR is committed to seeking permission to reproduce all third-party content that it uses in its assessment materials. OCR has attempted to identify and contact all copyright holders whose work is used in this paper. To avoid the issue of disclosure of answer-related information to candidates, all co ...
Chapter 12: The Life Cycle of Stars (contʼd)
Chapter 12: The Life Cycle of Stars (contʼd)

... ball of neutrons only a few km across!! ...
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Corvus (constellation)



Corvus is a small constellation in the Southern Celestial Hemisphere. Its name comes from the Latin word ""raven"" or ""crow"". It includes only 11 stars with brighter than 4.02 magnitudes. One of the 48 constellations listed by the 2nd-century astronomer Ptolemy, it remains one of the 88 modern constellations. The four brightest stars, Gamma, Delta, Epsilon, and Beta Corvi from a distinctive quadrilateral in the night sky. The young star Eta Corvi has been found to have two debris disks.
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