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June 2015 - Bristol Astronomical Society
June 2015 - Bristol Astronomical Society

CS3_Ch 3 - Leon County Schools
CS3_Ch 3 - Leon County Schools

... Life Cycle of a Star (cont.) • When a star’s hydrogen supply is nearly gone, the star leaves the main sequence and begins the next stage of its life cycle. • All stars form in the same way, but stars die in different ways, depending on their masses. • Massive stars eventually become red ...
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... Gravity brings global clusters together Global clusters are large groups of stars that are held together by their own gravity. These groups of stars are very old and often have millions of members. ...
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Slide 1

r*=13.6 km MPA1 EOS
r*=13.6 km MPA1 EOS

... "None of this was realized before simply because we couldn't get to the scene of the explosion fast enough." "Swift has the unique ability to detect bursts and turn its X-ray and ultravioletoptical telescopes to the explosion's embers within minutes. As such, Swift is detecting new burst details tha ...
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Astronomy and Survey of Information

General Astronomy - Stockton University
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... sky. A small arrow appeared in the sky. He directed the torch to the letters N, S, E, W and drew the attention of the audience to them. Students observed that all the stars appearing were moving from the east to the west direction. The lecturer explained that the stars in the night sky showed as if ...
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... Red Giants: : Stars in upper right, those are colder (3000K) but very bright, so they should have large surface area ⇒ must be very big. ...
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... C. It is moving away from the Earth. D. It will live longer than a B spectral class main sequence star. E. It is the same size as a red giant star of the same temperature. 28. There are reported to be about 6,000 stars visible to the naked eye. How many of those stars would you expect to be part of ...
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... Orbital paths of inner planets and sun. Time Animation. Black, white, and red star chart colors for normal, bright, and night viewing conditions, respectively. Chart can be rotated to any of the 16 compass points and also flipped along the North - South axis. Chart can be "live, realtime", or static ...
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... a. About 40 weeks. b. About 30,000 years. c. About 30 million years. d. About 1 billion years. e. About 5 billion years. ...
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SMMP_BISANA - Infinity and Beyond
SMMP_BISANA - Infinity and Beyond

... mythology is so complete that no further distinction is made between them"--the stars were no longer merely identified with certain gods or heroes, but actually were perceived as divine(Seznec, 37-40). ...
Physics- HSC- Module 9.7 Astrophysics
Physics- HSC- Module 9.7 Astrophysics

... During the late 19th and early 20th centuries, astronomers obtained spectra and parallax distances for many stars, a powerful tool was discovered for classifying and understanding stars. Around 1911-13, Enjar Hertzsprung and Henry Norris Russell independently found that stars could be divided into t ...
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Mass and the Properties of Main Sequence Stars

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Lecture 9: Stellar Spectra

... A star’s spectrum uniquely locates the star within the overall sequence of stellar properties. Powerful tool for understanding the physics of stars. ...
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... • Stars of given type of spectrum and the same colors have the same absolute magnitude (99.9%) • Stars have different apparent magnitudes depending on their distance. • Stars behind dust clouds look redder than they are intrinsically, so… m-M=5 log d1 –5+ A(l) (i.e., the star looks fainter) ...
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Auriga (constellation)



Auriga is one of the 48 constellations listed by the 2nd-century astronomer Ptolemy and remains one of the 88 modern constellations. Located north of the celestial equator, its name is the Latin word for ""charioteer"", associating it with various mythological charioteers, including Erichthonius and Myrtilus. Auriga is most prominent during winter evenings in the Northern Hemisphere, along with the five other constellations that have stars in the Winter Hexagon asterism. Because of its northern declination, Auriga is only visible in its entirety as far as 34° south; for observers farther south it lies partially or fully below the horizon. A large constellation, with an area of 657 square degrees, it is half the size of the largest constellation, Hydra.Its brightest star, Capella, is an unusual multiple star system among the brightest stars in the night sky. Beta Aurigae is an interesting variable star in the constellation; Epsilon Aurigae, a nearby eclipsing binary with an unusually long period, has been studied intensively. Because of its position near the winter Milky Way, Auriga has many bright open clusters in its borders, including M36, M37, and M38, popular targets for amateur astronomers. In addition, it has one prominent nebula, the Flaming Star Nebula, associated with the variable star AE Aurigae.In Chinese mythology, Auriga's stars were incorporated into several constellations, including the celestial emperors' chariots, made up of the modern constellation's brightest stars. Auriga is home to the radiant for the Aurigids, Zeta Aurigids, Delta Aurigids, and the hypothesized Iota Aurigids.
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