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The star and the trees prostrate
The star and the trees prostrate

... core that eventually cools and contracts gravitationally to about the size of the Earth. The result is a white dwarf: the more massive it is, the greater its inward gravitational pull, and the smaller it becomes. A teaspoonful of white dwarf material would weigh five-and-a-half tons or more in the E ...
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... • Each protostar will turn into one main sequence star • 90% of stars are main sequence stars • Vary in surface temperature and absolute magnitude ...
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HW #8 Answers (Due 10/21)

... Cloud collision with spiral arms – As molecular clouds orbit in a spiral galaxy they pass they periodically pass through an over density of gas which is related to the spiral density wave in the galaxy. When this happens, the interaction between the cloud and the spiral density wave can compress a c ...
Physical Science Laboratory: Skyglobe
Physical Science Laboratory: Skyglobe

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Lecture 31 - 2 The Death of Stars: Stellar Recycling Phase 3 -
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... • Helium core shrinks by a factor of ~30 to a size approximately that of the Earth • Hydrogen “burning” (i.e. H→He+energy release) continues in a thin shell just outside collapsing He core. • total luminosity of star increases by 100 to 1000 due to renewed H burning + heating of collapsing core. • o ...
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... But three or four times in every thousand years occurs something beside which even a nova pales into total insignificance. When a star becomes a supernova, it may for a little while outshine all the massed suns of the galaxy. The Chinese astronomers watched this happen in AD 1054, not knowing what i ...
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PDF Version

... varies with the star’s intrinsic brightness. The star’s apparent brightness, which is the brightness that we can see ourselves, is equal to the intrinsic brightness divided by the square of the distance from us to the star. Astronomers used Cepheid variables in a nearby galaxy, which are all about t ...
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... Mizar, 88 light years distant, is the middle star in the handle of the Big Dipper. It was the first binary star system to be imaged with a telescope. Spectroscopic observations show periodic Doppler shifts in the spectra of Mizar A and B, indicating that they are each binary stars. But they were too ...
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... A Star’s brightness, depends on its distance from us. - there are stars much more luminous than our sun in the sky, however, they are not nearly as bright because they are far away. - Scientists will use apparent brightness and flux interchangeably. A star’s apparent brightness = ...
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September 2013 - Joliet Junior College

... The three stars that makeup the Summer Triangle are directly above at midevening and the Milky Way runs between them. Cassiopeia is above the Summer Triangle and looks like a “W” of stars. The Milky Way runs from Cassiopeia through the Triangle down to Sagittarius at the horizon. Sagittarius looks l ...
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... The star Rigel is about 100,000 times brighter than the Sun and belongs to spectral type B8. The star Sirius B is about 3000 times dimmer than the Sun and also belongs to spectral type B8. Which star has the greatest surface temperature? 1. Rigel 2. Sirius B 3. They have the same temperature. 4. Th ...
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Perseus (constellation)



Perseus, named after the Greek mythological hero Perseus, is a constellation in the northern sky. It was one of 48 listed by the 2nd-century astronomer Ptolemy and among the 88 modern constellations defined by the International Astronomical Union (IAU). It is located in the northern celestial hemisphere near several other constellations named after legends surrounding Perseus, including Andromeda to the west and Cassiopeia to the north. Perseus is also bordered by Aries and Taurus to the south, Auriga to the east, Camelopardalis to the north, and Triangulum to the west.The galactic plane of the Milky Way passes through Perseus but is mostly obscured by molecular clouds. The constellation's brightest star is the yellow-white supergiant Alpha Persei (also called Mirfak), which shines at magnitude 1.79. It and many of the surrounding stars are members of an open cluster known as the Alpha Persei Cluster. The best-known star, however, is Algol (Beta Persei), linked with ominous legends because of its variability, which is noticeable to the naked eye. Rather than being an intrinsically variable star, it is an eclipsing binary. Other notable star systems in Perseus include X Persei, a binary system containing a neutron star, and GK Persei, a nova that peaked at magnitude 0.2 in 1901. The Double Cluster, comprising two open clusters quite near each other in the sky, was known to the ancient Chinese. The constellation gives its name to the Perseus Cluster (Abell 426), a massive galaxy cluster located 250 million light-years from Earth. It hosts the radiant of the annual Perseids meteor shower—one of the most prominent meteor showers in the sky.
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