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Death of a medium sized star |
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It becomes a white dwarf, expels its outer layer, when the fusion turns off there is not enough matter to sustain itself |
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They run out of stuff to fuse with, it takes energy to fuse and iron takes away from star so star collapses and blows its outer layer creating a supernova black hole or neutron |
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Exotic state of matter difficult to compress to smaller mass Electron White dwarf neutron star |
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the material surrounding a medium mass star during its death |
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No hydrogen in spectra When a binary system strips the outer hydrogen layer from a massive star onto a second star |
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No Hydrogen in spectra When a white dwarf in a binary star steals mass from companion star and reaches mass of 1.4 solar masses |
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Have hydrogen lines and appear to be from the collapse and explosion of a massive star |
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The debris left in space after a supernova |
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1.4 neutron star and what dwarf |
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The sudden brightening of a star that makes it seem to be a new star |
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A star made up of degenerate neutron star matter, has a strong magnetic field and is the size of the sun in mass |
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a mass that has collapsed to such a small volume that its gravity prevents escape of all things even light |
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A source of precisely timed radio bursts, believed to be spinning neutron stars. |
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The explanation of a pulsar as a spinning neutron star sweeping beams of electromagnetic radiation around the sky |
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the center or point where all matter is concentrated |
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The radius to which all the mass of an object needs to be packed into to become a black hole |
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The boundary in a black hole where nothing can escape |
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The slowing of clocks or time in strong gravitational fields |
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A large system of stars, star clusters, gas, dust, and nebulae orbiting a common center of mass |
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E0-E7 no gas dust, hot bright stars seen |
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SA, SB, SC dust, gas and hot blue young stars seen |
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bar structure in the neucleus (milky way) |
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has a nucleus but no spiral, no gas or dust is visible either |
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All remaining unclassified galaxies |
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a unit of distance=1 million pc |
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the amount by which you look into the past when you look at a distant galaxy time=distance to galaxy in ly |
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Hubble Law and importance |
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The linear relation between the distances to galaxies and their velocity of recession it is proof the galaxy is expanding and we can therefore determine the distance to galaxies |
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How can a type Ia supernova be used to determine distances to galaxies |
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They all reach the same absolute mag. -17 Find apparent mag. and then you can get the distance |
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The study of large scale structure and the evolution of the universe |
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If you look in any direction you line of sight will eventually fall onto a star |
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Theory of origin of the universe at high density and high temperature |
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Electrons connect with protons and lets light travel 3,000K |
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Period after the big bang before stars ignited after recombination |
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The stage in the early history of the universe when ultra violet photons from the first stars ionized the gas filling space |
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the universe is uniform on the large scale that it IS |
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The universe looks the same in any direction That it LOOKS |
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any observer in the universe sees the same thing |
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A finite sphere with no boundary |
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an infinite saddle with no boundary |
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an infinite with no boundaries what our universe actually is |
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The average density of the universe needed to make it flat |
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Non luminous matter that is detected only by its gravitational influence |
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The hypothesis that the planets formed from the same cloud of gas ad dust that formed the sun |
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small dense rocky little to no atmosphere (inner planets) mercury, Venus, mars, earth |
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large low density thick atmosphere liquid interior (outer planets) Saturn, Uranus, Neptune, Jupiter |
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Small rocky world mostly between mars and jupiter in the asteroid belt |
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A small bit of matter heated by friction to incandescent vapor as it falls into Earth's Atmosphere |
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A Meteor that survives its passage through the atmosphere and strikes the ground |
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A meteor in space before it enters earths atmosphere |
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On of the small icy bodies that orbit the sun and produce tails of gas and dust when they approach the sun |
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a planet orbiting a star other than the sun |
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