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Explorations: An Introduction to Astronomy 2e Arny | |||||
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| Key Terms |
Chapter 7: Survey of the Solar System |
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Accretion (229) |
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addition of matter to a body. Examples are
gas falling onto a star and asteroids colliding and sticking together. |
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asteroid belt (222) |
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a region between the orbits of Mars and Jupiter
in which most of the Solar Systems asteroids are located. |
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asteroids (222) |
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a small, generally rocky, solid body orbiting
the Sun and ranging in diameter from a few meters to hundreds of kilometers. |
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Bodes law (224) |
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a numerical expression for the approximate
distances of most of the planets from the Sun. |
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Comets (222) |
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a small body in orbit around the Sun, consisting
of a tiny, icy core and a tail of gas and dust. The tail forms only when
the comet is near the Sun. |
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Condensation (228) |
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the change from gas to liquid. This occurs when a gas cools and its molecules stick together to form liquid
or solid particles. |
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inner planets (220) |
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a planet orbiting in the inner part of the
Solar System. Sometimes taken to mean Mercury, Venus, Earth, and Mars. |
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interstellar cloud (227) |
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a cloud of gas and dust in between the stars.
Such clouds may be many light years in diameter. |
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interstellar grains (227) |
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microscopic solid dust particles in interstellar
space. These grains absorb starlight, making distant stars appear dimmer
than they truly are. |
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Jovian planets (221) |
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one of the giant, gaseous planets: Jupiter,
Saturn, Uranus, and Neptune. The name Jovian was chosen because Jupiters
structure is representative of the other three. |
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Oort cloud (222) |
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a vast region in which comet nuclei orbit. This cloud
lies far beyond the orbit of Pluto. |
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outer planets (220) |
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a planet whose orbit lies in the outer part
of the Solar System. Jupiter, Saturn, Uranus, Neptune, and Pluto are outer
planets. |
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planetesimal (230) |
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one of the numerous small, solid bodies that, when gathered together, form a planet. |
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solar nebula (228) |
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the rotating disk of gas and dust from which
the Sun and planets formed. |
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solar nebula hypothesis (227) |
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the hypothesis that the Solar System formed
from a rotating cloud of gas and dust, the solar nebula |
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Solar System (219) |
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the Sun, planets, their moons, and other
bodies that orbit the Sun. |
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terrestrial planets (221) |
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a rocky planet similar to the Earth in size and structure. The terrestrial planets are Mercury, Venus, Earth, and Mars. |
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