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13 Cards in this Set
- Front
- Back
achondrite
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Stony meteorite containing no chondrules or volatiles. (p. 455)
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carbonaceous chondrite
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Stony meteorite that contains both chondrules and volatiles. These chondrites may be the least-altered remains of the solar nebula still present in the solar system. (p. 455)
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chondrite
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A stony meteorite that contains chondrules. (p. 455)
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chondrule
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Round, glassy body found in some stony meteorites. Believed to have solidified very quickly from molten drops of silicate material. (p. 455)
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coma
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The glowing head of a comet. (p. 464)
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dust tail
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A comet tail composed of dust released from the nucleus and pushed away by the pressure of sunlight. Also known as a type II tail. (p. 464)
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gas tail
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A comet tail composed of ionized gas atoms released from the nucleus and carried outward by the solar wind. Also called a type I comet tail. (p. 464)
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meteor shower
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A multitude of meteors that appear to come from the same region of the sky. Believed to be caused by comet debris. (p. 456)
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Oort cloud
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The hypothetical source of comets. A swarm of icy bodies believed to lie in a spherical shell extending to 100,000 AU from the sun. (p. 462)
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stony-iron meteorite
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A meteorite composed of stone and iron mixed together. (p. 455)
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type I comet tail
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See gas tail.
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type II comet tail
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See dust tail.
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Widmanstatten pattern
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Bands in iron meteorites due to large crystals of nickel-iron alloys. (p. 455)
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