Difference between revisions of "M-type asteroids"
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(New page: '''M-type asteroids''' are a type of asteroid or minor planet. Asteriods are generally classified into broad categories such as C-type, S-type, or M-type according to their brightness and...) |
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| + | '''M-type asteroids''' are a type of asteroid or minor planet. Asteroids are generally classified into broad categories such as C-type, S-type, or M-type according to their brightness and color. Brightness, or albedo, is a measurement of how well the object reflects light. Albedo ranges from 0 (perfectly black) to 1 (perfectly reflecting).<ref>http://www.planetary.org/explore/topics/near_earth_objects/asteroids_and_comets/facts.html</ref> | ||
These mid-region main belt objects are relatively bright, with albedos ranging from 0.10 to 0.18. Composition is apparently dominated by metallic iron. | These mid-region main belt objects are relatively bright, with albedos ranging from 0.10 to 0.18. Composition is apparently dominated by metallic iron. | ||
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== References == | == References == | ||
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<references/> | <references/> | ||
[[Category:Astronomy]] | [[Category:Astronomy]] | ||
Revision as of 04:51, May 18, 2007
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M-type asteroids are a type of asteroid or minor planet. Asteroids are generally classified into broad categories such as C-type, S-type, or M-type according to their brightness and color. Brightness, or albedo, is a measurement of how well the object reflects light. Albedo ranges from 0 (perfectly black) to 1 (perfectly reflecting).[1]
These mid-region main belt objects are relatively bright, with albedos ranging from 0.10 to 0.18. Composition is apparently dominated by metallic iron. M-type asteroids inhabit the main belt's middle region. .[2] They make up some 10% of the total asteroid population.[3]