Difference between revisions of "M-type asteroids"
Jump to navigation
Jump to search
m |
(update for navbox) |
||
| Line 1: | Line 1: | ||
| − | |||
'''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> | '''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> | ||
| Line 10: | Line 9: | ||
<references/> | <references/> | ||
| + | |||
| + | {{Solarsystem}} | ||
[[Category:Astronomy]] | [[Category:Astronomy]] | ||
Revision as of 12:21, July 16, 2007
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]
References
| |||||||||||||||||||||||||||||
