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・ P-SCH
・ P-selectin
・ P-selectin glycoprotein ligand-1
・ P-series fuels
・ P-site
・ P-space
・ P-Square
・ P-Square discography
・ P-stable group
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・ P-Toluic acid
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P-type asteroid
・ P-type ATPase
・ P-type calcium channel
・ P-Unit
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・ P-Vine Records
・ P-wave
・ P-wave modulus
・ P-Xylene
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・ P-y method
・ P.
・ P. A. Antony
・ P. A. Ariyaratne


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P-type asteroid : ウィキペディア英語版
P-type asteroid
P-type asteroids have low albedo and a featureless reddish spectrum. It has been suggested that they have a composition of organic rich silicates, carbon and anhydrous silicates, possibly with water ice in their interior. P-type asteroids are found in the outer asteroid belt and beyond. There are 33 P-type asteroids.〔
==Taxonomy==
An early system of asteroid taxonomy was established in 1975 from the doctoral thesis work of David J. Tholen. This was based upon observations of a group of 110 asteroids. The U-type classification was used as a miscellaneous class for asteroids with unusual spectra that didn't fit into the C and S-type asteroid classifications. In 1976, some of these U-type asteroids with unusual moderate albedo levels were labeled as M-type.
Around 1981, an offshoot of the M-type asteroid branch appeared for minor planets that had a spectra that was indistinguishable from M-type, but they also had low albedo that did not lie within the M-type criteria. These were initially labeled X-type asteroids, then type DM (dark M) or PM (pseudo-M), before acquiring their own unique classification as P-type asteroids (where the P indicates "pseudo-M").〔

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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