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J-type asteroids : ウィキペディア英語版
J-type asteroid
J-type asteroids are asteroids with spectra similar to that of diogenite meteorites and so, presumably, to the deeper layers of the crust of 4 Vesta.
Their spectra are rather similar to that of the V-type asteroids but have a particularly strong 1 μm absorption band.
Examples are 2442 Corbett, 3869 Norton, 4005 Dyagilev, and 4215 Kamo.〔R. P. Binzel and S. Xu ''Chips off of asteroid 4 Vesta: Evidence for the parent body of basaltic achondrite meteorites'', Science, Vol. 260, p. 186 (1993).〕
==See also==

*Asteroid spectral types

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「J-type asteroid」の詳細全文を読む



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