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O-型小行星非常罕見，光譜類似於不尋常的小行星3628 Boznemcová，是與一般球粒隕石L6和LL6最為吻合的小行星。它們的光譜在0.75 μm有很深吸收功能的longward。
- S. J. Bus and R. P. Binzel Phase II of the Small Main-belt Asteroid Spectroscopy Survey: A feature-based taxonomy, Icarus, Vol. 158, pp. 146 (2002).
_mathilde.jpg){kind=small} | 這是一篇有關主帶小行星的小作品。您可以透過編輯或修訂擴充其內容。 |
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