Mid-infrared spectra of comets P/Borrelly, P/Faye, and P/Schaumasse

被引:41
作者
Hanner, MS [1 ]
Lynch, DK [1 ]
Russell, RW [1 ]
Hackwell, JA [1 ]
Kellogg, R [1 ]
Blaney, D [1 ]
机构
[1] AEROSP CORP,LOS ANGELES,CA 90009
基金
美国国家航空航天局;
关键词
D O I
10.1006/icar.1996.0209
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A 10 mu m silicate emission feature has been discovered in the spectra of comets P/Borrelly and P/Faye at R similar to 1.5 AU. These are the first short period comets in which silicate emission has definitely been detected. The broad emission features are about 25% above the continuum. No emission feature was present in the spectrum of P/Schaumasse; it is possible that the nucleus of P/Schaumasse was directly detected. If all of the observed flux originated from the nucleus, then the effective radius is about 3 km; the observed color temperature is consistent with a rapidly rotating nucleus. We present models that show how the shape of the silicate feature can depend on the way in which silicate and absorbing material are mixed in the grains. (C) 1996 Academic Press, Inc.
引用
收藏
页码:344 / 351
页数:8
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