Compositional variation on the surface of Centaur 8405 Asbolus

被引:25
作者
Kern, SD
McCarthy, DW
Buie, MW
Brown, RH
Campins, H
Rieke, M
机构
[1] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[2] Lowell Observ, Flagstaff, AZ 86001 USA
[3] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
[4] Res Corp, Tucson, AZ 85711 USA
基金
美国国家航空航天局;
关键词
infrared : solar system; Kuiper Belt; Oort Cloud;
D O I
10.1086/312932
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Near-infrared 1-2 mum spectra of the Centaur 8405 Asbolus (1995 GO) have been obtained using the Hubble Space Telescope near-infrared camera and multiobject spectrometer. Strong and variable absorption features indicate a significantly inhomogeneous surface characterized by water ice mixed with additional unknown constituents. Over a 1.7 hr interval, the observed spectra varied from a nearly featureless spectrum to a very complicated absorption spectrum, and the integrated flux varied in a manner consistent with previous light-curve observations. The accepted rotation period of 8.9351 hr assumes a shape-dominated light curve. Our observations indicate that the light curve may in fact be dominated by a relatively bright spot with a period of 4.47 hr, i.e., half the previous value.
引用
收藏
页码:L155 / L159
页数:5
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