Detection of thermal emission from 1993 SC - First results

被引：2

作者：

Thomas, N ^{[1
]}

Eggers, S ^{[1
]}

Ip, WH ^{[1
]}

Lichtenberg, G ^{[1
]}

Fitzsimmons, A ^{[1
]}

Keller, HU ^{[1
]}

Williams, I ^{[1
]}

Hahn, G ^{[1
]}

Nauer, H ^{[1
]}

机构：

[1] Max Planck Inst Aeron, D-37189 Katlenburg Lindau, Germany

来源：

MINOR BODIES IN THE OUTER SOLAR SYSTEM | 2000年

关键词：

D O I：

10.1007/10651968_3

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report on observations of the Kuiper-Belt Objects, 1993 SC and 1996 TL66 using the European Space Agency's Infrared Space Observatory. The measurements indicate a first detection of 1993 SC at 90 microns and yield a measurement of the radius of 164 (+/-35) km and a geometric albedo of 0.022 (+/-0.013). For 1996 TL66, an effective radius of 316(+/-49) km and a geometric albedo of 0.030(+/-0.015) have been derived although, in this case, it cannot be ruled out that the signal is not actually from the KBO. This paper represents a brief report of an article published more fully elsewhere [13].

引用

页码：25 / 31

页数：7

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