Discovery of a large dust disk around the nearby star AU Microscopii

被引:190
作者
Kalas, P
Liu, MC
Matthews, BC
机构
[1] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[2] Univ Calif Berkeley, Radio Astron Lab, Berkeley, CA 94720 USA
[3] Univ Calif Santa Cruz, Natl Sci Fdn, Ctr Adapt Opt, Santa Cruz, CA 95064 USA
[4] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
基金
美国国家科学基金会;
关键词
D O I
10.1126/science.1093420
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
We present the discovery of a circumstellar dust disk surrounding AU Microscopii (AU Mic, GJ 803, HD 197481). This young M star at 10 parsec has the same age and origin as beta Pictoris, another nearby star surrounded by a dust disk. The AU Mic disk is detected between 50 astronomical units ( AU) and 210 AU radius, a region where dust lifetimes exceed the present stellar age. Thus, AU Mic is the nearest star where we directly observe the solid material required for planet formation. Because 85% of stars are M-type, the AU Mic disk provides new clues on how the majority of planetary systems might form and evolve.
引用
收藏
页码:1990 / 1992
页数:3
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