Detecting the dusty debris of terrestrial planet formation

被引：103

作者：

Kenyon, SJ

Bromley, BC

机构：

[1] Smithsonian Astrophys Observ, Cambridge, MA 02138 USA

[2] Univ Utah, Dept Phys, Salt Lake City, UT 84112 USA

来源：

ASTROPHYSICAL JOURNAL | 2004年 / 602卷 / 02期

基金：

美国国家航空航天局;

关键词：

circumstellar matter; planetary systems; solar system : formation; stars : formation;

D O I：

10.1086/382693

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We use a multiannulus accretion code to investigate debris disks in the terrestrial zone at 0.7 - 1.3 AU around a 1 M. star. Terrestrial planet formation produces a bright dusty ring of debris with a lifetime of greater than or similar to 10(6) yr. The early phases of terrestrial planet formation are observable with current facilities; the late stages require more advanced instruments with adaptive optics.

引用

页码：L133 / L136

页数：4

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