Journal
ASTROPHYSICAL JOURNAL
Volume 602, Issue 2, Pages L133-L136Publisher
IOP PUBLISHING LTD
DOI: 10.1086/382693
Keywords
circumstellar matter; planetary systems; solar system : formation; stars : formation
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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.
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