Detecting the Dusty Debris of Terrestrial Planet Formation

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Published 2004 February 5 © 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Scott J. Kenyon and Benjamin C. Bromley 2004 ApJ 602 L133 DOI 10.1086/382693

1538-4357/602/2/L133

Abstract

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 ≳106 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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10.1086/382693