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arXiv · astro-ph/0401343

Detecting the Dusty Debris of Terrestrial Planet Formation

Scott J Kenyon·Benjamin C Bromley
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Abstract

We use a multiannulus accretion code to investigate debris disks in the terrestrial zone, at 0.7-1.3 AU around a 1 solar mass star. Terrestrial planet formation produces a bright dusty ring of debris with a lifetime of at least 1 Myr. 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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Scott J Kenyon, Benjamin C Bromley. 2004-01-16. Detecting the Dusty Debris of Terrestrial Planet Formation. https://doi.org/10.1086/382693

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