Detecting the Dusty Debris of Terrestrial Planet Formation
- 5 February 2004
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 602 (2) , L133-L136
- https://doi.org/10.1086/382693
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.Comment: 11 pages of text, 3 figures, accepted for ApJ Letters, additional info at http://cfa-www.harvard.edu/~kenyon/pf/terra/tdKeywords
All Related Versions
This publication has 57 references indexed in Scilit:
- Damping of Terrestrial‐Planet Eccentricities by Density‐Wave Interactions with a Remnant Gas DiskThe Astrophysical Journal, 2002
- Making More Terrestrial PlanetsIcarus, 2001
- ISOCAM observations of the $\mathsf{\rho}$ Ophiuchi cloud: Luminosity and mass functions of the pre-main sequence embedded clusterAstronomy & Astrophysics, 2001
- Accretion Disks around Young Objects. III. Grain GrowthThe Astrophysical Journal, 2001
- Spectral Energy Distributions of Passive T Tauri Disks: InclinationThe Astrophysical Journal, 1999
- Vortices in Circumstellar DisksThe Astrophysical Journal, 1995
- Accretion disks around T Tauri starsThe Astrophysical Journal, 1988
- Spectral evolution of young stellar objectsThe Astrophysical Journal, 1987
- Collisional history of asteroids: Evidence from Vesta and the Hirayama familiesIcarus, 1985
- The Gas Drag Effect on the Elliptic Motion of a Solid Body in the Primordial Solar NebulaProgress of Theoretical Physics, 1976