Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-23T11:52:18.067Z Has data issue: false hasContentIssue false

Light from Shattered Worlds: Debris from Giant Impacts

Published online by Cambridge University Press:  06 January 2014

Alan P. Jackson*
Affiliation:
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
Mark C. Wyatt
Affiliation:
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
William R. F. Dent
Affiliation:
Joint ALMA Observatory, Alonso de Córdova 3107, Vitacura - Santiago, Chile
Aki Roberge
Affiliation:
Goddard Space Flight Centre, 8800 Greenbelt Road, Greenbelt, Maryland, 20771, USA
*
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Large impacts in the outer parts of a planetary system will produce debris discs that display a strong, distinctive, asymmetry, which will last for 105 year timescales. Debris resulting from a large impact may be able to explain the asymmetries in some known debris discs that have hitherto been difficult to understand.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013 

References

Agnor, C. & Asphaug, E., 2004, ApJL, 613, L157Google Scholar
Brown, M. E., Barkume, K. M., Ragozzine, D., & Schaller, E. L., 2007, Nature, 446, 294CrossRefGoogle Scholar
Canup, R. M., 2011, AJ, 141, 35CrossRefGoogle Scholar
Chambers, J. E., 1999, MNRAS, 304, 793CrossRefGoogle Scholar
Jackson, A. P. & Wyatt, M. C., 2012, MNRAS, 425, 657CrossRefGoogle Scholar
Kokubo, E. & Ida, S., 1998, Icarus, 131, 171CrossRefGoogle Scholar
Stewart, S. T. & Leinhardt, Z. M., 2012, ApJ, 751, 32CrossRefGoogle Scholar