Collisional evolution of Trans-Neptunian populations: Effects of fragmentation physics and estimates of the abundances of gravitational aggregates
- 28 February 2009
- journal article
- Published by Elsevier BV in Planetary and Space Science
- Vol. 57 (2), 201-215
- https://doi.org/10.1016/j.pss.2008.09.007
Abstract
No abstract availableKeywords
This publication has 36 references indexed in Scilit:
- Coupling dynamical and collisional evolution of small bodies: II. Forming the Kuiper belt, the Scattered Disk and the Oort CloudIcarus, 2007
- Cratering of icy targets by different impactors: Laboratory experiments and implications for cratering in the Solar SystemIcarus, 2005
- The Size Distribution of Trans-Neptunian BodiesThe Astronomical Journal, 2004
- Coupling dynamical and collisional evolution of small bodies:: an application to the early ejection of planetesimals from the Jupiter–Saturn regionIcarus, 2003
- Updated collisional probabilities of minor body populationsAstronomy & Astrophysics, 2001
- How Many Rubble Piles Are in the Asteroid Belt?Icarus, 2001
- Catastrophic Disruptions RevisitedIcarus, 1999
- New Views of AsteroidsScience, 1997
- Collisional Evolution of Edgeworth–Kuiper Belt ObjectsIcarus, 1997
- Wavy size distributions for collisional systems with a small-size cutoffPlanetary and Space Science, 1994