Oort cloud and Scattered Disc formation during a late dynamical instability in the Solar System
- 1 July 2013
- journal article
- Published by Elsevier BV in Icarus
- Vol. 225 (1), 40-49
- https://doi.org/10.1016/j.icarus.2013.03.012
Abstract
No abstract availableKeywords
This publication has 55 references indexed in Scilit:
- Considerations on the magnitude distributions of the Kuiper belt and of the Jupiter TrojansIcarus, 2009
- ON A SCATTERED-DISK ORIGIN FOR THE 2003 EL61COLLISIONAL FAMILY—AN EXAMPLE OF THE IMPORTANCE OF COLLISIONS ON THE DYNAMICS OF SMALL BODIESThe Astronomical Journal, 2008
- Injection of Oort Cloud comets: the fundamental role of stellar perturbationsCelestial Mechanics and Dynamical Astronomy, 2008
- The population of faint Jupiter family comets near the EarthIcarus, 2006
- On The Origin of The High-Perihelion Scattered Disk: The Role of The Kozai Mechanism And Mean Motion ResonancesCelestial Mechanics and Dynamical Astronomy, 2005
- Comet nucleus size distributions from HST and Keck telescopesIcarus, 2004
- CCD observations of distant comets from Palomar and Steward ObservatoriesIcarus, 2003
- The Buildup of a Tightly Bound Comet Cloud around an Early Sun Immersed in a Dense Galactic Environment: Numerical ExperimentsIcarus, 2000
- An idealized short-period comet model: Surface insolation, H2O flux, dust flux, and mantle evolutionIcarus, 1984
- Comet showers and the steady-state infall of comets from the Oort cloudThe Astronomical Journal, 1981