Survival of a proto-atmosphere through the stage of giant impacts: the mechanical aspects
- 11 June 2003
- journal article
- Published by Elsevier
- Vol. 164 (1) , 149-162
- https://doi.org/10.1016/s0019-1035(03)00101-5
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- Making the Terrestrial Planets: N-Body Integrations of Planetary Embryos in Three DimensionsIcarus, 1998
- Erosion of terrestrial planet atmosphere by surface motion after a large impactPublished by Elsevier ,1998
- The Origin of the Moon and the Single Impact Hypothesis V☆Icarus, 1997
- Evolution of Earth's Noble Gases: Consequences of Assuming Hydrodynamic Loss Driven by Giant Impact☆Icarus, 1997
- The formation of terrains antipodal to major impactsIcarus, 1991
- Evolution of a steam atmosphere during earth's accretionIcarus, 1988
- Shock viscosity and the prediction of shock wave rise timesJournal of Applied Physics, 1985
- The evolution of an impact-generated atmosphereIcarus, 1982
- Earth's melting due to the blanketing effect of the primordial dense atmosphereEarth and Planetary Science Letters, 1979
- Equation of State of Metals from Shock Wave MeasurementsPhysical Review B, 1955