A co-accretional model of satellite formation
- 1 April 1975
- Vol. 24 (4), 516-524
- https://doi.org/10.1016/0019-1035(75)90071-8
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
- Dynamics of lunar origin and orbital evolutionReviews of Geophysics, 1975
- Where are the Satellites of the Inner Planets?Nature Physical Science, 1973
- Outcomes of Tidal EvolutionThe Astrophysical Journal, 1973
- On the model of the accumulation of the moon compatible with the data on the composition and the age of lunar rocksEarth, Moon, and Planets, 1973
- On the rotation of the Earth produced by gravitational accretion of particlesIcarus, 1968
- Q in the solar systemIcarus, 1966
- Rediscussion of Maxwell's ADAMS Prize Essay on the stability of Saturn S ringsThe Astronomical Journal, 1964
- On the Eccentricity of Satellite Orbits in the Solar SystemMonthly Notices of the Royal Astronomical Society, 1963
- On the secular accelerations of PHOBOS and Jupiter VThe Astronomical Journal, 1954
- Accretion of matter by a satelliteThe Astronomical Journal, 1954