Orbital stability of massive protoplanets in the terrestrial planet region of the solar system
- 1 December 1978
- journal article
- Published by Springer Nature in Earth, Moon, and Planets
- Vol. 19 (4) , 421-424
- https://doi.org/10.1007/bf00901972
Abstract
No abstract availableKeywords
This publication has 5 references indexed in Scilit:
- The Effects of Tidal Forces on the Stability and Dispersal Rates of a ProtoplanetMonthly Notices of the Royal Astronomical Society, 1975
- Stability criteria for triple starsCelestial Mechanics and Dynamical Astronomy, 1972
- Segregation of materials in cosmogonyProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1965
- A capture theory of the origin of the Solar SystemProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1964
- The origin of the solar systemProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1960