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Orbital stability of massive protoplanets in the terrestrial planet region of the solar system

✍ Scribed by J. R. Donnison; I. P. Williams


Publisher
Springer Netherlands
Year
1978
Tongue
English
Weight
213 KB
Volume
19
Category
Article
ISSN
1573-0794

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If a planetary-mass body were present in the asteroid belt, the orbits of the terrestrial planets and those of the giant planets would be more closely coupled. A greater exchange of angular momentum could affect the stability of the terrestrial planets. Moreover, the planet in the asteroid belt coul