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Preliminary Results on Formation of Jetstreams by Gravitational Scattering

Published online by Cambridge University Press:  12 April 2016

R.T. Giuli*
Affiliation:
NASA Manned Spacecraft Center

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Alfvén and Arrhenius (1970) have considered the development and stability of jetstreams by collisional interactions among grains; and they propose that in a jetstream environment, grains may collect and adhere to form self-gravitating embryos. Gravitational attraction of smaller particles by these embryos may then lead to a net accretion because high relative approach speeds, which could erode or break up embryos, have been minimized during the formation of the jetstream.

Type
Part II-Origin of Asteroids Interrelations with Comets, Meteorites, and Meteors
Copyright
Copyright © NASA 1971

References

References

Alfvén, H., and Anhenius, G. 1970, Structure and Evolutionary History of the Solar System, I. Astrophys. Space Sci. 8, 338421.Google Scholar
Giuli, R.T. 1968a, On the Rotation of the Earth Produced by Gravitational Accretion of Particles. Icarus 8, 301323.Google Scholar
Giuli, R.T. 1968b, Gravitational Accretion of Small Masses Attracted From Large Distances as a Mechanism for Planetary Rotation. Icarus 9, 186190.CrossRefGoogle Scholar

Discussion References

Fish, F.F. Jr. 1967, Angular Momenta of the Planets. Icarus 7, 251256.Google Scholar
Giuli, R.T. 1968a, On the Rotation of the Earth Produced by Gravitational Accretion of Particles. Icarus 8, 301323.CrossRefGoogle Scholar
Giuli, R.T. 1968b, Gravitational Accretion of Small Masses Attracted From Large Distances as a Mechanism for Planetary Rotation. Icarus 9, 186190.CrossRefGoogle Scholar
Hartmann, W.K., and Larson, S.M. 1967, Angular Momenta of Planetary Bodies. Icarus 7, 257260.Google Scholar
MacDonald, G.J.F. 1963, The Internal Constitutions of the Inner Planets and the Moon. Space Sci. Rev. 2, 473557.Google Scholar