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Preliminary Results on Formation of Jetstreams by Gravitational Scattering
Published online by Cambridge University Press: 12 April 2016
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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
- Information
- International Astronomical Union Colloquium , Volume 12: Physical Studies of Minor Planets , 1971 , pp. 247 - 250
- Copyright
- Copyright © NASA 1971
References
References
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Discussion References
Giuli, R.T.
1968a, On the Rotation of the Earth Produced by Gravitational Accretion of Particles. Icarus
8, 301–323.CrossRefGoogle Scholar
Giuli, R.T.
1968b, Gravitational Accretion of Small Masses Attracted From Large Distances as a Mechanism for Planetary Rotation. Icarus
9, 186–190.CrossRefGoogle Scholar
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1967, Angular Momenta of Planetary Bodies. Icarus
7, 257–260.Google Scholar
MacDonald, G.J.F.
1963, The Internal Constitutions of the Inner Planets and the Moon. Space Sci. Rev.
2, 473–557.Google Scholar
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