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Cosmogony of the asteroidal belt (1974)

Burkenroad, M. D. ; Alfven, H. ; Ip, W.-H.

In: Other Sources

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Publication Date: 2011-08-16

Description: In the plot of asteroids considered the mass density is substituted for the number density. This approach provides a better definition of the limits of the main belt, and demonstrates more clearly that the asteroids, like the Saturnian rings, have condensed from partially corotating plasma. A diagram shows that the whole main belt is located below 2/3 of Jupiter's orbit. This means that the main belt asteroids may have been derived from condensation which took place inside Jupiter's orbit.

Keywords: SPACE SCIENCES

Type: Nature; 250; Aug. 23

Format: text

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