Earth, Moon, and Planets

, Volume 56, Issue 1, pp 47–52

Mass distribution in the asteroid belt

  • Jozef Klačka
Article

DOI: 10.1007/BF00054599

Cite this article as:
Klačka, J. Earth Moon Planet (1992) 56: 47. doi:10.1007/BF00054599

Abstract

The dependence of the cumulative number of numbered asteroids (up to 3720) on their absolute magnitude is investigated. The differential mass index k is derived from these relations for fainter asteroids. A steeper slope (2.2 < k < 2.4) is found in the four most populous asteroid familes (Flora, Koronis, Eos and Themis) and a flatter slope (1.3 < k < 1.6) for non-family asteroids. This indicates that there are two different asteroid populations in the asteorid belt. Total masses of the asteroid families may be greater than it is commonly accepted.

Copyright information

© Kluwer Academic Publishers 1992

Authors and Affiliations

  • Jozef Klačka
    • 1
  1. 1.Department of Astronomy and AstrophysicsMFF UKMlynská dolinaCzech and Slovak Federal Republic

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