Small and planetary bodies of the solar system - Critical mass of the icy bodies

Details Small and planetary bodies of the solar system - Critical mass of the icy bodies Small and planetary bodies of the solar system - Critical mass of the icy bodies

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993avest..27...71s&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 27, no. 1, p. 71-82.

Astronomy and Astrophysics

Astronomy

3

Asteroids, Natural Satellites, Planetary Composition, Planetary Mass, Planets, Icy Satellites, Planetary Evolution, Planetary Gravitation, Plastic Deformation, Yield Strength

Scientific paper

Available data on the observed transition between planetary and small solar system bodies are reviewed. It is shown that the limits of this transition are determined by the fundamental strength of the matter of small bodies. The quantitative theory of this transition is examined, and results agree well with experimental and observational data. Strict limits for yield stress values of materials of icy small bodies with low temperatures were obtained. Values of the critical mass of these small bodies were also obtained.

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