Latitude variations of the density of the interior of Mars

Details Latitude variations of the density of the interior of Mars Latitude variations of the density of the interior of Mars

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982avest..16...34d&link_type=abstract

(Astronomicheskii Vestnik, vol. 16, Jan.-Mar. 1982, p. 34-36.) Solar System Research, vol. 16, no. 1, July 1982, p. 28, 29. Tra

Astronomy and Astrophysics

Astronomy

Density Distribution, Latitude, Mars (Planet), Planetary Structure, Angular Distribution, Gravitational Fields, Mars Surface, Planetary Cores, Planetary Gravitation, Planetary Mantles, Topography

Scientific paper

On the basis of the gravitational field, topographic and maximal fluctuations of the density on the planetary surface data a latitudinal variation of the Martian density was established. It is shown that the maximal variations of the density can be observed on the limits "crust - mantle", "mantle - core". A transition layer in the silicate mantle at a depth of about 700 km is revealed.

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