Instability of Small-size Planetary Cores and the Development of the Moon

Details Instability of Small-size Planetary Cores and the Development of the Moon Instability of Small-size Planetary Cores and the Development of the Moon

Apr 1964

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1964natur.202..378h&link_type=abstract

Nature, Volume 202, Issue 4930, pp. 378-380 (1964).

Physics

Scientific paper

IT can be proved1 (if the gravity coefficient G varies with
time2) that once, many millions of years ago, the Moon had a
metallic central core, the radius of which decreased as the time
elapsed. This hypothesis is based on Prof. L. Egyed's theory of the
expansion of the Earth3.

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