Sep 1947
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1947natur.160..330a&link_type=abstract
Nature, Volume 160, Issue 4062, pp. 330 (1947).
Physics
33
Scientific paper
BY assuming that diamagnetic bodies are pushed out of a magnetic field, it may be shown that a diamagnetic particle attracted to a magnet by gravitational forces will take up a position in space in the equatorial plane of the straight magnet at a certain distance from the latter. The `satellite' can vibrate elastically about the point of equilibrium, describing a certain curve. The period of vibration in the radial and meridional directions is close to the period of the Kepler rotation of a magnetically indifferent satellite about a body of the same mass. Several identical particles arrange themselves around the magnet. Such a combination of bodies is in the nature of a static planetary system as distinct from the Kepler dynamic planetary system.
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