Other
Scientific paper
Oct 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.514..129f&link_type=abstract
In: Earth-like planets and moons. Proceedings of the 36th ESLAB Symposium, 3 - 8 June 2002, ESTEC, Noordwijk, The Netherlands. E
Other
Planets: Surface Structures: Formation
Scientific paper
Elementary empirical analysis of the distribution of the centers of different formations of the Earth-like planets and moons (CPF) leads us to a conclusion about ordered character of their positions. The definite inclined belts of the concentration of the CF, grid phenomenon in their latitudinal and longitudinal distribution, antipodal CF are observed on the surface of the Mercury, Venus, Moon, Mars, Io and other planets and satellites. Here we present some first results of the mathematical-statistical analysis by axography method of the ordered center positions of different formations (montes, dorsa, pateras, albedo features and others) for above-mentioned bodies of the Solar system.
Barkin Yu V.
Ferrandez M. G.
Ferrándiz José Manuel
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