The cumulative size-frequency distributions of impact craters on planetary bodies in the Solar system appear to approximate a universal inverse square power law for small crater radii. In this paper, we show how this distribution can be understood easily in terms of geometrical statistics, using a de-Sitter geometry of the configuration space of circles on the Euclidean plane and on the unit sphere. The effect of crater overlap is also considered. © 2012 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.
CITATION STYLE
Gibbons, G. W., & Werner, M. C. (2013). On de-Sitter geometry in crater statistics. Monthly Notices of the Royal Astronomical Society, 429(2), 1045–1050. https://doi.org/10.1093/mnras/sts401
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