Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
Scientific paper
2009-03-30
Astronomy and Astrophysics
Astrophysics
Earth and Planetary Astrophysics
27 pages, 13 figures, 1 table; accepted by AJ
Scientific paper
In this paper we present a new method for dating the surface of the Moon, obtained by modeling the incoming flux of impactors and converting it into a size distribution of resulting craters. We compare the results from this model with the standard chronology for the Moon showing their similarities and discrepancies. In particular, we find indications of a non-constant impactor flux in the last 500 Myr and also discuss the implications of our findings for the Late Heavy Bombardment hypothesis. We also show the potential of our model for accurate dating of other inner Solar System bodies, by applying it to Mercury.
Cremonese Gabriele
Marchi Simone
Martellato Elena
Massironi Matteo
Mottola Stefano
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