2009/03/30 by Simone Marchi, S. Marchi, S. Mottola +7 · 193 citations
Physics and Astronomy · #Astro and Planetary Science #Chronology #Flux (metallurgy) #Mercury (programming language) #Planetary Science and Exploration #Solar System #Space Science and Extraterrestrial Life #Surface exposure dating #astro-ph.EP
paper · pdf · doi:10.1088/0004-6256/137/6/4936
published in The Astronomical Journal 137(6), 4936-4948 (Institute of Physics) · 27 pages, 13 figures, 1 table; accepted by AJ
arxiv created 2009/03/30 · openalex publication_date 2009/05/04 · arxiv updated 2015/05/13 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/06
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 nonconstant 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.