The Mass Influx of the Inner Solar System Estimated by a Lunar-Like Chronology Model

Details The Mass Influx of the Inner Solar System Estimated by a Lunar-Like Chronology Model The Mass Influx of the Inner Solar System Estimated by a Lunar-Like Chronology Model

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1947h&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1947

Physics

Scientific paper

Aim of this work is to test one of the most simplest and straightforward
hypothesis: What if the early highly populated asteroid belt (AB) is
the main source for the masses impacted in the inner solar system, not
only now, but also before 3.0 Ga?

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