The Earth-Moon system during the Late Heavy Bombardment period

• Main Authors: Jorgensen, Uffe Graae, Appel, Peter W. U., Hatsukawa, Yuichi, Frei, Robert, Oshima, Masumi, Toh, Yosuke, Kimura, Atsushi
• Format: Text
• Language: unknown
• Published: arXiv 2009
• Subjects: Earth and Planetary Astrophysics astro-ph.EP; FOS Physical sciences; Greenland
• Online Access: https://dx.doi.org/10.48550/arxiv.0907.4104; https://arxiv.org/abs/0907.4104

The Late Heavy Bombardment (LHB) period is the narrow time interval between 3.8 and 3.9 Gyr ago, where the bulk of the craters we see on the Moon formed. Even more craters formed on the Earth. During a field expedition to the 3.8 Gyr old Isua greenstone belt in Greenland, we sampled three types of metasedimentary rocks, that contain direct traces of the LHB impactors by a seven times enrichment (150 ppt) in iridium compared to present day ocean crust (20 ppt). We show that this enrichment is in agreement with the lunar cratering rate, providing the impactors were comets, but not if they were asteroids. Our study is a first direct indication of the nature of the LHB impactors, and the first to find an agreement between the LHB lunar cratering rate and the Earth's early geochemical record (and the corresponding lunar record). The LHB comets that delivered the iridium we see at Isua will at the same time have delivered the equivalent of a km deep ocean, and we explain why one should expect a cometary ocean to become roughly the size of the Earth's present-day ocean, not only in terms of depth but also in terms of the surface area it covers. : Accepted for publication in Icarus