A Sawtooth-like Timeline for the First Billion Year of Lunar Bombardment

We revisit the early evolution of the Moon's bombardment. Our work combines modeling (based on plausible projectile sources and their dynamical decay rates) with constraints from the lunar crater record, radiometric ages of the youngest lunar basins, and the abundance of highly siderophile elem...

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Main Authors: Morbidelli, Alessandro, Marchi, Simone, Bottke, William F., Kring, David A.
Format: Text
Language:unknown
Published: arXiv 2012
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.1208.4624
https://arxiv.org/abs/1208.4624
id ftdatacite:10.48550/arxiv.1208.4624
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spelling ftdatacite:10.48550/arxiv.1208.4624 2023-05-15T18:23:16+02:00 A Sawtooth-like Timeline for the First Billion Year of Lunar Bombardment Morbidelli, Alessandro Marchi, Simone Bottke, William F. Kring, David A. 2012 https://dx.doi.org/10.48550/arxiv.1208.4624 https://arxiv.org/abs/1208.4624 unknown arXiv https://dx.doi.org/10.1016/j.epsl.2012.07.037 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Earth and Planetary Astrophysics astro-ph.EP FOS Physical sciences article-journal Article ScholarlyArticle Text 2012 ftdatacite https://doi.org/10.48550/arxiv.1208.4624 https://doi.org/10.1016/j.epsl.2012.07.037 2022-04-01T13:36:27Z We revisit the early evolution of the Moon's bombardment. Our work combines modeling (based on plausible projectile sources and their dynamical decay rates) with constraints from the lunar crater record, radiometric ages of the youngest lunar basins, and the abundance of highly siderophile elements in the lunar crust and mantle. We deduce that the evolution of the impact flux did not decline exponentially over the first billion years of lunar history, but also there was no prominent and "narrow" impact spike some 3.9 Gy ago, unlike that typically envisioned in the lunar cataclysm scenario. Instead, we show the timeline of the lunar bombardment has a sawtooth-like profile, with an uptick in the impact flux near 4.1 Gy ago. The impact flux at the beginning of this weaker cataclysm was 5-10 times higher than the immediately preceding period. The Nectaris basin should have been one of the first basins formed at the sawtooth. We predict the bombardment rate since about 4.1Gy ago declined slowly and adhered relatively close to classic crater chronology models (Neukum and Ivanov (1994)). Overall we expect that the sawtooth event accounted for about 1/4 of the total bombardment suffered by the Moon since its formation. Consequently, considering that about 12-14 basins formed during the sawtooth event, we expect that the net number of basins formed on the Moon was about 45-50. From our expected bombardment timeline, we derived a new and improved lunar chronology suitable for use on Pre-Nectarian surface units. According to this chronology, a significant portion of the oldest lunar cratered terrains has an age of 4.38-4.42 Gyr. Moreover, the largest lunar basin, South Pole Aitken, is older than 4.3Gy, and therefore was not produced during the lunar cataclysm. : In press in EPSL Text South pole DataCite Metadata Store (German National Library of Science and Technology) Aitken ENVELOPE(-44.516,-44.516,-60.733,-60.733) South Pole
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Earth and Planetary Astrophysics astro-ph.EP
FOS Physical sciences
spellingShingle Earth and Planetary Astrophysics astro-ph.EP
FOS Physical sciences
Morbidelli, Alessandro
Marchi, Simone
Bottke, William F.
Kring, David A.
A Sawtooth-like Timeline for the First Billion Year of Lunar Bombardment
topic_facet Earth and Planetary Astrophysics astro-ph.EP
FOS Physical sciences
description We revisit the early evolution of the Moon's bombardment. Our work combines modeling (based on plausible projectile sources and their dynamical decay rates) with constraints from the lunar crater record, radiometric ages of the youngest lunar basins, and the abundance of highly siderophile elements in the lunar crust and mantle. We deduce that the evolution of the impact flux did not decline exponentially over the first billion years of lunar history, but also there was no prominent and "narrow" impact spike some 3.9 Gy ago, unlike that typically envisioned in the lunar cataclysm scenario. Instead, we show the timeline of the lunar bombardment has a sawtooth-like profile, with an uptick in the impact flux near 4.1 Gy ago. The impact flux at the beginning of this weaker cataclysm was 5-10 times higher than the immediately preceding period. The Nectaris basin should have been one of the first basins formed at the sawtooth. We predict the bombardment rate since about 4.1Gy ago declined slowly and adhered relatively close to classic crater chronology models (Neukum and Ivanov (1994)). Overall we expect that the sawtooth event accounted for about 1/4 of the total bombardment suffered by the Moon since its formation. Consequently, considering that about 12-14 basins formed during the sawtooth event, we expect that the net number of basins formed on the Moon was about 45-50. From our expected bombardment timeline, we derived a new and improved lunar chronology suitable for use on Pre-Nectarian surface units. According to this chronology, a significant portion of the oldest lunar cratered terrains has an age of 4.38-4.42 Gyr. Moreover, the largest lunar basin, South Pole Aitken, is older than 4.3Gy, and therefore was not produced during the lunar cataclysm. : In press in EPSL
format Text
author Morbidelli, Alessandro
Marchi, Simone
Bottke, William F.
Kring, David A.
author_facet Morbidelli, Alessandro
Marchi, Simone
Bottke, William F.
Kring, David A.
author_sort Morbidelli, Alessandro
title A Sawtooth-like Timeline for the First Billion Year of Lunar Bombardment
title_short A Sawtooth-like Timeline for the First Billion Year of Lunar Bombardment
title_full A Sawtooth-like Timeline for the First Billion Year of Lunar Bombardment
title_fullStr A Sawtooth-like Timeline for the First Billion Year of Lunar Bombardment
title_full_unstemmed A Sawtooth-like Timeline for the First Billion Year of Lunar Bombardment
title_sort sawtooth-like timeline for the first billion year of lunar bombardment
publisher arXiv
publishDate 2012
url https://dx.doi.org/10.48550/arxiv.1208.4624
https://arxiv.org/abs/1208.4624
long_lat ENVELOPE(-44.516,-44.516,-60.733,-60.733)
geographic Aitken
South Pole
geographic_facet Aitken
South Pole
genre South pole
genre_facet South pole
op_relation https://dx.doi.org/10.1016/j.epsl.2012.07.037
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.1208.4624
https://doi.org/10.1016/j.epsl.2012.07.037
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