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Large impact cratering during lunar magma ocean solidification.

التفاصيل البيبلوغرافية
العنوان: Large impact cratering during lunar magma ocean solidification.
المؤلفون: Miljković K; Curtin University, School of Earth and Planetary Science, Space Science and Technology Centre, Perth, WA, Australia. katarina.miljkovic@curtin.edu.au., Wieczorek MA; Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Nice, France., Laneuville M; Earth-Life Science Institute, Tokyo, Japan., Nemchin A; Curtin University, School of Earth and Planetary Science, Space Science and Technology Centre, Perth, WA, Australia., Bland PA; Curtin University, School of Earth and Planetary Science, Space Science and Technology Centre, Perth, WA, Australia., Zuber MT; Massachusetts Institute of Technology, Cambridge, MA, USA.
المصدر: Nature communications [Nat Commun] 2021 Sep 14; Vol. 12 (1), pp. 5433. Date of Electronic Publication: 2021 Sep 14.
نوع المنشور: Journal Article
اللغة: English
بيانات الدورية: Publisher: Nature Pub. Group Country of Publication: England NLM ID: 101528555 Publication Model: Electronic Cited Medium: Internet ISSN: 2041-1723 (Electronic) Linking ISSN: 20411723 NLM ISO Abbreviation: Nat Commun Subsets: PubMed not MEDLINE; MEDLINE
أسماء مطبوعة: Original Publication: [London] : Nature Pub. Group
مستخلص: The lunar cratering record is used to constrain the bombardment history of both the Earth and the Moon. However, it is suggested from different perspectives, including impact crater dating, asteroid dynamics, lunar samples, impact basin-forming simulations, and lunar evolution modelling, that the Moon could be missing evidence of its earliest cratering record. Here we report that impact basins formed during the lunar magma ocean solidification should have produced different crater morphologies in comparison to later epochs. A low viscosity layer, mimicking a melt layer, between the crust and mantle could cause the entire impact basin size range to be susceptible to immediate and extreme crustal relaxation forming almost unidentifiable topographic and crustal thickness signatures. Lunar basins formed while the lunar magma ocean was still solidifying may escape detection, which is agreeing with studies that suggest a higher impact flux than previously thought in the earliest epoch of Earth-Moon evolution.
(© 2021. The Author(s).)
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تواريخ الأحداث: Date Created: 20210915 Latest Revision: 20230206
رمز التحديث: 20240628
مُعرف محوري في PubMed: PMC8440705
DOI: 10.1038/s41467-021-25818-7
PMID: 34521860
قاعدة البيانات: MEDLINE
الوصف
تدمد:2041-1723
DOI:10.1038/s41467-021-25818-7