Persistent or repeated surface habitability on Mars during the Late Hesperian - Amazonian

This is a Preprint and has not been peer reviewed. The published version of this Preprint is available: https://doi.org/10.1002/2017GL072660.

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Authors

Edwin Kite , Jonathan Sneed, David Mayer , Sharon Wilson

Abstract

Large alluvial fan deposits on Mars record relatively recent habitable surface conditions (≲3.5 Ga, Late Hesperian – Amazonian). We find net sedimentation rate <(4-8) μm/yr in the alluvial-fan deposits, using the frequency of craters that are interbedded with alluvial fan deposits as a fluvial-process chronometer. Considering only the observed interbedded craters sets a lower bound of >20 Myr on the total time interval spanned by alluvial-fan aggradation, >10^3-fold longer than previous lower limits. A more realistic approach that corrects for craters fully entombed in the fan deposits raises the lower bound to >(100-300) Myr. Several factors not included in our calculations would further increase the lower bound. The lower bound rules out fan-formation by a brief climate anomaly. Therefore, during the Late Hesperian – Amazonian on Mars, persistent or repeated processes permitted habitable surface conditions.

DOI

https://doi.org/10.31223/osf.io/uw3ex

Subjects

Astrophysics and Astronomy, Earth Sciences, Geology, Physical Sciences and Mathematics, The Sun and the Solar System

Keywords

Mars, alluvial fans, habitability, impact craters

Dates

Published: 2019-01-01 10:40

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License

GNU Lesser General Public License (LGPL) 2.1

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