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Hydrocarbons on Mars

Published online by Cambridge University Press:  21 September 2023

Jaroslav Klokočník*
Affiliation:
Astronomical Institute, Czech Academy of Sciences, Fričova 298, CZ 251 65 Ondřejov, Czech Republic
Jan Kostelecký
Affiliation:
Research Institute of Geodesy, Topography and Cartography, CZ 250 66 Zdiby 98, Czech Republic Faculty of Mining and Geology, VSB-TU Ostrava, CZ 708 33 Ostrava, Czech Republic
Aleš Bezděk
Affiliation:
Astronomical Institute, Czech Academy of Sciences, Fričova 298, CZ 251 65 Ondřejov, Czech Republic
Václav Cílek
Affiliation:
Geological Institute, Czech Academy of Sciences, CZ 165 00 Praha 6, Rozvojová 269, Prague, Czech Republic
*
Corresponding author: Jaroslav Klokočník; Email: jklokocn@asu.cas.cz

Abstract

Providing evidence for possible oil-type occurrences on Mars means providing an indication for the past life on Mars. We do this via analysis of the combed (aligned) gravity strike angles, one of the gravity (gravitational) aspects (descriptors) derived from one of the recent gravitational field models of Mars, currently having the highest accessible precision and resolution. After intensive testing for features on the Earth and the Moon, the gravity aspects are applied for Mars. We detect candidates for the groundwater/hydrocarbon/mud/petroleum-bearing sites in the largest areas with as many as possible combed gravity strike angles, uniformly ordered into ‘plates’. They appear mainly but not only in the hypothetical northern Martian palaeo-ocean (the northern lowlands). It turns out that the combed strike angles are sensitive not only to uniformly ordered sediments of the basins, but also to supposed lahars.

Type
Research Article
Copyright
Copyright © The Author(s), 2023. Published by Cambridge University Press

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