Remote 3D geological analysis of possible sedimentary layer geometries in upper Aeolis Mons, Gale Crater, Mars

Divya M Persaud; Robert Barnes; Yu Tao; Jan-Peter Muller

doi:https://doi.org/10.5194/epsc2020-450

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EPSC Abstracts

Vol.14, EPSC2020-450, 2020, updated on 08 Oct 2020

https://doi.org/10.5194/epsc2020-450

Europlanet Science Congress 2020

© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Remote 3D geological analysis of possible sedimentary layer geometries in upper Aeolis Mons, Gale Crater, Mars

Divya M Persaud¹, Robert Barnes², Yu Tao¹, and Jan-Peter Muller¹

Divya M Persaud et al.

¹Imaging Group, Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Surrey, RH5 6NT
²Department of Earth Science and Engineering, Imperial College London, London, UK

How to cite: Persaud, D. M., Barnes, R., Tao, Y., and Muller, J.-P.: Remote 3D geological analysis of possible sedimentary layer geometries in upper Aeolis Mons, Gale Crater, Mars, Europlanet Science Congress 2020, online, 21 September–9 Oct 2020, EPSC2020-450, https://doi.org/10.5194/epsc2020-450, 2020

This abstract has been withdrawn on 03 Sep 2020.