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A Cerberus Fossae Seismic Network

Authors :
Stahler, S. C.
Panning, Mark P.
Antonangeli, D.
Banerdt, W. B.
Banks, M.
Ceylan, S.
Charalambous, C.
Clinton, John
Daubar, I.
Fernando, B.
Giardini, Domenico
Grott, M.
Horleston, A.
Hurst, K.
Kawamura, T.
Khan, A.
Kim, D.
Knapmeyer, M.
Knapmeyer-Endrun, Brigitte
Lorenz, L.
Margerin, L.
Marusiak, A
Menina, S.
Mittelholz, A.
Murdoch, N.
Nishikawa, Y.
Nunn, C.
Perrin, C.
Pike, William T.
Schmelzbach, C.
Schmerr, N.
Schimmel, Martin
Spiga, A.
Stott, A.
Taylor, J.
Weber, R.
Stahler, S. C.
Panning, Mark P.
Antonangeli, D.
Banerdt, W. B.
Banks, M.
Ceylan, S.
Charalambous, C.
Clinton, John
Daubar, I.
Fernando, B.
Giardini, Domenico
Grott, M.
Horleston, A.
Hurst, K.
Kawamura, T.
Khan, A.
Kim, D.
Knapmeyer, M.
Knapmeyer-Endrun, Brigitte
Lorenz, L.
Margerin, L.
Marusiak, A
Menina, S.
Mittelholz, A.
Murdoch, N.
Nishikawa, Y.
Nunn, C.
Perrin, C.
Pike, William T.
Schmelzbach, C.
Schmerr, N.
Schimmel, Martin
Spiga, A.
Stott, A.
Taylor, J.
Weber, R.
Publication Year :
2023

Abstract

Scientific Rationale: It is by now widely accepted that Mars had a wet and periodically warm past in the Noachian e.g. [1], but it is still open whether liquid water has played any role geologically in recent times or is even present in significant amounts near the surface today e.g. [2]. One key young area are the Cerberus Fossae (C.F.), a system of < 10 Ma old, 1200 km long grabens in Eastern Elysium Planitia. They connect to sediments in Athabasca Valles that have been interpreted as fluvial sediments from a frozen water layer molten by volcanism 8-10 Ma ago [3], but could alternatively be explained by very low viscosity lava as well [4]

Details

Database :
OAIster
Publication Type :
Electronic Resource
Accession number :
edsoai.on1431966297
Document Type :
Electronic Resource