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| Título: | A Cerberus Fossae Seismic Network |
Autor: | Stahler, S. C.; Panning, Mark P.; Antonangeli, D.; Banerdt, W. B.; Banks, M.; Ceylan, S.; Charalambous, C. CSIC ORCID; 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 CSIC ORCID ; Spiga, A.; Stott, A.; Taylor, J.; Weber, R. | Palabras clave: | Mission goals of a proposed Cerberus Fossae Seismic Network | Fecha de publicación: | 13-mar-2023 | Resumen: | 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] | URI: | http://hdl.handle.net/10261/352167 |
| Aparece en las colecciones: | (Geo3Bcn) Comunicaciones congresos |
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