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Por favor, use este identificador para citar o enlazar a este item: http://hdl.handle.net/10261/352167
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dc.contributor.authorStahler, S. C.-
dc.contributor.authorPanning, Mark P.-
dc.contributor.authorAntonangeli, D.-
dc.contributor.authorBanerdt, W. B.-
dc.contributor.authorBanks, M.-
dc.contributor.authorCeylan, S.-
dc.contributor.authorCharalambous, C.-
dc.contributor.authorClinton, John-
dc.contributor.authorDaubar, I.-
dc.contributor.authorFernando, B.-
dc.contributor.authorGiardini, Domenico-
dc.contributor.authorGrott, M.-
dc.contributor.authorHorleston, A.-
dc.contributor.authorHurst, K.-
dc.contributor.authorKawamura, T.-
dc.contributor.authorKhan, A.-
dc.contributor.authorKim, D.-
dc.contributor.authorKnapmeyer, M.-
dc.contributor.authorKnapmeyer-Endrun, Brigitte-
dc.contributor.authorLorenz, L.-
dc.contributor.authorMargerin, L.-
dc.contributor.authorMarusiak, A-
dc.contributor.authorMenina, S.-
dc.contributor.authorMittelholz, A.-
dc.contributor.authorMurdoch, N.-
dc.contributor.authorNishikawa, Y.-
dc.contributor.authorNunn, C.-
dc.contributor.authorPerrin, C.-
dc.contributor.authorPike, William T.-
dc.contributor.authorSchmelzbach, C.-
dc.contributor.authorSchmerr, N.-
dc.contributor.authorSchimmel, Martin-
dc.contributor.authorSpiga, A.-
dc.contributor.authorStott, A.-
dc.contributor.authorTaylor, J.-
dc.contributor.authorWeber, R.-
dc.date.accessioned2024-03-28T08:27:37Z-
dc.date.available2024-03-28T08:27:37Z-
dc.date.issued2023-03-13-
dc.identifier.urihttp://hdl.handle.net/10261/352167-
dc.description.abstractScientific 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]-
dc.languageeng-
dc.relation.isversionofPublisher's version-
dc.subjectMission goals of a proposed Cerberus Fossae Seismic Network-
dc.titleA Cerberus Fossae Seismic Network-
dc.typecomunicación de congreso-
dc.date.updated2024-03-28T08:27:37Z-
dc.rights.holderopenAccess-
dc.rights.licensehttp://creativecommons.org/licenses/by/4.0/-
dc.relation.csicSí-
dc.type.coarhttp://purl.org/coar/resource_type/c_5794es_ES
item.grantfulltextopen-
item.fulltextWith Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
item.openairetypecomunicación de congreso-
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