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Accumulation and erosion of Mars' south polar layered deposits
Authors:Seu Roberto  Phillips Roger J  Alberti Giovanni  Biccari Daniela  Bonaventura Francesco  Bortone Marco  Calabrese Diego  Campbell Bruce A  Cartacci Marco  Carter Lynn M  Catallo Claudio  Croce Anna  Croci Renato  Cutigni Marco  Di Placido Antonio  Dinardo Salvatore  Federico Costanzo  Flamini Enrico  Fois Franco  Frigeri Alessandro  Fuga Oreste  Giacomoni Emanuele  Gim Yonggyu  Guelfi Mauro  Holt John W  Kofman Wlodek  Leuschen Carlton J  Marinangeli Lucia  Marras Paolo  Masdea Arturo  Mattei Stefania  Mecozzi Riccardo  Milkovich Sarah M  Morlupi Antonio  Mouginot Jérémie  Orosei Roberto  Papa Claudio  Paternò Tobia
Institution:Dipartimento INFOCOM, Università di Roma "La Sapienza," I-00184 Rome, Italy. roberto.seu@uniroma1.it
Abstract:Mars' polar regions are covered with ice-rich layered deposits that potentially contain a record of climate variations. The sounding radar SHARAD on the Mars Reconnaissance Orbiter mapped detailed subsurface stratigraphy in the Promethei Lingula region of the south polar plateau, Planum Australe. Radar reflections interpreted as layers are correlated across adjacent orbits and are continuous for up to 150 kilometers along spacecraft orbital tracks. The reflectors are often separated into discrete reflector sequences, and strong echoes are seen as deep as 1 kilometer. In some cases, the sequences are dipping with respect to each other, suggesting an interdepositional period of erosion. In Australe Sulci, layers are exhumed, indicating recent erosion.
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