10 caprarelli etal_schiaparelli_29_02_2012

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SCHIAPARELLI CRATER G. Caprarelli 1 , M. Pondrelli 2 , E. Jones 3 , D. Flannery 4 , R. Orosei 5 , M. Walter 4 , C. Lineweaver 3 1 School of the Environment, University of Technology Sydney, PO Box 123, Broadway, NSW 2007, Australia; 2 International Research School of Planetary Sciences, Università G. d’Annunzio, V.lePindaro 42, 65127 Pescara (Italy); 3 Planetary Science Institute, Research School of Astronomy and Astrophysics and Research School of Earth Sciences, Australian National University, Canberra, ACT, 0200, Australia; 4 Australian Centre for Astrobiology, School of Biotechnology and Biomolecular Sciences, The University of New South Wales, Sydney, 2052, Australia; 5 National Institute for Astrophysics - Physics of Interplanetary Space (INAF-IFSI), 100 Via del Fosso del Cavaliere, 00133 Rome (Italy). NOTE ADDED BY JPL WEBMASTER: This content has not been approved or adopted by, NASA, JPL, or the California Institute of Technology. This document is being made available for information purposes only, and any views and opinions expressed herein do not necessarily state or reflect those of NASA, JPL, or the California Institute of Technology.

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Page 1: 10 caprarelli etal_schiaparelli_29_02_2012

SCHIAPARELLI CRATER

G. Caprarelli1, M. Pondrelli2, E. Jones3, D. Flannery4, R. Orosei5, M. Walter4, C. Lineweaver3

1School of the Environment, University of Technology Sydney, PO Box 123, Broadway, NSW 2007, Australia; 2International Research School of Planetary Sciences, Università

G. d’Annunzio, V.le Pindaro 42, 65127 Pescara (Italy); 3Planetary Science Institute, Research School of Astronomy and Astrophysics and Research School of Earth

Sciences, Australian National University, Canberra, ACT, 0200, Australia; 4Australian Centre for Astrobiology, School of Biotechnology and Biomolecular Sciences, The

University of New South Wales, Sydney, 2052, Australia; 5National Institute for Astrophysics - Physics of Interplanetary Space (INAF-IFSI), 100 Via del Fosso del

Cavaliere, 00133 Rome (Italy).

NOTE ADDED BY JPL WEBMASTER: This content has not been approved or adopted by, NASA, JPL, or the California Institute of Technology. This document is being made available for information purposes only, and any views and opinions expressed herein do not necessarily state or reflect those of NASA, JPL, or the California Institute of Technology.

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0 60°E

30°N

30°S

30°W

60°S

30°E 90°E

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Previous work

(in / around Schiaparelli)

• Mouginis-Mark et al. (1981)� Geologic reconstruction

• Malin and Edgett (2000)� Light toned deposits

• Kass et al. (2003)� Landing conditions (“safe” landing)

• Wiseman et al. (2009; 2010)� Hydrated minerals (Schiaparelli; Meridiani)

• Feldman et al. (2011, and earlier papers)� Neutron data

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Wiseman et

al. (2009)

Malin and Edgett(2000)

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< 2 2-10 > 10

SLOPES (°)

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Site Name SCHIAPARELLI CRATER

Landing Ellipse Center Coordinates:Latitude, Longitude 3.942°S, 13.875°E

MOLA elevation -0.150 km

Prime Science and Sampling Targets 1. Hydrated minerals [Highest Priority]

2. Rock specimens from rim of Schiaparelli [LowestPriority]

Distance of Science and/or Sampling Targets from Ellipse Center

Hydrated minerals – 50 km to N

Rocks – 30 km to W

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H8363_0000

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H8363_0000

C2

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H8363_0000

C2

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r0600047

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Rationale and Conclusion

• Long geological history

• Variety of lithotypes

• Evidence of near surface hydrated mineral deposits near surface

• “Safe” landing site

• Proximity of landing site to:� Outcrops of possible subsurface rocks (C2)

� Rim of crater� Sampling of rim > Ancient geological history

� Possible egress out of crater for sampling of surrounding area