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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.
0 60°E
30°N
30°S
30°W
60°S
30°E 90°E
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
Wiseman et
al. (2009)
Malin and Edgett(2000)
< 2 2-10 > 10
SLOPES (°)
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 [Lowest
Priority]
Distance of Science and/or Sampling Targets from
Ellipse Center
Hydrated minerals – 50 km to N
Rocks – 30 km to W
H8363_0000
H8363_0000
C2
H8363_0000
C2
r0600047
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

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10 caprarelli etal_schiaparelli_29_02_2012

  • 1. 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.
  • 3. 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
  • 4. Wiseman et al. (2009) Malin and Edgett(2000)
  • 5. < 2 2-10 > 10 SLOPES (°)
  • 6. 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 [Lowest Priority] Distance of Science and/or Sampling Targets from Ellipse Center Hydrated minerals – 50 km to N Rocks – 30 km to W
  • 11. 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