1 / 18

Vasco da Gama

Vasco da Gama. In Situ Mars Explorer. Scientific Goals. Follow the Carbon Methane, Other Organics Possible association with water Link carbon and geological features to possible extant and extinct life. Roadmap. Precursor Mission & Assumptions Landing site discussion

muriel
Download Presentation

Vasco da Gama

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. Vasco da Gama In Situ Mars Explorer VdG:ISME - July 2004

  2. Scientific Goals • Follow the Carbon • Methane, Other Organics • Possible association with water • Link carbon and geological features to possible extant and extinct life VdG:ISME - July 2004

  3. Roadmap • Precursor Mission & Assumptions • Landing site discussion • Scientific and Technical Justifications • Rover concept • Payload package • Bioscience and Geochemical Science • Summary VdG:ISME - July 2004

  4. Precursor mission • Spaced-based remote sensing (in development) • Avoids terrestrial atmospheric extinction • Spatially resolved measurements of atmospheric CH4 and photochemical products on Mars (Organics Origin Observatory) • Fundamental assumption and problem definition • Precursor space-based mission has spatially resolved methane gradients, focusing the search for carbon reservoirs in potential VdG:ISME landing sites VdG:ISME - July 2004

  5. Landing Sites • Equatorial Meridiani • Relatively near Opportunity • Hale Crater Gullies • 35o S, 324o E VdG:ISME - July 2004

  6. Landing Sites VdG:ISME - July 2004

  7. Scientific Justification: Meridiani • Atmospheric CH4 localization assumed • Interesting even if this is not assumed • Nature of hydrogen detection? • Relatively warm • Surface sulfates, hematite co-localized • Carbonates below these? • Aqueous precipitates can preserve micro-fossils (Squyres 2004, Int’l School for Astrobiology) VdG:ISME - July 2004

  8. Hale Crater Gullies • Again, assumed CH4 (although very tentative “current-day” detections indicate equatorial presence) • Possible water signatures (possible carbonates) • Natural surface excavation • Possible hydrothermal alteration VdG:ISME - July 2004

  9. Malin and Edgett 2000 Gullies VdG:ISME - July 2004

  10. Technical Justification-Landing • Landing error ellipse shrunk to 5km x 10km • Practical, uncomplicated, low-mass methods to increase accuracy • Navigation telemetry from existing positions to increase transverse accuracy • Closed-loop navigation system to respond to sensed variations in atmospheric density (Squyres 2004, personal communication) VdG:ISME - July 2004

  11. Hale Landing • Feasible • Smaller error ellipse • Increased rover range Edgett et al. 2003 VdG:ISME - July 2004

  12. The Rovers • Science payloads identical • Both have slope-climbing abilities • Powered by RTGs • Eliminates low-latitude and nighttime operations as a hazard • Heavier spacecraft, but increases operational parameters • Digging scoop • depth 1m in regolith VdG:ISME - July 2004

  13. Instrumentation • Main body • Pancam copy, Mini mid IR TES (MMIRTES) • Raman analysis and multi-range sensing package (up to 100m) • GCMS • rock-crushing package • Circular Dichroism Filter Set Spectrometer • 96 well culture plates, geared towards autotrophic methanogens VdG:ISME - July 2004

  14. Instrumentation • Manipulator arm • Microscope with fluorescence capabilities • Raman Capabilities (via fibre optics) • Mössbauer • APXS with micron sized mapping • Sample manipulation VdG:ISME - July 2004

  15. Raman • Complements MMIRTES • Organics • Minerals VdG:ISME - July 2004 Ellery & Wynn-Williams 2003

  16. GCMS NAP Signs of Life, Moldowan VdG:ISME - July 2004

  17. H2/CO2 atmosphere shielded from martian surface radiation Moveable 100x microscope Tiny Mars rock (~1mm) 500uL media: Combinations of organic rich, organic poor, nitrates, and phosphates DAPI, (gradual sonication) Light source (for microscopy) VdG:ISME - July 2004

  18. Summary • Precursor methane localization • Twin Rovers • Meridiani & Hale Crater gullies • Rovers • Climbing capabilities • Enhanced power • Enhanced instrument package (Raman, GCMS, Fluorescence) • Dual biological and geological payload VdG:ISME - July 2004

More Related