1. Jet Propulsion Laboratory California Institute of Technology Pasadena, CA Current Orbiter Capabilities for Future Landing Site Selection Richard Zurek Mars Program Office Chief Scientist Jet Propulsion Laboratory California Institute of Technology MRO Mars Express Odyssey

2. Jet Propulsion Laboratory California Institute of Technology Pasadena, CA Proposed* Mars Mission Architecture MRO Mars Express Odyssey MER 2013 2011 Operational Phoenix (completed) Phoenix (completed) Mars Science Laboratory 2001-2007 MAVEN* Aeronomy Orbiter *Proposed Missions 2009 2016 2018 2020 & Beyond ESA—NASA ExoMars Trace Gas Orbiter* ESA—NASA ExoMars Trace Gas Orbiter* NASA—ESA Rovers* (Astrobiology/ Sample Return Cache) NASA—ESA Rovers* (Astrobiology/ Sample Return Cache) Possible NASA-ESA Joint Mars Initiative 2 Pre-decisional - For Planning and Discussion Purposes Only ESA—EDL Demonstrator*

3. Jet Propulsion Laboratory California Institute of Technology Pasadena, CA Orbiter Support for Future Missions Orbital Information is critical to future missions landing on Mars in the following ways: –Identification, Characterization, and Certification (for safety) of landing sites –Characterization of atmospheric environments for EDL –Characterization of surface environments for landed operations MER, PHX and MSL have all benefited from such data Future landers now proposed include the ExoMars 2016 EDM and a 2018 Dual Rover missions Large areas of the planet have been covered at increased spatial resolutions, with some coverage continuing to expand Major assets for providing additional critical data are currently: ODY, MEX, MRO –2016 EMTGO data would arrive late in the process for any launch in 2018 po3 Pre-decisional - For Planning and Discussion Purposes Only

4. Jet Propulsion Laboratory California Institute of Technology Pasadena, CA HRSC OMEGA Surface Spatial Scale 1 km 300 m 100 m 30 m 10 m 3 m 1m 0.3 m Visible Visible - Near Infrared Thermal Wavelength Phenomena Sea beds? Channels Polar Layering Paleolakes? Salt Flats? Layering Vents/Springs? Mineral Deposits Gullies Debris Fans Fine Layering Patterned Ground Fractures Rocks THEMIS VIS THEMIS TES MOC-NA MOC-WA HRSC (SRC) MRO CRISM- Survey CTX MARCI CRISM HiRISE MEX ODY MGS MOC 1-D CPROTO Required for Site Certification & Morphologic Detail Thousands of small area exposures Stratigraphic relationships of layers with aqueous minerals Observation Attributes ~70% 100% ~2% ~1% ~62% ~56% 4 Daily Global Maps >>50% ~40% ~85% 2.8%

5. Jet Propulsion Laboratory California Institute of Technology Pasadena, CA Surface Coverage ProjectTeamObservationObjectiveResoln: m/pixelCoverage* ODYTHEMIS (mid) Day IR (late) Day IR Night IR VIS Composition Morphology Thermal Inertia Morphology 100 18 ~ 40% (55%) ~100% ~ 40% (54%) MEX HRSC VIS (color, stereo) Morphology≤ 20 ≤ 60 ~56% ~85% OMEGA VIS-IRComposition~300>> 50% CRISM VIS-NIRComposition ~200 in 72 bnd ~200 in 264 bnd ~ 18 in 544 bnd ~70% (80%) ~15% ~ few % MROCTX VIS (stereo)Morphology~ 6 62% HiRISE VIS (stereo, color swath) Morphology (composition) ~0.3 – 0.6 (color) ~ 1% 5 * % of Mars surface covered with good quality data (total including high opacity periods)

6. Jet Propulsion Laboratory California Institute of Technology Pasadena, CA MEX HRSC Coverage 6 Totals: 56% at ≤ 20 m/pixel 85% at ≤ 60 m/pixel

7. Jet Propulsion Laboratory California Institute of Technology Pasadena, CA MRO CTX Coverage Map 7 As of July 31, 2010 MSSS / JPL / NASA

8. Jet Propulsion Laboratory California Institute of Technology Pasadena, CA Coverage by time under low-opacity conditions Coverage by latitude under low-opacity conditions MRO CRISM Coverage (as of Sep. 2010) ~71% low-opacity mapping coverage TypePSP+ESPESP FRT100453918 HRL31951286 HRS1719795 Targeted total149595999 EPF58852164 LMB94 Gimbaled Total 209388257 TOD94526082 MSW25570 MSP segment4303812547 HSP segment6968 HSV segment1449 Survey segment total 5145520964 8

9. Jet Propulsion Laboratory California Institute of Technology Pasadena, CA Capabilities for Site Selection (1 of 2) ODY: Approved for second Extended Mission (FY11-12) −THEMIS IR & VIS: Working well in mid-afternoon orbit −Limited fuel will still support operations thru MSL prime mission MEX: Approved thru FY10, likely to be confirmed thru 2012, and request to be extended thru FY14 under review −Uncertain remaining fuel load should support operations thru this period −Orbit phasing periodically limits day-time viewing −All instruments still operating MRO: Approved for first full Extended Mission (FY11-12) −Telecom is essentially single string, but has been that way for 4 years −Safe mode entries vexing, but not thought to be life-limiting −Fuel not currently an issue given latest scenarios for covering MSL EDL −MCS, MARCI, CTX, SHARAD continue to work as in PSP/ESP −HiRISE and CRISM have seen some degradation (next slide) 9

10. Jet Propulsion Laboratory California Institute of Technology Pasadena, CA Capabilities for Site Selection (2 of 2) MRO instrument issues: –HiRISE: Team has used longer and more frequent warm-ups to compensate for increasing ADC (analog to digital converters) bit flip errors Considering an onboard annealing sequence which ground testing indicates could reduce errors by breaking up and dispersing the ADC contamination −CRISM: Both the gimbal (needed for high resolution) and the coolers (needed for IR observations) have degraded with time Plan: Use full VNIR/IR capability for 2 weeks every other month in mini- campaigns focused on high priority items (especially during periods of higher data rate) VNIR-only mode can be used at other times (but avoid major dust events) o VNIR (0.4 to 1.1µm) aqueous mineral signatures are limited to ferric minerals Bottom Line: Full-resolution VNIR/IR targeting reserved for high priority targets 10

11. Jet Propulsion Laboratory California Institute of Technology Pasadena, CA MRO EM Predicted Data Volumes MSL Launch MSL Arrival Solar Conjunction S. SummerN. SpringN. Summer 270Ls = 090180 (Relatively) Low Dust Opacity

12. Jet Propulsion Laboratory California Institute of Technology Pasadena, CA Summary Current Orbiter capabilities for support of future landed missions are substantial, but instruments and spacecraft are aging –Best to start the process now for proposed missions like 2018 Need site criteria (e.g., as being developed by the E2E SAG) –Need to use the capabilities conservatively where instrument and/or spacecraft limitations dictate Landing site selection processes should be structured so that the life-limited capabilities are used only for the highest priority items –Need to use the data already in hand—there’s a lot, even though more needs to be done on many interesting places –Need to set site priorities using existing data and increased coverage of lower resolution/survey observations May be useful to exploit correlations that have emerged between spectral and visible imagers (e.g., color variations and VNIR, IR & thermal IR) –Need to have realistic expectations about the number of sites that could be certified (i.e., with nearly complete high resolution coverage) and the schedule of data acquisition 12 Pre-decisional - For Planning and Discussion Purposes Only