← LeaderboardsInvestigatorsiAttributed = a PI's even-split share of each grant — a $1M grant with 2 PIs counts $500K each.
Planetary Science Institute
Tucson, AZ
$127,367,024
Total funding
369
Grants
Funding over time
peak $34.5M · FY2005–24$50M$37.5M$25M$12.5M$0
'05
'06
'07
'08
'09
'10
'11
'12
'13
'14
'15
'16
'17
'18
'19
'20
'21
'22
'23
'24
Funding mix
By agency
NASA$121,254,400 · 346
NSF$6,112,624 · 23
By mechanism
—$127,367,024 · 369
Investigators at Planetary Science Institute
InvestigatorsiAttributed = a PI's even-split share of each grant — a $1M grant with 2 PIs counts $500K each.
Exposure= the full size of every grant they're on ($1M each).
Rising Stars
First grant in the last 5 yrs
Not enough data
Emerging Leaders
6–10 yrs in
Not enough data
All-Time
Most funded here, all years
Not enough data
Largest grants
MULTIPLE YEAR AWARD WITH INCREMENTAL FUNDING FOR YEARS ONE TO FIVE. THIS PROPOSAL IS ENTITLED "TREX: TOOLBOX FOR RESEARCH AND EXPLORATION." THIS IS AWARDED IN RESPONSE TO COOPERATIVE AGREEMENT NOTICE (CAN) NO. NNH16ZDA009C NASA SOLAR SYSTEM EXPLORATION RESEARCH VIRTUAL INSTITUTE (SSERVI) CYCLE THREE. THE PRINCIPAL INVESTIGATOR IS DR. AMANDA R. HENDRIX WITH PLANETARY SCIENCE INSTITUTE (PSI). PROJECT SUMMARY: THE OVERARCHING GOAL OF THE TREX TEAM IS DEVELOP TOOLS AND RESEARCH METHODS FOR EXPLORATION OF AIRLESS SURFACES THAT ARE COATED IN FINE-GRAINED DUST TO PREPARE FOR HUMAN MISSIONS. OUR TEAM WILL USING LABORATORY SPECTRAL MEASUREMENTS AND EXPERIMENTS ACCOMPANIED BY STUDIES OF EXISTING DATA FROM THE MOON AND SMALL BODIES TO UNDERSTAND THEIR SURFACE CHARACTERISTICS AND TO INVESTIGATE IN SITU RESOURCE UTILIZATION (ISRU) POTENTIAL ON SMALL-BODY TARGETS. ADDITIONALLY OUR TEAM WILL DEVELOP INSTRUMENTATION (ESPECIALLY ULTRA-VIOLET_UV_VISIBLE CAPABILITIES) AND SOFTWARE FOR FUTURE USE AT THOSE BODIES (EITHER REMOTELY AND/OR WITH HUMANS). THESE TOOLS WILL IMPROVE MISSION SUCCESS BY DECREASING RISK AND ASSURING THE SAFETY OF ASTRONAUTS AND SPACECRAFT. THE TREX TASKS COMPLEMENT THOSE OF CURRENT SSERVI TEAMS BY EMPHASIZING ANALYSES OF THE FINEST FRACTION OF GRAINS AND UV WAVELENGTHS. TREX HAS 4 THEMES THAT WILL BE ADDRESSED THROUGH THE LIFE TIME OF THE AWARD. THEY ARE: 1) DEVELOPMENT OF NON-AMBIENT (VACUUM MULTI-TEMPERATURE) BROAD WAVELENGTH SPECTRAL DATABASE OF PLANETARY MATERIALS. WE WILL UTILIZE A RANGE OF FACILITIES TO MAKE THE SPECTRAL MEASUREMENTS WITH UNIQUE AND OVERLAPPING CAPABILITIES IN ORDER TO DERIVE A ROBUST SET OF CROSS-CALIBRATED LAB DATA. 2) INVESTIGATIONS OF FINE-GRAINED MATERIALS ON THE LUNAR SURFACE. LAB DATA FROM THEME ONE WILL BE USED ALONG WITH SPACECRAFT DATA OF THE MOON AND MODELING TECHNIQUES TO CHARACTERIZE LUNAR GRAIN SIZE MINERALOGY AND CORRELATIONS WITH GEOLOGIC FEATURES WITH AN OVERALL GOAL OF INVESTIGATION ISRU POTENTIAL AND FUTURE INSTRUMENT DEVELOPMENT NEEDS. 3) INVESTIGATIONS OF FINE GRAINED MATERIALS ON THE SURFACES OF SMALL BODIES. NEAR EARTH OBJECTS (NEO) AND THE MARTIAN MOONS ARE POTENTIAL FUTURE HUMAN DESTINATIONS AND EVOKE A NUMBER OF CRITICAL QUESTIONS REGARDING THE DIVERSITY OF THEIR COMPOSITIONS AND DYNAMICAL HISTORIES. AND 4) DECISION-MAKING IN A FINE-GRAINED ANALOG ENVIRONMENT. WE WILL DEVELOP BOTH SOFTWARE AND INSTRUMENTATION FOR SUE IN THE FIELD AS A TESTING GROUND FOR FUTURE ROBOTIC PLANETARY USES. THE TASKS ACCOMPLISHED BY THE TREX TEAM WILL ENABLE NASA' EXPLORATION OF THE MOON NEO AND THE MOONS OF THE MARS BY ACQUIRING THE INFORMATION AND KNOWLEDGE THAT WILL SERVE AS TOOLS FOR FUTURE HUMAN AND ROBOTIC EXPLORATION. TREX HAS ASSEMBLED AN INTERNATIONAL TEAM OF EXPERTS TO ADDRESS THESE FOUR THEMES LEVERAGING A NUMBER OF MEMBERS OF THE EXISTING DISTRIBUTED PSI STAFF STRUCTURE AND THEIR EXTENSIVE KNOWLEDGE OF THE MOON SMALL BODIES DATA ANALYSIS AND INSTRUMENT TECHNIQUES AND BY INCORPORATING STUDENTS POST-DOCTORAL RESEARCHERS AND KEY PARTNERS AT OTHER INSTITUTIONS.$5,485,341
· FY2020 · National Aeronautics and Space Administration
PURPOSE THE OVERALL GOAL IS TO CURATE THE EXISTING AND ARCHIVE THE FUTURE SMALL BODIES DATA (COMETS, ASTEROIDS, METEORITES, NEOS, TNOS), ACT AS LEAD$5,303,332
· FY2016 · National Aeronautics and Space Administration
RENEWAL FOR THE COOPERATIVE AGREEMENT NOTICE - THE SMALL BODIES NODE OF NASA'S PLANETARY DATA SYSTEM WITH THE MINOR PLANET CENTER$4,795,957
· FY2022 · National Aeronautics and Space Administration
THE SMALL BODIES NODE (SBN) WAS FIRST CREATED IN A CALL FOR PROPOSALS APPROXIMATELY 15 YEARS AGO. THE ORIGINAL TEAM WAS FORMED FROM PARTICIPANTS IN T$3,259,654
· FY2010 · National Aeronautics and Space Administration
THE NEAR INFRARED VOLATILES SPECTROMETER SYSTEM (NIRVSS) IS AN INSTRUMENT PACKAGE DESIGNED TO ACQUIRE IMAGING AND SPECTRAL DATA OF TARGETS WITHIN THE LUNAR PERMANENTLY SHADED REGIONS (PSRS). AT ITS CORE THE INSTRUMENT CONSISTS OF A MONOCHROMATIC IMAGER AND A SPECTROMETER THAT COVERS THE WAVELENGTH RANGE OF 1.3 M TO 4 M AT A SPECTRAL RESOLUTION OF 15 TO 30 NM. THE IMAGER USES A SET OF COLOR LEDS TO ILLUMINATE THE TARGET AT DIFFERENT WAVELENGTHS WHEREAS A TUNGSTEN LAMP ILLUMINATES THE TARGET FOR THE SPECTROMETER. THREE VERSIONS OF THIS INSTRUMENT ARE EXPECTED TO FLY TO THE MOON AS PAYLOADS ON THE ASTROBOTICS LANDER ON CL19 AND ON THE VOLATILES INVESTIGATING POLAR EXPLORATION ROVER (VIPER) TO BE LAUNCHED ON 2021 2022 AND 2023 RESPECTIVELY. WE PROPOSE HERE TO SUPPORT THE DEVELOPMENT AND OPERATIONS OF NIRVSS BY: 1) DEVELOPING DATA ANALYSIS TOOLS TO USE IN THE INTERPRETATION OF NIRVSS DATA. 2) SUPPORTING DATA ANALYSIS AND INTERPRETATION. 3) PREPARING THE DATA FOR RELEASE WITH THE PDS.$1,810,552
· FY2020 · National Aeronautics and Space Administration
WE PLAN TO INVESTIGATE GEOLOGIC AND TOPOGRAPHIC SETTINGS AND TRIGGERS OF LARGE HISTORIC PRE-HISTORIC AND FUTURE LANDSLIDES IN THE HIMALAYA AND KARAKORAM INCLUDING RIVER DAMMING AND OTHER ASSOCIATED HAZARDOUS EVENTS OF TRANSBOUNDARY CONSEQUENCES. THE REGION OF INTEREST INVOLVES THE INTERNATIONAL BORDER AREAS WITHIN THE LARGER REGION DEPICTED IN FIGURE 1. WE WILL MODEL SUSCEPTIBILITIES OF THE TERRAIN TO PRODUCE SIMILAR LARGE LANDSLIDES IN THE FUTURE DUE TO ICE MELT SEISMICITY OR STOCHASTIC FAILURES. WE WILL USE U OF A S DISTRIBUTED MEMORY CLUSTER TO COMPUTE SEISMIC WAVE PROPAGATION AND SURFACE INTERACTION IN THE COMPLEX TOPOGRAPHY AND FIRST-ORDER GEOLOGIC STRUCTURE OF THE 2015 GORKHA-EARTHQUAKE-AFFECTED HIMALAYAN REGION AND THE 2005 KASHMIR EARTHQUAKE AREA IN THE KARAKORAM. SHAKING-RELATED LANDSLIDE SUSCEPTIBILITY WILL BE TESTED USING OUTCOME OF THE 2015 GORKHA EARTHQUAKE; MONSOON RELATED LANDSLIDES WILL BE EVALUATED NEARBY BUT WHERE SEISMICITY WAS WEAK.$1,345,672
· FY2020 · National Aeronautics and Space Administration
THIS PROPOSAL IS TO SUPPORT THE PI'S ACTIVITIES AS DEPUTY PRINCIPAL INVESTIGATOR OF THE CHEMIN MINERALOGICAL INSTRUMENT THAT IS PART OF THE MARS SCIE$1,109,682
· FY2011 · National Aeronautics and Space Administration
MOTIVATION: THE LUNAR HEAT FLUX RADIOMETER (HFR) WILL PEER INTO THE LUNAR SUBSURFACE USING MICROWAVE WAVELENGTHS (~10-200CM 300MHZ TO 6GHZ AND A 90GHZ SURFACE RADIOMETER) PROVIDING A MEASUREMENT OF GEOTHERMAL HEAT FLUX WITHOUT NEED FOR DRILLING.$1,033,535
· FY2020 · National Aeronautics and Space Administration
UNDERSTANDING RADIATION PROCESSING AND ALTERATION OF ICY REGOLITHS$976,331
· FY2020 · National Aeronautics and Space Administration
SHAPE, TOPOGRAPHY AND INTERNAL STRUCTURE OF MERCURY FROM MDIS DATA DURING THE PAST TWO DECADES, I HAVE DEVELOPED TECHNIQUES FOR COMBINING STEREOGRAPH$897,050
· FY2008 · National Aeronautics and Space Administration
INVESTIGATING THE GEOPHYSICAL CONTROL OF 67P CHURYUMOV GERASIMENKOS OUTBURST PLUMES$887,770
· FY2022 · National Aeronautics and Space Administration
SATELLITE ALTIMETRY HAS RESHAPED OUR VISION OF THE GLOBAL EDDY FIELD WITH LONG-LIVED PROPAGATING COHERENT EDDIES NOW UNDERSTOOD TO BE A MAJOR FEATURE OF THE OCEAN CIRCULATION. MUCH OF OUR UNDERSTANDING OF THE GLOBAL EDDY FIELD IS BASED ON GRIDDED$867,049
· FY2021 · National Aeronautics and Space Administration
PLANETARY SCIENCE INSTITUTE US NEAR-EARTH OBJECT SURVEILLANCE SATELLITE SCIENCE TEAM SUPPORT: THIS PROPOSAL REQUESTS SUPPORT FOR THE PARTICIPATION$851,166
· FY2009 · National Aeronautics and Space Administration
THE AIM OF THE PROPOSED WORK IS TO EVALUATE A NEW SCINTILLATOR, EUROPIUM DOPED STRONTIUM IODIDE, FOR PLANETARY GAMMA RAY SPECTROSCOPY. THE PROPOSAL W$841,885
· FY2016 · National Aeronautics and Space Administration
WE PROPOSE TO STUDY AN INSTRUMENT CONCEPT TO IMPROVE UPON CURRENT CAPABILITIES IN UV IMAGING SPECTROSCOPY FOR PLANETARY USES. THE CONCEPT IS A UV MICROMIRROR SPECTROGRAPH WITH A WIDE VARIETY OF POTENTIAL APPLICATIONS INCLUDING DISCOVERY- AND NEW FRONTIERS-CLASS MISSIONS. THE STATE-OF-THE-ART UV IMAGING SPECTROGRAPHS SUCH AS THE SWRI-BUILT ALICE INSTRUMENTS (INCLUDING JUNO UVS ROSETTA ALICE AND LRO LAMP) AND THE LASP-BUILT CASSINI UVIS AND MAVEN IUVS RETURN USEFUL DATASETS FROM THEIR TARGETS AND HAVE OPENED UP THE FIELD TO THE NEXT QUESTIONS TO ADDRESS. RECENT TECHNOLOGICAL ADVANCES HAVE ENABLED INSTRUMENT IMPROVEMENTS FOR THE NEXT GENERATION OF PLANETARY SCIENCE MISSIONS. FURTHERMORE A RANGE OF POSSIBLE UPCOMING MISSIONS COULD SUCCESSFULLY UTILIZE SUCH IMPROVED UV INSTRUMENTATION. THE GOAL OF THIS PROGRAM IS TO DEVELOP A PROOF-OF-CONCEPT INSTRUMENT FOR INTEGRAL FIELD FAR-UV SPECTROSCOPY. BY UTILIZING A PAIR OF DIGITAL MICROMIRROR ARRAYS THIS CONCEPT INSTRUMENT WILL BE CAPABLE OF DISSECTING THE FOCAL PLANE AND RE-FORMING IT INTO A SERIES OF SLITSHAPES TO OVERCOME THE LIMITATIONS OF SPECTRAL CONFUSION. THE TRL OF THE SYSTEM IS CURRENTLY ESTIMATED AT ~2. WE EXPECT TO ADVANCE THE TRL TO ~4 THROUGH THIS PICASSO PROGRAM TO BE READY TO PROPOSE TO MATISSE FOR FOLLOW-ON WORK AND FURTHER TRL ADVANCEMENT.$836,502
· FY2020 · National Aeronautics and Space Administration
NASA S DAWN SPACECRAFT COMPLETED ITS YEARLONG MAPPING MISSION AROUND ASTEROID (4) VESTA IN AUGUST 2012. DURING THIS PERIOD, THE DAWN FRAMING CAMERA ($795,222
· FY2014 · National Aeronautics and Space Administration
THIS PROPOSAL COVERS DR. DAVID VANIMAN'S ACTIVITIES AS A CO-INVESTIGATOR FOR THE CHEMIN MINERALOGICAL INSTRUMENT WHICH IS PART OF THE INSTRUMENT SUITE ON THE MARS SCIENCE LABORATORY (MSL) ROVER CURIOSITY DURING THE EXTENDED MISSION PHASE THROUGH 2019 AND INTO 2021. THE PROPOSAL INCLUDES CONTINUING SUPPORT FOR STEVE CHIPERA AS WELL AS COVERAGE FOR DR. PATRICIA CRAIG AS A CHEMIN POST-DOCTORAL RESEARCH SCIENTIST. DR. VANIMAN WAS A NAMED CO-I ON THE ORIGINAL CHEMIN INSTRUMENT PROPOSAL SUBMITTED TO THE MSL MISSION ANNOUNCEMENT OF OPPORTUNITY AND HIS INCLUSION WAS VALIDATED AT THAT TIME BY DR. MICHAEL MEYER MARS PROGRAM SCIENTIST AT NASA HEADQUARTERS. IN THE INTERVAL BETWEEN CHEMIN'S SELECTION AS AN MSL PAYLOAD ELEMENT AND THE LAUNCH OFMSL (PHASES A-D OF THE INSTRUMENT PROJECT) DR. VANIMAN WAS SUPPORTED THROUGH CONTRACTS ADMINISTERED DIRECTLY FROM THE MARS PROGRAM OFFICE AT THE JET PROPULSION LABORATORY DURING WHICH TIME HE WAS MADE DEPUTY PI OF CHEMIN. IN THIS CAPACITY DAVID VANIMAN HAS HAD EQUAL AUTHORITY AND RESPONSIBILITY TO THE CHEMIN PI DR. DAVID BLAKE. DURING PHASE E OF THE INSTRUMENT PROJECT (MISSION OPERATIONS) VANIMAN'S ACTIVITIES HAVE BEEN SUPPORTED THROUGH COOP AGREEMENTS ADMINISTERED THROUGH AMES RESEARCH CENTER. IN 2017 THE DEPUTY PI WERE TRANSFERRED TO ELIZABETH RAMPE OFNASA-JSC AND VANIMAN TRANSITIONED TO CO-I STATUS; THIS TRANSITION WAS AGREED TO BY MICHAEL MEYER MARS PROGRAM SCIENTIST AT NASA HEADQUARTERS. THE DUTIES AND OBLIGATIONS OF CHEMIN CO-I'S FOR THE PRIME MISSION WERE DELINEATED IN THE CHEMIN EXPERIMENT OPERATIONS PLAN (JPL D-36918) "CHEMIN EOP" OR "EOP" AND PUBLICATIONS LISTED THEREIN. THESE DUTIES AND OBLIGATIONS HAVE WORKED WELL DURING THE PRIME MISSION AND THE FIRST AND SECOND EXTENDED MISSIONS AND WILL BE MAINTAINED INTO THE THIRD EXTENDED MISSION.$790,760
· FY2020 · National Aeronautics and Space Administration
THE PLANETARY SCIENCE INSTITUTE (PSI) WITH OUR PARTNER THE TUCSON REGIONAL SCIENCE CENTER (RSC) PROPOSES TO: 1) OFFER A SERIES OF PROFESSIONAL DEVE$750,188
· FY2010 · National Aeronautics and Space Administration
WE WILL OBSERVE 38 UHJS USING THREE SITES IN THE NORTHERN AND SOUTHERN HEMISPHERE USING MOSTLY MODERATE-APERTURE ROBOTICIZED TELESCOPES TO ACQUIRE HUNDREDS OF TRANSITS WITH MIDTIMES ACCURATE TO 1-2 MINUTES. WE WILL UPDATE THE TRANSIT EPHEMERIDES$705,335
· FY2022 · National Aeronautics and Space Administration
SULFATES ARE A COMMON MINERAL IDENTIFIED FROM ORBITAL REMOTE SENSING DATA OF MARS WITH SEVERAL LOCATIONS HAVING LARGE DEPOSITS SUCH AS MERIDIANI PLANUM VALLES MARINERIS AND THE CENTRAL MOUND IN GALE CRATER (AEOLIS MONS). THE GALE SULFATES LIE ABOVE A PHYLLOSILICATE UNIT AND BELOW A SPECTRALLY BLAND POSSIBLE AEOLIAN DEPOSIT. BOTH MONOHYDRATED AND POLYHYDRATED SULFATES HAVE BEEN IDENTIFIED WITHIN AEOLIS MONS. ADDITIONALLY A DARK-TONED MARKER BED IS OBSERVED WITHIN THE SULFATES AT GALE BUT ITS EXTENT AND ORIGIN ARE UNKNOWN. IN PREPARATION FOR THE SULFATE INVESTIGATION BY THE CURIOSITY ROVER WE INTEND TO PERFORM A DETAILED STUDY OF THE SULFATES ACROSS AEOLIS MONS USING ORBITAL REMOTE SENSING DATA SETS. FOR THIS PROJECT WE HAVE OUTLINED SEVERAL TASKS THAT WILL CHARACTERIZE AND INTERPRET THE SULFATES AND MARKER BED WITHIN AEOLIS MONS TO PROVIDE ADDITIONAL INSIGHTS INTO THE GEOLOGIC HISTORY OF GALE CRATER AND THE FORMATION OF SULFATES ON MARS. TASK 1 WILL USE CRISM IMAGES TO DETERMINE THE COMPOSITION OF THE SULFATES IN PARTICULAR DISTINGUISHING BETWEEN MONOHYDRATED AND POLYHYDRATED SULFATES AS WELL AS OTHER MINERALS MIXED WITH THE SULFATES. THESE CRISM IMAGES COMBINED WITH VISIBLE IMAGES FROM HIRISE CTX AND HRSC IMAGES WILL BE USED FOR GEOLOGIC MAPPING OF THE SULFATES AND MARKER BED ACROSS THE ENTIRE MOUND EXTENDING THE MAPPING CURRENTLY BEING PERFORMED AT 1:60 000 SCALE OF WESTERN AEOLIS MONS BY CO-I THOMSON. TASK 2 WILL PRODUCE 8 NEW HIRISE-DERIVED DIGITAL TERRAIN MODELS (DTMS) AND THEN MEASURE BEDDING ORIENTATION AND THICKNESS OF THE SULFATES AND MARKER BED FROM THESE DTMS. WE WILL CREATE DETAILED STRATIGRAPHIC SECTIONS AT APPROXIMATELY 8-12 LOCATIONS ACROSS AEOLIS MONS THAT ENCOMPASS THE SULFATES AND THE MARKER BED. THE RESULTS WILL ENHANCE OUR UNDERSTANDING OF THE VERTICAL AND LATERAL VARIABILITY OF THE SULFATES AND DETERMINE IF THE SULFATES THAT WILL BE EXPLORED BY THE CURIOSITY ROVER ARE REPRESENTATIVE OF ALL THE SULFATES SEEN FROM ORBIT ACROSS AEOLIS MONS. FOR THE MARKER BED WE WILL UTILIZE THE DTMS TO DETERMINE IF THE BED ALWAYS OCCURS BETWEEN THE SAME SULFATE LAYERS MEASURE ITS ELEVATION AND THICKNESS ACROSS AEOLIS MONS AND LOOK FOR VARIATIONS IN SLOPE AND DIP OF THE BED. WE WILL THEN USE THESE MEASUREMENTS TO SUGGEST THE MOST PLAUSIBLE FORMATION MECHANISM(S) FOR THE MARKER BED AS WELL AS IDENTIFY THE KEY QUESTIONS ABOUT THE MARKER BED THAT COULD BE ADDRESSED BY THE MSL ROVER INSTRUMENTS AS PART OF TASK 4. TASK 3 WILL COMPARE OUR RESULTS FROM THE GALE SULFATES TO OTHER SULFATES FOUND ON MARS ESPECIALLY THOSE IN MERIDIANI PLANUM AND VALLES MARINERIS WHERE TEAM MEMBERS HAVE ALREADY CONDUCTED PREVIOUS ANALYSES. THE GOAL IS TO LEARN IF THE GALE SULFATES ARE SIMILAR IN THEIR COMPOSITION AND MORPHOLOGY TO OTHER MARTIAN SULFATE DEPOSITS. FORMATION SCENARIOS FOR THE SULFATES WITHIN THE GALE MOUND WILL BE INVESTIGATED IN RELATION TO OTHERS ON MARS USING PREVIOUSLY PUBLISHED CHEMICAL MODELING AND LABORATORY STUDIES OF SULFATE DEPOSITION. TASK 4 WILL LOOK SPECIFICALLY AT ORBITAL DATA OF THE SULFATES THAT ARE LIKELY TO BE TRAVERSED BY THE CURIOSITY ROVER IN ORDER TO RELAY OUR FINDINGS FROM THIS INVESTIGATION AND PROVIDE KEY QUESTIONS TO THE MSL SCIENCE TEAM THAT COULD BE INVESTIGATED BY THE ROVER ONCE IT REACHES THE SULFATES AND MARKER BED BASED UPON OUR RESULTS FROM TASKS 1-3. THIS PROPOSAL IS RELEVANT TO MDAP BECAUSE IT ADDRESSES THE MDAP GOAL TO ENHANCE THE SCIENTIFIC RETURN FROM MISSIONS TO MARS CONDUCTED BY NASA AND OTHER SPACE AGENCIES BY USING MULTIPLE MARTIAN DATA SETS FROM FOUR SEPARATE ORBITAL MISSIONS (MGS ODY MEX AND MRO) AND WILL CONTRIBUTE TO ONGOING GEOLOGIC ANALYSES OF THE SURFACE OF MARS WITH A FOCUS ON SULFATE DEPOSITS AT GALE CRATER.$678,815
· FY2020 · National Aeronautics and Space Administration