Analyze awards, watch incumbents and competitors, track new transactions or changes, and use award history to shape recompete and capture strategy.
Award ID | Description | Recipient | Total Value | Awarding Agency | Funding Agency | Set Aside | NAICS | PSC | Award Date | Start Date | End Date | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| REFRACTORY MINERALS - ARCHIVES FROM THE EARLY SOLAR SYSTEM | FIELD MUSEUM OF NATURAL HISTORY | $515,863 | NATIONAL AERONAUTICS AND SPACE ADMINISTRATION | NATIONAL AERONAUTICS AND SPACE ADMINISTRATION | — | — | AJ11GENERAL SCIENCE AND TECHNOLOGY R&D SERVICES; GENERAL SCIENCE AND TECHNOLOGY; BASIC RESEARCH | Feb 5, 2021 | Jan 1, 2021 | Jun 30, 2026 | ||
| THE KNOWLEDGE OF THE ORIGIN OF THE STARTING MATERIAL OF OUR SOLAR SYSTEM IS AN ISSUE OF FUNDAMENTAL INTEREST IN PLANETARY SCIENCE. AFTER THE DISCOVERY OF PRESOLAR GRAINS (PSG) IN 1987 IT WAS POSSIBLE FOR THE FIRST TIME TO STUDY SOLID SAMPLES OF STARS IN THE LABORATORY. THIS PROVIDED A UNIQUE PERSPECTIVE ON THE ORIGIN AND COMPOSITION OF THE MATERIAL FROM WHICH THE SOLAR SYSTEM FORMED. WE PROPOSE TO USE ATOM-PROBE TOMOGRAPHY (APT) TO STUDY THE COMPOSITIONS OF PRESOLAR NANOGRAINS THAT ARE TOO SMALL TO STUDY WITH NANOSIMS. THE GOAL IS TO BETTER UNDERSTAND THE ORIGINS OF THESE UNDERSTUDIED SAMPLES, INFORMATION NOT OBTAINABLE OTHERWISE (TASK 1). WE ALSO PROPOSE TO EXTEND THE SMALL NUMBER OF KNOWN PRESOLAR EXPOSURE AGES OF LARGE PRESOLAR SIC GRAINS. OUR APPROACH IS TO USE HE AND NE, AND LI ISOTOPIC ANALYSIS IN CONJUNCTION WITH IMPROVED NUCLEAR RECOIL CORRECTIONS AND PRODUCTION RATES FOR COSMOGENIC NUCLIDES TO STUDY THE PRESOLAR CHRONOLOGY OF THE SOLAR SYSTEM S STARTING MATERIAL (TASK 2). TASK 1: MUCH FRUITFUL EFFORT WAS DEVOTED TO THE ANALYSES OF PSG IN THE UM-SIZE RANGE TO DETERMINE STELLAR SOURCES AND TO GAIN UNPRECEDENTED INSIGHT INTO PROCESSES OPERATING WITHIN THOSE STARS. WHILE PSG IN THIS SIZE RANGE ARE READILY ACCESSIBLE TO ION PROBES, THEY ARE NOT NECESSARILY REPRESENTATIVE OF SMALLER PSG. THE SMALLEST SIZE FRACTION OF PRESOLAR CR-RICH SPINELS WAS DISCOVERED TO CARRY THE LARGEST ISOTOPIC ANOMALIES. THE SMALL FRACTION OF PRESOLAR NANODIAMONDS HAS NOT YET BEEN QUANTIFIED. EVEN WITH THE LATEST GENERATION OF THE HIGHEST RESOLUTION ION PROBE, THE NANOSIMS, SAMPLES SMALLER THAN 50-100 NM ARE DIFFICULT TO ANALYZE DUE TO LIMITATIONS IN SPATIAL RESOLUTION AND SENSITIVITY. TO ADDRESS THIS ISSUE WE DEVELOPED METHODS TO APPLY APT TO EXTRATERRESTRIAL SAMPLES. THE NEAR ATOMIC-RESOLUTION AND HIGH SENSITIVITY MAKES APT THE IDEAL TECHNIQUE TO ANALYZE THE ELEMENTAL AND ISOTOPIC COMPOSITIONS OF SAMPLES THAT ARE TOO SMALL FOR THE NANOSIMS (<50 NM). WE SUCCESSFULLY PERFORMED APT OF METEORITIC NANODIAMONDS, A LUNAR DUST GRAIN, AN IRON METEORITE, AND QUANTIFIED INSTRUMENTAL BIAS. WE CAN NOW RELIABLY ANALYZE WITH APT SMALL SAMPLES, INCL. PRESOLAR NANOGRAINS THE GOAL OF OUR PROPOSED INVESTIGATION (TASK 1). COMPARED TO NANOSIMS THE TOMOGRAPHIC APPROACH OF APT PROVIDES AN UNDILUTED SAMPLE ANALYSIS WITHOUT CONTRIBUTIONS FROM THE UNDERLYING SUBSTRATE OR SURROUNDING MATRIX. THE OBJECTIVE OF THIS TASK IS TO PERFORM APT ON PRESOLAR NANO-OXIDES AND NANODIAMONDS TO OBTAIN ELEMENTAL AND ISOTOPE DATA TO PROVIDE NEW INSIGHTS INTO STELLAR ORIGINS, FORMATION PROCESSES, AND POSSIBLY ALTERATION IN THE EARLY SOLAR SYSTEM. TASK 2: THE KNOWLEDGE OF THE TIME SPAN BETWEEN THE FORMATION OF PSG AND THEIR INCORPORATION INTO FORMING PLANETESIMALS IS STILL LIMITED. WE HAVE SUCCESSFULLY MEASURED COSMOGENIC HE AND NE IN LARGE PRESOLAR SIC GRAINS, APPLIED NUCLEAR RECOIL LOSS CORRECTIONS, AND CALCULATED PRESOLAR COSMIC-RAY EXPOSURE AGES USING PRESOLAR PRODUCTION RATES OF COSMOGENIC NUCLIDES. SO FAR, A TOTAL OF ONLY 40 PSG HAVE BEEN DATED. MOST GRAINS HAD PRESOLAR AGES<300 MA AND ONLY A FEW HAD HIGHER AGES UP TO ~2 GA. THE KNOWLEDGE OF THE PRODUCTION RATES IN THE INTERSTELLAR MEDIUM IS ONE OF THE MOST CRITICAL ELEMENTS IN THE CALCULATION OF PRESOLAR EXPOSURE AGES. SINCE OUR LAST PUBLICATION MORE REALISTIC PRODUCTION RATES HAVE BEEN DEVELOPED. FOR THE FIRST TIME, THESE RATES USE THE GALACTIC COSMIC-RAY SPECTRUM AS OBSERVED OUTSIDE THE HELIOSPHERE BY VOYAGER. WE PROPOSE TO MEASURE PRESOLAR COSMOGENIC NUCLIDES OF HE, NE AND LI IN LARGE PRESOLAR SIC. WE WILL USE OUR NEW DATA TO TEST THE HYPOTHESIS THAT THE DOMINANCE OF YOUNG PRESOLAR AGES IS A CONSEQUENCE OF A STARBURST EVENT AND TO EXPLORE THE PRESOLAR CHRONOLOGY OF THE STARTING MATERIAL OF OUR SOLAR SYSTEM. WHILE OUR METHOD HAS LARGE UNCERTAINTIES COMPARED TO RADIOMETRIC CHRONOMETERS, IT IS CURRENTLY THE ONLY METHOD THAT PROVIDES AGES OF PSG, THE OLDEST MATERIAL AVAILABLE FOR STUDY IN THE SOLAR SYSTEM. | FIELD MUSEUM OF NATURAL HISTORY | $499,518 | NATIONAL AERONAUTICS AND SPACE ADMINISTRATION | NATIONAL AERONAUTICS AND SPACE ADMINISTRATION | — | — | AR21 | Mar 20, 2019 | Feb 17, 2019 | Feb 16, 2024 | ||
| CREATION OF THREE BRAIN SCOOP EPISODES WITH FIELD MUSEUM | FIELD MUSEUM OF NATURAL HISTORY | $24,506 | SMITHSONIAN INSTITUTION | SMITHSONIAN INSTITUTION | — | 512110Motion Picture and Video Production | T006PHOTO/MAP/PRINT/PUBLICATION- FILM/VIDEO TAPE PRODUCTION | Sep 10, 2018 | Sep 10, 2018 | Aug 10, 2020 | ||
| IGF::OT::IGF SMALL TOOTH SAWFISH GENETIC ANALYSIS | FIELD MUSEUM OF NATURAL HISTORY | $5,000 | NATIONAL OCEANIC AND ATMOSPHERIC ADMINISTRATION | NATIONAL OCEANIC AND ATMOSPHERIC ADMINISTRATION | — | 541990All Other Professional, Scientific, and Technical Services | B516SPECIAL STUDIES/ANALYSIS- ANIMAL/FISHERIES | Sep 12, 2016 | Sep 12, 2016 | Sep 29, 2017 | ||
| WE PROPOSE TO STUDY THE ELEMENTAL AND ISOTOPIC COMPOSITION OF THE OLDEST MATERIAL IN THE SOLAR SYSTEM, PRESOLAR GRAINS AND METEORITIC NANODIAMONDS, TO IMPROVE OUR UNDERSTANDING OF THE ORIGIN OF OUR SOLAR SYSTEM. OUR FIRST GOAL IS TO START TO ESTABLISH A PRESOLAR CHRONOLOGY BY DETERMINING INTERSTELLAR RESIDENCE TIMES OF LARGE PRESOLAR SILICON CARBIDE (SIC) GRAINS BY PRESOLAR COSMIC-RAY EXPOSURE AGE DATING WITH NOBLE GAS MASS SPECTROMETRY AND SECONDARY ION MASS SPECTROMETRY (NANOSIMS) (TASK 1). AGES FROM PRESOLAR GRAIN HAVE THE POTENTIAL TO PROVIDE CRUCIAL INFORMATION TOWARDS A BETTER UNDERSTANDING OF PROCESSES IN THE INTERSTELLAR MEDIUM AND THE LATE EVOLUTION OF OUR GALAXY. OUR SECOND GOAL IS TO FULLY ESTABLISH ATOM-PROBE TOMOGRAPHY (APT) IN ISOTOPE COSMOCHEMISTRY BY CORRECTING FOR REMAINING TECHNICAL BIASES. THIS BUILDS ONTO OUR PIONEERING EFFORT IN DEVELOPING APT FOR COSMOCHEMISTRY THAT WE STARTED FOUR YEARS AGO. OUR IMMEDIATE SCIENTIFIC OBJECTIVE IS TO HELP ANSWERING THE 26-YEAR-OLD QUESTION OF THE ORIGIN OF METEORITIC NANODIAMONDS THROUGH ANALYSES OF THE CARBON ISOTOPIC COMPOSITION OF SINGLE GRAINS (TASK 2). APT IS THE ONLY TECHNIQUE WITH THE REQUIRED SPATIAL RESOLUTION AND SENSITIVITY TO ANALYZE CARBON ISOTOPES IN INDIVIDUAL NANODIAMONDS. IN ADDITION, WE WILL APPLY APT TO THE ANALYSIS OF OTHER TYPES OF PRESOLAR GRAINS, SPECIFICALLY PRESOLAR CR-ANOMALOUS NANO-OXIDES (TASK 3). THESE SAMPLES ARE TOO SMALL FOR CLEAN, UNMIXED ISOTOPE ANALYSIS WITH OTHER TECHNIQUES SUCH AS NANOSIMS. APT OF SUCH NANO-OXIDES HAS THE POTENTIAL TO PROVIDE NEW INFORMATION ON THE NUCLEOSYNTHETIC SOURCES AND THE EARLY SOLAR SYSTEM. APT HAS THE POTENTIAL TO LAUNCH THE FIELD OF ISOTOPE COSMOCHEMISTRY INTO PREVIOUSLY UNEXPLORED TERRITORY WITH IN IMPROVEMENT OF SPATIAL RESOLUTION OF ABOUT TWO ORDERS OF MAGNITUDE COMPARED TO NANOSIMS. | FIELD MUSEUM OF NATURAL HISTORY | $213,688 | NATIONAL AERONAUTICS AND SPACE ADMINISTRATION | NATIONAL AERONAUTICS AND SPACE ADMINISTRATION | — | — | AR21 | Dec 9, 2014 | Jan 1, 2015 | May 9, 2019 | ||
| IGF::OT::IGF WILDLIFE SAMPLING PROJECT | FIELD MUSEUM OF NATURAL HISTORY | $149,955 | CENTERS FOR DISEASE CONTROL AND PREVENTION | CENTERS FOR DISEASE CONTROL AND PREVENTION | — | 712110Museums | B516SPECIAL STUDIES/ANALYSIS- ANIMAL/FISHERIES | Aug 24, 2012 | Aug 24, 2012 | Sep 19, 2013 | ||
| WILDLIFE SAMPLING PROJECT | FIELD MUSEUM OF NATURAL HISTORY | $158,000 | CENTERS FOR DISEASE CONTROL AND PREVENTION | CENTERS FOR DISEASE CONTROL AND PREVENTION | — | 712110Museums | R499SUPPORT- PROFESSIONAL: OTHER | Sep 19, 2011 | Sep 19, 2011 | Sep 19, 2012 | ||
| WORKSHOP ON CAREX AND CONUS | FIELD MUSEUM OF NATURAL HISTORY | $40,000 | SMITHSONIAN INSTITUTION | SMITHSONIAN INSTITUTION | — | 712110Museums | U099EDUCATION/TRAINING- OTHER | Jul 20, 2011 | Jul 20, 2011 | Oct 30, 2011 | ||
| WE PROPOSE TO STUDY THE ELEMENTAL AND ISOTOPIC COMPOSITIONS OF SOLID SAMPLES OF STARS, PRESOLAR GRAINS, AND NANODIAMONDS THAT HAVE BEEN EXTRACTED FROM METEORITES TO UNDERSTAND THEIR ORIGINS. THE PROPOSED RESEARCH IS STRUCTURED INTO THREE RELATED SUBTASKS: 1) ATOM-PROBE ANALYSES OF METEORITIC NANODIAMONDS AND PRESOLAR SILICON CARBIDE (SIC): OUR GOAL IS TO ANSWER THE FUNDAMENTAL QUESTIONS OF THE ENIGMATIC ORIGIN (STELLAR VS. SOLAR SYSTEM) OF METEORITIC NANODIAMONDS, ASSOCIATED CARBONACEOUS PHASES AND OF THE FORMATION HISTORY OF PRESOLAR SUBGRAINS. THE RESOLUTION OF THE NANOSIMS ION MICROPROBE IS NOT SUFFICIENT TO ANALYZE THE ISOTOPIC COMPOSITIONS OF SMALL SUBGRAINS WITHIN PRESOLAR GRAINS AND OF INDIVIDUAL METEORITIC NANODIAMONDS (AVG. DIAM. ~3 NM). THEREFORE, THESE MINERALS ARE AMONG THE LEAST UNDERSTOOD REFRACTORY PHASES IN METEORITES. THE KNOWLEDGE OF ISOTOPIC COMPOSITIONS OF SUBGRAINS IS ESSENTIAL FOR A BETTER UNDERSTANDING OF THE ORIGIN AND FORMATION OF PRESOLAR DUST. ANALYSES OF C ISOTOPES OF INDIVIDUAL NANODIAMONDS ARE REQUIRED TO DETERMINE THEIR PRESOLAR FRACTION AND THEIR STELLAR SOURCES. WE PROPOSE TO TAKE ADVANTAGE OF THE ATOMIC RESOLUTION OF THE ATOM PROBE TOMOGRAPH (APT) TO ANALYZE THE ELEMENTAL AND ISOTOPIC COMPOSITIONS OF INDIVIDUAL METEORITIC NANODIAMONDS, ASSOCIATED PHASES AND PRESOLAR SUBGRAINS. WE RECENTLY PRESENTED FIRST SUCCESSFUL APT ANALYSES OF PRESOLAR SIC, AND PRELIMINARY DATA OF SAMPLES WITH NANODIAMONDS. APTS INCREASE THE SPATIAL RESOLUTION FOR ISOTOPE ANALYSES IN COSMOCHEMISTRY BY TWO ORDERS OF MAGNITUDE. 2) INTERSTELLAR RESIDENCE TIMES OF PRESOLAR GRAINS: THE TIME SPAN BETWEEN THE FORMATION OF PRESOLAR GRAINS IN STELLAR OUTFLOWS AND THEIR INCORPORATION INTO EARLY SOLAR-SYSTEM SOLIDS IS CRUCIAL FOR A BETTER UNDERSTANDING OF THE STAR FORMATION HISTORY IN OUR GALAXY, PROCESSING OF SOLAR SYSTEM PRECURSOR MATERIAL IN THE INTERSTELLAR MEDIUM AND FORMATION PROCESSES OF THE SOLAR SYSTEM. RECENTLY, WE REPORTED PRESOLAR COSMIC-RAY EXPOSURE AGES OF TWENTY LARGE PRESOLAR MAINSTREAM SIC GRAINS. MOST GRAINS HAVE PRESOLAR AGES CONSIDERABLY SHORTER THAN THEORETICAL ESTIMATES OF THEIR LIFETIMES. THE AGE DISTRIBUTION MAY BE EXPLAINED BY STARBURST ACTIVITY 1-2 BILLION YEARS PRIOR TO THE BIRTH OF THE SUN, POSSIBLY DUE TO A GALACTIC MERGER. HERE, WE PROPOSE TO TEST THE PRESOLAR STARBURST HYPOTHESIS BY DETERMINING INTERSTELLAR RESIDENCE TIMES OF A LARGER NUMBER OF LARGE PRESOLAR SIC GRAINS. TO DETERMINE CONCENTRATIONS OF COSMOGENIC NE, HE AND LI WE INTEND TO USE THE WELL-ESTABLISHED TECHNIQUES NOBLE GAS MASS SPECTROMETRY AND NANOSIMS. 3) NUCLEOSYNTHETIC ISOTOPES IN PRESOLAR GRAINS: NUCLEOSYNTHETIC ISOTOPES MEASURED IN INDIVIDUAL PRESOLAR GRAINS PROVIDE INFORMATION ON THE TYPE OF STELLAR SOURCES, ON NUCLEOSYNTHETIC REACTIONS, STELLAR MIXING AND ION-TRAPPING PROCESSES IN OUR PARENT STARS. THE NUCLEOSYNTHETIC COMPONENT ALSO NEEDS TO BE KNOWN TO CALCULATE COSMOGENIC COMPONENT TO DETERMINE EXPOSURE AGES. HERE, WE PROPOSE TO ANALYZE NUCLEOSYNTHETIC ISOTOPES IN INDIVIDUAL PRESOLAR GRAINS OF DIFFERENT TYPES AND FROM DIFFERENT PRIMITIVE METEORITES IN A COORDINATED MULTI-INSTRUMENT STUDY TO ANSWER THESE QUESTIONS. THIS INVOLVES RELIABLE ANALYTICAL TECHNIQUES INCLUDING TIME-OF-FLIGHT SECONDARY ION MASS SPECTROMETRY, NANOSIMS, NOBLE GAS SPECTROMETRY AND RESONANCE IONIZATION MASS SPECTROMETRY. THE PROPOSED SAMPLE-FOCUSED RESEARCH WILL INCREASE OUR UNDERSTANDING OF THE CHEMICAL ORIGIN OF THE SOLAR SYSTEM AND WILL CONTRIBUTE TO THE DEVELOPMENT OF FUTURE MISSIONS, IN PARTICULAR SAMPLE RETURN MISSION TO PRIMITIVE SOLAR SYSTEM OBJECTS. THIS IS HIGHLY SIGNIFICANT TO NASA'S COSMOCHEMISTRY PROGRAM GOALS, THE PLANETARY SCIENCE RESEARCH PROGRAM, NASA'S RESEARCH OBJECTIVES AND STRATEGIC GOAL OUTLINED IN THE SUMMARY OF THE SCIENCE PLAN 2007 FOR NASA'S SCIENCE MISSION DIRECTORATE 2007-2016 AND TO ONE OF THE PRINCIPAL GOALS OF NASA'S VISION FOR SCIENCE, TO UNDERSTAND OUR ORIGINS. | FIELD MUSEUM OF NATURAL HISTORY | $176,000 | NATIONAL AERONAUTICS AND SPACE ADMINISTRATION | NATIONAL AERONAUTICS AND SPACE ADMINISTRATION | — | — | AR21 | May 3, 2011 | Mar 24, 2011 | Mar 23, 2015 | ||
| INVESTIGATE LARGETOOTH SAWFISH | FIELD MUSEUM OF NATURAL HISTORY | $25,000 | NATIONAL OCEANIC AND ATMOSPHERIC ADMINISTRATION | NATIONAL OCEANIC AND ATMOSPHERIC ADMINISTRATION | — | 541990All Other Professional, Scientific, and Technical Services | R499SUPPORT- PROFESSIONAL: OTHER | Sep 1, 2010 | Sep 1, 2010 | Apr 1, 2011 | ||
| SAWFISH RESEARCH | FIELD MUSEUM OF NATURAL HISTORY | $7,800 | NATIONAL OCEANIC AND ATMOSPHERIC ADMINISTRATION | NATIONAL OCEANIC AND ATMOSPHERIC ADMINISTRATION | — | 712110Museums | R499SUPPORT- PROFESSIONAL: OTHER | Sep 2, 2008 | Sep 2, 2008 | Dec 1, 2009 | ||
| EMPLOYEE DON'T HAVE CREDIT CARD FOR THIS ACCOUNT. | FIELD MUSEUM OF NATURAL HISTORY | $369 | VETERANS AFFAIRS, DEPARTMENT OF | — | — | — | 9999MISCELLANEOUS ITEMS | Mar 25, 2008 | Mar 25, 2008 | Apr 4, 2008 | ||
| TICKETS WAS PURCHASE FOR VETERAN FROM DAY TX CENTE | FIELD MUSEUM OF NATURAL HISTORY | $497 | VETERANS AFFAIRS, DEPARTMENT OF | — | — | — | G004SOCIAL- SOCIAL REHABILITATION | Aug 23, 2006 | Aug 23, 2006 | Aug 25, 2006 | ||
| FIELD MUSEUM OF NATURAL HISTORY/ EXHIBIT | FIELD MUSEUM OF NATURAL HISTORY | $100,000 | DEPT OF THE ARMY | DEPT OF THE ARMY | — | 712110Museums | R499SUPPORT- PROFESSIONAL: OTHER | Aug 11, 2006 | Aug 11, 2006 | Sep 16, 2007 | ||
| CHANGE ADMINISTRATION AS IN BLK. 6 AND 15 | FIELD MUSEUM OF NATURAL HISTORY | $0 | NATIONAL AERONAUTICS AND SPACE ADMINISTRATION | — | — | — | AG41ENERGY R&D SERVICES; ENERGY INFORMATION, POLICY AND REGULATION; BASIC RESEARCH | Apr 4, 2006 | Apr 4, 2006 | Sep 30, 2008 | ||
| EARLY SOLAR SYSTEM PROCESSES AND TIME SCALES FROM ISOTOPIC INVESTIGATIONS OF METEORITES. | FIELD MUSEUM OF NATURAL HISTORY | $0 | NATIONAL AERONAUTICS AND SPACE ADMINISTRATION | — | — | — | AR21 | Mar 13, 2006 | Mar 1, 2006 | Feb 28, 2009 | ||
| REPORT ON PEREGRINE FALCON TERRIT. | FIELD MUSEUM OF NATURAL HISTORY | $1,250 | US FISH AND WILDLIFE SERVICE | — | — | 712110Museums | B534SPECIAL STUDIES/ANALYSIS- WILDLIFE | Sep 14, 2005 | Sep 14, 2005 | Aug 15, 2006 | ||
| GEOCHEMICAL & ISOTOPIC INVESTIGATIONS OF METERORITES | FIELD MUSEUM OF NATURAL HISTORY | $147,537 | NATIONAL AERONAUTICS AND SPACE ADMINISTRATION | — | — | — | AR21 | Mar 22, 2005 | Mar 1, 2005 | Apr 30, 2008 | ||
| GEOCHEMICAL AND ISOTOPIC INVESTIGATIONS OF METEORI TES | FIELD MUSEUM OF NATURAL HISTORY | $345,000 | NATIONAL AERONAUTICS AND SPACE ADMINISTRATION | — | — | — | AR21 | Apr 29, 2002 | Oct 1, 2003 | Apr 30, 2005 | ||
| A PROPOSAL FOR EARTH SCIENCES RESEARCH AT THE FIELD MUSEUM | FIELD MUSEUM OF NATURAL HISTORY | $249,989 | NATIONAL AERONAUTICS AND SPACE ADMINISTRATION | — | — | — | AR21 | Sep 21, 2001 | Sep 21, 2001 | Sep 14, 2004 | ||
| THE FIELD MUSEUM'S K-8 ENVIRONMENTAL EDUCATION INI TIATIVE: LOCAL & GLOBAL STUDIES ON EARTH SCIE | FIELD MUSEUM OF NATURAL HISTORY | $915,000 | NATIONAL AERONAUTICS AND SPACE ADMINISTRATION | — | — | — | AR21 | Jun 21, 2000 | Jun 21, 2000 | Nov 30, 2003 | ||
| — | FIELD MUSEUM OF NATURAL HISTORY | $0 | NATIONAL BIOLOGICAL SURVEY | — | — | — | R702SUPPORT- MANAGEMENT: DATA COLLECTION | Sep 15, 1995 | Sep 15, 1995 | Sep 15, 1997 |