• ⌘ + K
  • Home
  • 0
    Inbox
Explore
  • Browse All
  • Health
  • FedCiv
  • Defense
  • Events
Work
  • Teaming Hub
  • Watchlists
  • Bookmarks
  • Notes
Research
  • Grants
    • Contracts
    • Vehicles
    • OTAs
    • OTIDVs
    • DLA DIBBS
    • SBIR/STTR
  • Agencies
  • NAICS
  • PSC
  • DOGE Tracker

Federal Contract Awards

17awards

Analyze awards, watch incumbents and competitors, track new transactions or changes, and use award history to shape recompete and capture strategy.

Awardee
is
MRGUP99ZAZ59
Award ID
Description
Recipient
Total Value
Awarding Agency
Funding Agency
Set Aside
NAICS
PSC
Award Date
Start Date
End Date
80NSSC24K1000
EARMARK, ESTABLISHING S-BAND LUNAR TRACKING SUPPORT CAPABILITIESMOREHEAD STATE UNIVERSITY$9,953,000NATIONAL AERONAUTICS AND SPACE ADMINISTRATIONNATIONAL AERONAUTICS AND SPACE ADMINISTRATION——AJ11GENERAL SCIENCE AND TECHNOLOGY R&D SERVICES; GENERAL SCIENCE AND TECHNOLOGY; BASIC RESEARCHSep 17, 2024Aug 1, 2024Sep 30, 2026
80NSSC22P0183
GROUND TESTING SUPPORT FOR LUNAR NODE-1MOREHEAD STATE UNIVERSITY$37,863NATIONAL AERONAUTICS AND SPACE ADMINISTRATIONNATIONAL AERONAUTICS AND SPACE ADMINISTRATION—611310Colleges, Universities, and Professional SchoolsAR11SPACE R&D SERVICES; SPACE FLIGHT, RESEARCH AND SUPPORTING ACTIVITIES; BASIC RESEARCHNov 17, 2021Nov 17, 2021Nov 30, 2023
80NSSC20K0824
WE PROPOSE A 100KS OBSERVATION OF THE UNIQUE OUTBURSTING SEYFERT GALAXY IC 3599, TO BE TRIGGERED IF IT FLARES AGAIN IN 2019.MOREHEAD STATE UNIVERSITY$0NATIONAL AERONAUTICS AND SPACE ADMINISTRATIONNATIONAL AERONAUTICS AND SPACE ADMINISTRATION——AR21Apr 6, 2020Mar 9, 2020Oct 14, 2021
80NSSC19K0742
THE GOAL OF THIS PROPOSAL IS TO OBTAIN THE UNDERLYING XRAY SPECTRUM OF THE X-RAY TRANSIENT NARROW LINE SEYFERT 1 GALAXY WPVS 007 DURING ONE OF ITS RARE X-RAY HIGH STATES. WHILE WPVS 007 IS TYPICALLY IN EXTREMELY LOW XRAY FLUX STATES WHICH ARE CAUSED PRIMARILY BY ABSORPTION, IT HAS SHOWN EPISODES OF VERY VIOLENT X-RAY ACTIVITY. IN ORDER TO UNDERSTAND THE REAL NATURE OF THE X-RAY ABSORBER, A GOOD KNOWLEDGE OF THE UNDERLYING X-RAY SPECTRUM IS CRUCIAL. THIS, HOWEVER, CAN ONLY BE DONE WHEN IT IS IN A HIGH STATE. WE THEREFORE PROPOSE A 35 KS TRIGGERED OBSERVATION OFWPVS 007 (INCLUDES THE 40% OVERHEAD FOR BACKGROUND FLARES)MOREHEAD STATE UNIVERSITY$0NATIONAL AERONAUTICS AND SPACE ADMINISTRATIONNATIONAL AERONAUTICS AND SPACE ADMINISTRATION——AR21May 7, 2019Mar 25, 2019Jul 27, 2020
80NSSC17K0665
THE PRISM CUBESAT MISSION WILL DETERMINE THE ORIGIN OF PHOBOS: DID IT FORM IN THE OUTER SOLAR SYSTEM OR IN SITU NEAR MARS, PERHAPS THROUGH A COLLISION OR BY COALESCENCE OF A DEBRIS DISK LEFT OVER FROM THE FORMATION OF MARS? PRISM WILL MEASURE PHOBOS' SURFACE COMPOSITION USING SECONDARY ION MASS SPECTROMETRY OR SIMS AND ANSWER THIS CRITICAL QUESTION. THE PRISM CUBESAT STUDY SUPPORTS THE GOALS OF THE PLANETARY SCIENCE DIVISION AS DESCRIBED IN THE 2014 NASA SCIENCE PLAN BECAUSE IT ADDRESSES THE QUESTION "HOW DID THE SOLAR SYSTEM FORM AND EVOLVE?" BY "EXPLORING AND OBSERVING THE OBJECTS IN THE SOLAR SYSTEM TO UNDERSTAND HOW THEY FORMED AND EVOLVED." PRISM, A 12U CUBESAT WILL DETERMINE THE COMPOSITION AND HENCE THE ORIGIN OF PHOBOS USING A HIGH RESOLUTION TIME-OF-FLIGHT (TOF) ION COMPOSI ION SPECTROMETER OF APPROXIMATELY 2U VOLUME TO OBSERVE THE SPECIES SPUTTERED FROM PHOBOS SURFACE - WITHOUT LANDING ON THE SURFACE.MOREHEAD STATE UNIVERSITY$99,998NATIONAL AERONAUTICS AND SPACE ADMINISTRATIONNATIONAL AERONAUTICS AND SPACE ADMINISTRATION——AR21Sep 13, 2017Aug 31, 2017Feb 28, 2018
80NSSC17K0237
THE BI-SAT OBSERVATIONS OF THE LUNAR ATMOSPHERE ABOVE SWIRLS (BOLAS) CONCEPT IS FOR A TETHERED CUBESAT MISSION CAPABLE OF MAKING REPEATED MEASUREMENTS AT LOW ALTITUDES ABOVE THE MOON REQUIRED IN ORDER TO UNDERSTAND VITAL ASPECTS OF THE LUNAR HYDROGEN CYCLE AND SPACE WEATHERING. OBTAINING OBSERVATIONS CLOSE TO THE LUNAR SURFACE IS EXTREMELY DIFFICULT DUE TO THE PRESENCE OF "MASCONS", WHICH MAKE ORBITING AT LOW ALTITUDES VERY UNSTABLE. AT PRESENT, ACQUIRING REPEATED MEASUREMENTS FROM VERY LOW ALTITUDES REQUIRES A LARGE SPACECRAFT WITH THE SIGNIFICANT AMOUNT OF FUEL (MASS) NECESSARY TO MAINTAIN ITS ORBIT. THE MOST GROUND-BREAKING ASPECT OF THE BOLAS CONCEPT IS THE USE OF TWO CUBESATS CONNECTED BY A TETHER MANY TENS OF KILOMETERS IN LENGTH, WHICH CAN BE USED TO MAKE SIMULTANEOUS HIGH AND LOW ALTITUDE MEASUREMENTS ABOVE THE SAME LOCATION ON THE MOON. CRUCIALLY, THE CENTER-OF-MASS OF THE TETHERED SPACECRAFT IS AT AN ALTITUDE WHERE THE ORBIT IS RELATIVELY STABLE AND SIGNIFICANTLY LESS PROPULSIVE MANEUVERING IS REQUIRED. THIS INNOVATION WILL ENABLE SMALLSAT MISSIONS TO MAKE IN SITU AND REMOTE SENSING MEASUREMENTS FROM LOW ALTITUDES THAT ARE CRITICAL TO ADDRESSING MANY COMPELLING QUESTIONS IN PLANETARY SCIENCE. THE BOLAS MISSION WILL FOCUS ON INVESTIGATING THE HYDROGEN CYCLE AND SPACE WEATHERING AT THE MOON, BY DETERMINING: (I) THE MECHANISMS AND DYNAMICS OF LUNAR HYDROGEN IMPLANTATION, AND THEIR DEPENDENCE ON SURFACE COMPOSITION, REGOLITH PROPERTIES, LOCAL TOPOGRAPHY, PLASMA CONDITIONS, TIME-OF-DAY, AND CRUSTAL MAGNETIC FIELDS; AND (II) HOW THIS RELATES TO THE FORMATION OF LUNAR SWIRLS , SPACE WEATHERING PROCESSES AND THE EVOLUTION OF AIRLESS BODIES. THESE SCIENCE OBJECTIVES ARE EXTREMELY TIMELY AND HIGHLY RELEVANT TO THE 2014 NASA SCIENCE PLAN, IN PARTICULAR TO THE QUESTION OF HOW THE SOLAR SYSTEM HAS FORMED AND EVOLVED, AND WILL PRODUCE HIGH IMPACT SCIENCE. FOR THE NECESSARY NEUTRALS, FIELDS AND PLASMA MEASUREMENTS, THE PRELIMINARY SCIENCE PAYLOAD CONSISTS OF AN ION SPECTROMETER, ENERGETIC NEUTRAL ATOM IMAGER, PLASMA WAVE SYSTEM, AND MAGNETOMETER. SIGNIFICANT DEVELOPMENT HAS ALREADY BEEN INVESTED IN MINIATURIZING THESE INSTRUMENTS FOR A CUBESAT PLATFORM. THE INSTRUMENTS WILL BE MOUNTED ON BOTH OF THE TETHERED CUBESATS IN ORDER THAT HIGH AND LOW ALTITUDE MEASUREMENTS CAN BE COMPARED. THIS WOULD BE ESPECIALLY IMPORTANT WHEN FLYING ABOVE A CRUSTAL MAGNETIC FIELD, AS IT WOULD PROVIDE CRUCIAL MEASUREMENTS RELATING TO THE FORCING FROM THE INCOMING SOLAR WIND AND THE RESPONSE OF THE PLASMA, FIELDS, AND NEUTRALS WITHIN THE "MINI-MAGNETOSPHERE". THIS WOULD THEN BE USED TO UNDERSTAND THE HYDROXYLATION, HYDRATION AND SPACE WEATHERING PROCESSES IN THESE REGIONS AND THEIR ROLE IN FORMING THE ENIGMATIC "SWIRL" PATTERNS ON THE LUNAR SURFACE. THE BOLAS CONCEPT STUDY TEAM CONSISTS OF A SMALL, EXPERT LUNAR SCIENCE AND INSTRUMENTATION TEAM AT GSFC; SPECIALISTS IN DESIGNING, INTEGRATING AND BUILDING CUBESATS AT MOREHEAD STATE UNIVERSITY (MSU); EXPERTS IN CUBESAT PROPULSION SYSTEMS AT BUSEK CO. INC.; PIONEERS IN SPACE TETHER SYSTEMS AT TETHERS UNLIMITED, INC.; AS WELL AS WORLD CLASS GSFC ENGINEERS TO PROVIDE THERMAL MANAGEMENT, ATTITUDE DETERMINATION AND CONTROL, AND FLIGHT DYNAMICS SOLUTIONS. A MAJOR TASK IN THE CONCEPT STUDY WILL BE ADDRESSING THE FEASIBILITY AND LIMITATIONS OF A TETHERED SMALLSAT, SUCH AS TETHER DEPLOYMENT (RETRACTION), STABILITY (ORBITAL CONFIGURATIONS), LIFETIME, ALTITUDE RANGE, AND ABILITY TO TARGET REGIONS-OF-INTEREST. THIS WILL INVOLVE TRADES BETWEEN TETHER LENGTH, MASS, AND DEPLOY-ABILITY, AS WELL AS SPACECRAFT SIZE, CONFIGURATION AND SCIENCE CAPABILITY. THE DEVELOPMENT OF THE BOLAS CONCEPT PROMISES TO SIGNIFICANTLY ENHANCE THE ABILITY OF SMALLSAT MISSIONS TO ACHIEVE CUTTING EDGE PLANETARY SCIENCE.MOREHEAD STATE UNIVERSITY$99,998NATIONAL AERONAUTICS AND SPACE ADMINISTRATIONNATIONAL AERONAUTICS AND SPACE ADMINISTRATION——AR21Jul 26, 2017Jul 10, 2017Feb 28, 2018
W912KZ17P0050
IGF::OT::IGF MOREHEAD STATE UNIVERSITY ADVERTISINGMOREHEAD STATE UNIVERSITY$5,000DEPT OF THE ARMYDEPT OF THE ARMY—541890Other Services Related to AdvertisingR701SUPPORT- MANAGEMENT: ADVERTISINGJun 13, 2017Jun 13, 2017May 31, 2018
NNX17AC39G
THE GOAL OF THIS PROPOSAL IS TO OBTAIN THE UNDERLYING X RAY SPECTRUM OF THE X RAY TRANSIENT NARROW LINE SEYFERT 1 GALAXY WPVS 007 DURING ONE OF ITS RARE X RAY HIGH STATES. WHILE WPVS 007 IS TYPICALLY IN EXTREMELY LOW X RAY FLUX STATES WHICH ARE CAUSED PRIMARILY BY ABSORPTION, IT HAS SHOWN EPISODES OF VERY VIOLENT X RAY ACTIVITY. IN ORDER TO UNDERSTAND THE REAL NATURE OF THE X RAY ABSORBER, A GOOD KNOWLEDGE OF THE UNDERLYING X RAY SPECTRUM IS CRUCIAL. THIS, HOWEVER, CAN ONLY BE DONE WHEN IT IS IN A HIGH STATE. WE THEREFORE PROPOSE A 35 KS TRIGGERED OBSERVATION OF WPVS 007 INCLUDES THE 40 OVERHEAD FOR BACKGROUND FLARESMOREHEAD STATE UNIVERSITY$0NATIONAL AERONAUTICS AND SPACE ADMINISTRATIONNATIONAL AERONAUTICS AND SPACE ADMINISTRATION——AR21Dec 16, 2016Nov 21, 2016Nov 20, 2017
ING16PX00609
PALYNOLOGY ANALYSIS SERVICES ON 23 SAMPLES; ''IGF::OT::IGF''MOREHEAD STATE UNIVERSITY$4,950US GEOLOGICAL SURVEYUS GEOLOGICAL SURVEY—541380Testing Laboratories and ServicesB517SPECIAL STUDIES/ANALYSIS- GEOLOGICALApr 6, 2016Apr 6, 2016Mar 31, 2017
NNH16CO86C
IGF::OT::IGF NASA BAA AWARD THIS IS AN AWARD UNDER THE NEXT SPACE TECHNOLOGIES FOR EXPLORATION PARTNERSHIPS (NEXTSTEP) BROAD AGENCY ANNOUNCEMENT (BAA). THE ULTIMATE GOAL OF THIS PROGRAM IS TO UNDERTAKE A MISSION TO THE MOON DURING EM-1 OR SIMILAR MISSION TO EARTH ESCAPE, THAT WILL ADDRESS SKGS ASSOCIATED WITH THE NATURE, LOCATION AND TRANSPORTATION PHYSICS OF LUNAR VOLATILES, AND TO DEMONSTRATE AN INNOVATIVE, HIGHLY CAPABLE RF ION PROPULSION SYSTEM AND 6U SPACECRAFT BUS. THE MISSION WILL REQUIRE PIONEERING APPROACH TO POWER GENERATION AND INNOVATIVE, LOW-COST APPROACHES TO THE DEVELOPMENT AND USE OF RADIATION-TOLERANT SYSTEMS TO MEET THE MISSION REQUIREMENTS. THE PROGRAM CAN BE CATEGORIZED GENERALLY INTO THREE PHASES: 1) DEVELOPMENT, 2) INTEGRATION AND TESTING, AND 3) MISSION OPERATIONS. SMALL SATELLITE MISSIONS ADDRESSING STRATEGIC KNOWLEDGE GAPS (SKG) WAS IDENTIFIED AS A KEY LONG TERM CAPABILITY AREA THAT COULD POTENTIALLY SIGNIFICANTLY BENEFIT FUTURE HUMAN SPACE EXPLORATION AND IN ADDITION ADDRESS COMMERCIAL INTERESTS SUCH AS IN-SITU RESOURCE PROSPECTING. MORE SPECIFICALLY, NASA ANTICIPATES MAKING LAUNCH OPPORTUNITIES FOR A LIMITED NUMBER OF SMALL SATELLITES AVAILABLE ON SPACE LAUNCH SYSTEM (SLS) AND OTHER BEYOND EARTH ORBIT MISSIONS. THIS BAA THRUST AREA INTENDS TO PROVIDE INTEGRATION AND LAUNCH OPPORTUNITIES FOR 6U CUBESAT PAYLOADS AS SECONDARY PAYLOADS ON DEEP SPACE MISSIONS. A CUBESAT IS A TYPE OF SPACE RESEARCH NANOSATELLITE. CUBESATS SUPPORTED BY THIS LAUNCH INITIATIVE INCLUDE ONLY 6U FORM FACTORS. CUBESATS OF TYPICALLY HAVE A MASS OF 1.33 KILOGRAMS PER 1U CUBE. A 6U CUBESAT TYPICALLY HAS A MASS OF 12 KG. THE MAXIMUM MASS COMPATIBLE WITH THE EM-1 DISPENSER IS 14 KG.MOREHEAD STATE UNIVERSITY$7,351,516NATIONAL AERONAUTICS AND SPACE ADMINISTRATIONNATIONAL AERONAUTICS AND SPACE ADMINISTRATION—541712AR21Nov 5, 2015Nov 5, 2015Dec 20, 2024
W912KZ14P0050
LIIFE AFTER HIGH SCHOOLMOREHEAD STATE UNIVERSITY$6,746DEPT OF THE ARMYDEPT OF THE ARMY—611310Colleges, Universities, and Professional SchoolsM1CAOPERATION OF SCHOOLSJun 18, 2014Jun 18, 2014Jun 24, 2014
NNG14WQ19P
IGF::OT::IGF IMPLEMENTATION OF A BACK-UP CAPABILITY FOR NASA WALLOPS FLIGHT FACILITY (WFF) HIGH GAIN UHF GROUND STATION: ALL LABOR AND MATERIALS REQUIRED FOR THE IMPLEMENTATION OF A BACK-UP CAPABILITY FOR NASA-GODDARD SPACE FLIGHT CENTER (NASA-GSFC) WALLOPS FLIGHT FACILITY (WFF) HIGH GAIN UHF GROUND STATION. THE WALLOPS ISLAND 18-METER DIAMETER UHF GROUND-STATION IS, TO DATE, ANSWERING A GROWING NEED FOR HIGH DATA RATE FROM CUBESATS OVER GOVERNMENT LICENSED FREQUENCIES. THIS IS A REQUEST TO ADD A BACKUP CAPABILITY FOR THE WALLOPS ISLAND 18-METER DIAMETER UHF GROUND STATION AT MOREHEAD STATE UNIVERSITY. REQUIRED WORK: MOREHEAD STATE WILL IMPLEMENT AN INNOVATIVE UHF FEED ON THE MOREHEAD STATE UNIVERSITY 21 M GROUND STATION THAT COULD ULTIMATELY LEAD TO A SYSTEM THAT WOULD PROVIDE COMMAND AND TELEMETRY OVER UHF TO SUPPORT THE NASA AND UNIVERSITY CUBESAT COMMUNITIES, SERVING AS A BACK-UP CAPABILITY TO THE NASA WALLOPS SPACE FLIGHT CENTER (WFF) UHF GROUND STATION. REQUIRED GAIN: 34 DB, DESIRED GAIN: 37 DB; REQUIRED EIRP: 3,000 W; DESIRED EIRP: 6,320 W. THE REQUIRED FREQUENCY RANGE: 400-470 MHZ UPLINK, AND DOWNLINK. INSTALLATION: PERMANENT (IN PARALLEL AND DOES NOT CONFLICT WITH OTHER FREQUENCY BAND OPERATIONS). REMOTE CONTROL: ALLOWS FOR REMOTE OPERATION AND SCHEDULING. TESTING: AFTER INSTALLATION, SHOW PROOF OF GAIN AND DETERMINE LOCAL INTERFERENCE. BUCKET TRUCK AND MAN LIFT OPERATIONS: SHALL BE PERFORMED BY MOREHEAD STATE UNIVERSITY FOLLOWING ESTABLISHED MOREHEAD STATE UNIVERSITY SAFETY GUIDELINES. REPORTS: PROVIDE MONTHLY STATUS UPDATES (ONE PAGE REPORTS WHICH DETAIL WORK ACCOMPLISHED AND PLANS FOR NEXT MONTH). PROVIDE A TEST REPORT SHOWING GAIN, MEASUREMENT AND LOCAL INTERFERENCE AT CONCLUSION. DRAWINGS: PROVIDE AS-BUILT DRAWINGS FOR THE FEED. SCHEDULE: THE FINAL REPORT SHALL BE DELIVERED WITHIN TWO MONTHS AFTER COMPLETION. THE FORMAT IS DEFINED BY THE UNIVERSITY, AND SHALL BE APPROXIMATELY ONE (1) PAGE.MOREHEAD STATE UNIVERSITY$45,766NATIONAL AERONAUTICS AND SPACE ADMINISTRATIONNATIONAL AERONAUTICS AND SPACE ADMINISTRATION—334290Other Communications Equipment ManufacturingAJ47Dec 9, 2013Dec 9, 2013Jan 31, 2015
W912KZ13P0064
LIFE AFTER HIGH SCHOOL MOREHEAD STATEMOREHEAD STATE UNIVERSITY$0DEPT OF THE ARMYDEPT OF THE ARMY—611310Colleges, Universities, and Professional SchoolsM1PAOPERATION OF RECREATION FACILITIES (NON-BUILDING)Jun 2, 2013Jun 2, 2013Oct 26, 2013
ING07PC90086
MAP INTERPRETATIONMOREHEAD STATE UNIVERSITY$261,444US GEOLOGICAL SURVEYUS GEOLOGICAL SURVEY—541370Surveying and Mapping (except Geophysical) ServicesR499SUPPORT- PROFESSIONAL: OTHERSep 24, 2007Sep 25, 2007Sep 24, 2011
NNX07AU32G
A STUDY OF THE X-RAY LUMINOUS NORTHWESTERN RIM OF THE GALACTIC SUPERNOVA REMNANT G266.2-1.2 G266.2-1.2 IS A YOUNG SHELL-TYPE SUPERNOVA REMNANT WITH AN X-RAY SPECTRUM DOMINATED BY NON-THERMAL EMISSION. PREVIOUS X-RAY STUDIES OF THIS REMNANT BY ASCA AND ROSAT REVEALED THAT THE NORTHWESTERN RIM OF G266.2-1.2 IS PARTICULARLY LUMINOUS, BUT THESE OBSERVATIONS LACKED THE CAPABILITY OF RESOLVING THIS RIM AND THE TRUE NATURE OF THE RIM'S SPECTRUM (THERMAL OR NON-THERMAL) HAS BEEN DEBATED. TO INVESTIGATE THIS RIM IN MORE DETAIL, WE PROPOSE TO CONDUCT A HIGH-RESOLUTION OBSERVATION USING CHANDRA. IT IS VERY LIKELY THAT THE RIM IS A SITE OF COSMIC-RAY ACCELERATION, AND THE DATA WILL BE ANALYZED TO STUDY THIS PHENOMENON IN DETAIL. WE WILL ALSO SEARCH FOR THERMAL EMISSION FROM SMALLER STRUCTURES WITHIN THE RIM TO TAKE ADVANTAGE OF CHANDRA'S UNPRECEDENTED HIGH ANGULAR RESOLUTION CAPABILITIES.MOREHEAD STATE UNIVERSITY$68,749NATIONAL AERONAUTICS AND SPACE ADMINISTRATIONNATIONAL AERONAUTICS AND SPACE ADMINISTRATION——AR21Sep 11, 2007Sep 11, 2007Sep 10, 2008
ING05ERCN0017
05-2783-0073 KY PHASE IIMOREHEAD STATE UNIVERSITY$223,345US GEOLOGICAL SURVEY——541990All Other Professional, Scientific, and Technical ServicesD315Aug 9, 2005Aug 9, 2005Aug 8, 2009
DABT2397H0155
—MOREHEAD STATE UNIVERSITY$0DEPT OF THE ARMY———U005EDUCATION/TRAINING- TUITION/REGISTRATION/MEMBERSHIP FEESDec 1, 1997Dec 1, 1997—
Page 1 of 1
  • Previous
  • Next