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         <ResourceName>The Compton Gamma-Ray Observatory (CGRO)</ResourceName>
         <ReleaseDate>2026-09-17T13:18:17</ReleaseDate>
         <Description>The Compton Gamma-Ray Observatory is one of NASA&#039;s four &quot;Great Observatories&quot;. It&#039;s specific mission is to study the sources and astrophysical processes (e.g., nuclear reactions, electron bremsstrahlung, matter-antimatter annihilation, elementary particle producation and decay, Compton scattering, and synchrotron radiation) that produce that highest energy electromagnetic radiation from the cosmos. GRO carries a complement of four instruments that provide simultaneous observations covering over five decades of energy from 0.1 MeV to 30 GeV: the Burst and Transient Source Experiment (BATSE), the Oriented Scintillation Spectrometer Experiment (OSSE), the Imaging Compton Telescope (COMPTEL), and the Energetic Gamma-Ray Experiment Telescope (EGRET).</Description>
         <Contact>
            <PersonID>spase://SMWG/Person/Neil.Gehrels</PersonID>
            <Role>ProjectManager</Role>
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         <Contact>
            <PersonID>spase://SMWG/Person/Olga.Y.Uritskaya </PersonID>
            <Role>MetadataContact</Role>
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         <InformationURL>
            <URL>https://nssdc.gsfc.nasa.gov/nmc/spacecraft/display.action?id=1991-027B</URL>
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      <Location>
         <ObservatoryRegion>Earth.NearSurface</ObservatoryRegion>
      </Location>
      <LaunchDate>1991-04-05</LaunchDate>
      <OperatingSpan>
         <StartDate>1991-04-05T12:00:00</StartDate>
         <StopDate>2000-05-01T00:00:00</StopDate>
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