The instruments include:
- The Lyman-Alpha Mapping Project, built and developed at the Southwest Research Institute in San Antonio. The instrument will map the entire lunar surface in the far ultraviolet spectrum and search for surface ice and frost in the polar regions and will provide images of permanently shadowed regions that are illuminated only by starlight
- The Cosmic Ray Telescope for the Effects of Radiation, or CRaTER, was built and developed by Boston University and the Massachusetts Institute of Technology in Boston. CRaTER will characterize the lunar radiation environment, allowing scientists to determine potential impacts to astronauts and other life. It also will test models on the effects of radiation and measure radiation absorption by a type of plastic that is like human tissue. The results could aid in the development of protective technologies to help keep future lunar crew members safe
- Diviner Lunar Radiometer Experiment was built and developed by the University of California, Los Angeles, and the Jet Propulsion Laboratory in Pasadena, California. Diviner will measure surface and subsurface temperatures from orbit. It will identify cold traps and potential ice deposits as well as rough terrain and other landing hazards
- The Lunar Orbiter Laser Altimeter was conceived and built by scientists and engineers at Goddard. The instrument will measure landing site slopes and lunar surface roughness and generate high resolution 3D maps of the moon. The instrument also will measure and analyze the lunar topography to identify both permanently illuminated and shadowed areas
- The Russian-built Lunar Exploration Neutron Detector has arrived from the Institute for Space Research in Moscow. The detector will create high-resolution maps of hydrogen distribution and gather information about the neutron component of lunar radiation. Its data will be analyzed for evidence of water ice near the moon’s surface
- The remaining instrument, the Lunar Reconnaissance Orbiter Camera from Arizona State University in Tempe, Arizona, will provide high resolution imagery to help identify landing sites and characterize the moon’s topography and composition and should arrive at Goddard in May


