Skip to Main Content
UCLA Logo Neos

NEO Surveyor spacecraft, the flight segment of NEO Surveyor (Image credit: NASA/JPL-Caltech)

The University of California-Los Angeles has a long history in leading NASA space missions and instruments, such as the DAWN mission to asteroids (1) Ceres and (4) Vesta, the Diviner Lunar Radiometer Experiment on the Lunar Reconnaissance Orbiter (LRO), the Wide-field Infrared Survey Explorer (WISE) and its extended mission the Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE), the Electron Losses and Fields (ELFIN) mission, and the RIMFAX Ground Penetrating Radar Experiment on NASA’s Mars 2020 Rover Mission. UCLA is home to the Near-Earth Object Surveyor mission as well as the NEOWISE mission, which is completing its final stages of data collection in July 2024. NEOWISE serves as a key precursor mission for the new NEO Surveyor, which will greatly expand NASA’s ability to find Earth-approaching asteroids and comets.

NEO Surveyor will complement the capabilities of NEOWISE and enable NASA to find NEOs much faster. NEO Surveyor’s flight segment is a space-based observatory of the same name. The NEO Surveyor payload contains an infrared telescope operating in two infrared bands, 4-5 microns and 6-10 microns.  With the use of an all-infrared telescope, NEO Surveyor is optimized for the task of finding and characterizing the impact risks posed by potentially hazardous objects, both as individual objects and as populations.