OSIRIS-REx Team Prepares for Next Step in NASA’s Asteroid Sample Return Mission

June 22, 2015 -

With launch only 15 months away, the team of the OSIRIS-REx asteroid sample return mission, led by the University of Arizona, is preparing to deliver its instruments for integration with the spacecraft over the next several months. OSIRIS-REx, which stands for Origins Spectral Interpretation Resource Identification and Security-Regolith Explorer, is the first U.S. mission to take a sample from an asteroid and bring it to Earth for study.

OSIRIS-REx will travel to Bennu, a near-Earth asteroid, to bring back a small sample to Earth for study. The mission is scheduled for launch in September 2016. The spacecraft will reach its asteroid target in 2018 and return a sample to Earth in 2023.

“These instruments are essential to accomplishing the mission’s science goals and unlocking the secrets of Bennu,” said Dante Lauretta, professor in the UA’s Lunar and Planetary Laboratory and principal investigator for OSIRIS-REx. “I am proud of the dedication to excellence that each of our instrument teams brings to this mission, and I look forward to all that we will discover at the asteroid.”

The spacecraft will carry five instruments from national and international partners. These instruments will be key to mapping and analyzing Bennu’s surface and will be critical in identifying a site from which a sample can be safely retrieved and ultimately returned to Earth.

The OSIRIS-REx Camera Suite, or OCAMS, consists of three cameras that will image Bennu during approach and proximity operations. Scientists and engineers at LPL designed and built OCAMS to image Bennu over nine orders of magnitude in distance, from 1 million kilometers (more than 620,000 miles) down to two meters (6.5 feet). PolyCam, the largest camera of the OCAMS suite, is both a telescope — acquiring the asteroid from far away while it is still a point of light — and a microscope capable of scrutinizing the pebbles on Bennu’s surface. MapCam will map the entire surface of Bennu from a distance of three miles, and the Sampling Camera, or SamCam, is designed to document the sample acquisition. The OCAMS instrument suite is scheduled to be installed on the spacecraft in September.

The OSIRIS-REx Laser Altimeter, or OLA, will scan Bennu to map the entire asteroid surface, producing local and global topographic maps. OLA is a contributed instrument from the Canadian Space Agency.

The OSIRIS-REx Thermal Emission Spectrometer, or OTES, will conduct surveys to map mineral and chemical abundances and to take Bennu’s temperature. OTES is provided by Arizona State University.

The OSIRIS-REx Visible and Infrared Spectrometer, or OVIRS, measures visible and infrared light from Bennu, which can be used to identify water and organic materials. The instrument is provided by NASA’s Goddard Space Flight Center.

A student experiment called the Regolith X-ray Imaging Spectrometer, or REXIS, will map elemental abundances on the asteroid. REXIS is a collaboration between the students and faculty of the Massachusetts Institute of Technology and Harvard College Observatory.

“This is an exciting time for the project,” said Mike Donnelly, OSIRIS-REx project manager, from NASA’s Goddard Space Flight Center in Greenbelt, Maryland.  “Years of effort are coming to culmination with the upcoming deliveries of the instruments to the spacecraft.”

NASA’s Goddard Space Flight Center in Greenbelt provides overall mission management, systems engineering and safety and mission assurance for OSIRIS-REx. Lockheed Martin Space Systems in Denver is building the spacecraft. OSIRIS-REx is the third mission in NASA’s New Frontiers Program. NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages New Frontiers for the agency’s Science Mission Directorate in Washington, D.C.

 

Media Contact

Erin Morton
OSIRIS-REx Communications
520-269-2493
morton@orex.lpl.arizona.edu

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