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The OVIRS Visible/IR Spectrometer on the OSIRIS-Rex MissionThe OSIRIS-REx (Origins Spectral Interpretation Resource Identification Security Regolith Explorer) Mission is a planetary science mission to study, and return a sample from, the carbonaceous asteroid 1999 RQ-36. The third mission selected under NASA's New Frontiers Program, it is scheduled to be launched in 2016. It is led by PI Dante Lauretta at the University of Arizona and managed by NASA's Goddard Space Flight Center. The spacecraft and the asteroid sampling mechanism, TAGSAM (Touch-And-Go Sample Acquisition Mechanism) will be provided by Lockheed Martin Space Systems. Instrumentation for studying the asteroid include: OCAMS (the OSIRIS-REx Camera Suite), OLA (the OSIRIS-REx Laser Altimeter, a scanning LIDAR), OTES (The OSIRIS-REx Thermal Emission Spectrometer, a 4-50 micron point spectrometer) and OVIRS (the OSIRIS-REx Visible and IR Spectrometer, a 0.4 to 4.3 micron point spectrometer). The payload also includes REXIS (the Regolith X-ray Imaging Spectrometer) a student provided experiment. This paper presents a description of the OVIRS instrument.
Document ID
20120013706
Document Type
Conference Paper
Authors
Reuter, D. C. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Simon-Miller, A. A. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 26, 2013
Publication Date
October 10, 2012
Subject Category
Instrumentation and Photography
Report/Patent Number
GSFC.ABS.6879.2012
Meeting Information
International Workshop on Instrumentation for Planetary Missions(Greenbelt, MD)
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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