Modeling the expected performance of the REgolith X-ray Imaging Spectrometer (REXIS)

OSIRIS-REx is the third spacecraft in the NASA New Frontiers Program and is planned for launch in 2016. OSIRIS-REx will orbit the near-Earth asteroid (101955) Bennu, characterize it, and return a sample of the asteroid's regolith back to Earth. The Regolith X-ray Imaging Spectrometer (REXIS) is...

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Main Authors: Inamdar, Niraj K. (Contributor), Hong, Jaesub (Author), Allen, Branden (Author), Grindlay, Jonathan E. (Author), Masterson, Rebecca A. (Contributor), Binzel, Richard P (Author)
Other Authors: Massachusetts Institute of Technology. Department of Aeronautics and Astronautics (Contributor), Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences (Contributor), Massachusetts Institute of Technology. Space Systems Laboratory (Contributor), Binzel, Richard P. (Contributor)
Format: Article
Language:English
Published: SPIE, 2015-07-21T16:02:07Z.
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Online Access:Get fulltext
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042 |a dc 
100 1 0 |a Inamdar, Niraj K.  |e author 
100 1 0 |a Massachusetts Institute of Technology. Department of Aeronautics and Astronautics  |e contributor 
100 1 0 |a Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences  |e contributor 
100 1 0 |a Massachusetts Institute of Technology. Space Systems Laboratory  |e contributor 
100 1 0 |a Inamdar, Niraj K.  |e contributor 
100 1 0 |a Binzel, Richard P.  |e contributor 
100 1 0 |a Masterson, Rebecca A.  |e contributor 
700 1 0 |a Hong, Jaesub  |e author 
700 1 0 |a Allen, Branden  |e author 
700 1 0 |a Grindlay, Jonathan E.  |e author 
700 1 0 |a Masterson, Rebecca A.  |e author 
700 1 0 |a Binzel, Richard P  |e author 
245 0 0 |a Modeling the expected performance of the REgolith X-ray Imaging Spectrometer (REXIS) 
260 |b SPIE,   |c 2015-07-21T16:02:07Z. 
856 |z Get fulltext  |u http://hdl.handle.net/1721.1/97874 
520 |a OSIRIS-REx is the third spacecraft in the NASA New Frontiers Program and is planned for launch in 2016. OSIRIS-REx will orbit the near-Earth asteroid (101955) Bennu, characterize it, and return a sample of the asteroid's regolith back to Earth. The Regolith X-ray Imaging Spectrometer (REXIS) is an instrument on OSIRIS-REx designed and built by students at MIT and Harvard. The purpose of REXIS is to collect and image sun-induced fluorescent X-rays emitted by Bennu, thereby providing spectroscopic information related to the elemental makeup of the asteroid regolith and the distribution of features over its surface. Telescopic reflectance spectra suggest a CI or CM chondrite analog meteorite class for Bennu, where this primitive nature strongly motivates its study. A number of factors, however, will influence the generation, measurement, and interpretation of the X-ray spectra measured by REXIS. These include: the compositional nature and heterogeneity of Bennu, the time-variable solar state, X-ray detector characteristics, and geometric parameters for the observations. In this paper, we will explore how these variables influence the precision to which REXIS can measure Bennu's surface composition. By modeling the aforementioned factors, we place bounds on the expected performance of REXIS and its ability to ultimately place Bennu in an analog meteorite class. 
520 |a Goddard Space Flight Center. OSIRIS-REx Program 
546 |a en_US 
655 7 |a Article 
773 |t Proceedings of SPIE--the International Society for Optical Engineering