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Moon Mineral Mapper (M3): A High Uniformity and High Precision Science Imaging Spectrometer in the Solar Reflected SpectrumThe Moon Mineralogy Mapper was selected as a NASA Discovery Mission of Opportunity in February 2005. At the core of this mission is an imaging spectrometer instrument with high spectral-spatial uniformity and high signal-to-noise ratio for the expected illumination conditions. The spectral range of the Moon Mineralogy Mapper is from 430 to 3000 nm with 10 nm spectral sampling. The radiometric range is from 0 to maximum expected radiance with 14 bit sampling. The spatial swath is nominally 40 Ian with 70 m spatial sampling. The Moon Mineralogy Mapper has both a global and target mode of data acquisition. In global spectral and spatial resolution full coverage of the Moon will be acquired. Target mode will be used to examine selected areas a full spectral and spatial resolution. The science objectives and mission and instrument characteristics are presented.
Document ID
20090010330
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
Authors
Green, Robert O.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Pieters, Carle
(Brown Univ. Providence, RI, United States)
Mouroulis, Pantazis
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 24, 2013
Publication Date
July 31, 2006
Subject Category
Solar Physics
Meeting Information
Meeting: International Geoscience and Remote Sensing Symposium
Location: Colorado
Country: United States
Start Date: July 31, 2006
End Date: August 4, 2006
Distribution Limits
Public
Copyright
Other
Keywords
mapping
image spectrometer
lunar surface

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