Lunar Reconnaissance Orbiter Overview: The Instrument Suite and Mission View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2007-04

AUTHORS

Gordon Chin, Scott Brylow, Marc Foote, James Garvin, Justin Kasper, John Keller, Maxim Litvak, Igor Mitrofanov, David Paige, Keith Raney, Mark Robinson, Anton Sanin, David Smith, Harlan Spence, Paul Spudis, S. Alan Stern, Maria Zuber

ABSTRACT

NASA’s Lunar Precursor Robotic Program (LPRP), formulated in response to the President’s Vision for Space Exploration, will execute a series of robotic missions that will pave the way for eventual permanent human presence on the Moon. The Lunar Reconnaissance Orbiter (LRO) is first in this series of LPRP missions, and plans to launch in October of 2008 for at least one year of operation. LRO will employ six individual instruments to produce accurate maps and high-resolution images of future landing sites, to assess potential lunar resources, and to characterize the radiation environment. LRO will also test the feasibility of one advanced technology demonstration package. The LRO payload includes: Lunar Orbiter Laser Altimeter (LOLA) which will determine the global topography of the lunar surface at high resolution, measure landing site slopes, surface roughness, and search for possible polar surface ice in shadowed regions, Lunar Reconnaissance Orbiter Camera (LROC) which will acquire targeted narrow angle images of the lunar surface capable of resolving meter-scale features to support landing site selection, as well as wide-angle images to characterize polar illumination conditions and to identify potential resources, Lunar Exploration Neutron Detector (LEND) which will map the flux of neutrons from the lunar surface to search for evidence of water ice, and will provide space radiation environment measurements that may be useful for future human exploration, Diviner Lunar Radiometer Experiment (DLRE) which will chart the temperature of the entire lunar surface at approximately 300 meter horizontal resolution to identify cold-traps and potential ice deposits, Lyman-Alpha Mapping Project (LAMP) which will map the entire lunar surface in the far ultraviolet. LAMP will search for surface ice and frost in the polar regions and provide images of permanently shadowed regions illuminated only by starlight. Cosmic Ray Telescope for the Effects of Radiation (CRaTER), which will investigate the effect of galactic cosmic rays on tissue-equivalent plastics as a constraint on models of biological response to background space radiation. The technology demonstration is an advanced radar (mini-RF) that will demonstrate X- and S-band radar imaging and interferometry using light weight synthetic aperture radar. This paper will give an introduction to each of these instruments and an overview of their objectives. More... »

PAGES

391-419

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s11214-007-9153-y

DOI

http://dx.doi.org/10.1007/s11214-007-9153-y

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1018627886


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104 rays
105 region
106 resolution
107 resources
108 response
109 robotic missions
110 robotics program
111 roughness
112 selection
113 series
114 site selection
115 site slope
116 sites
117 slope
118 space exploration
119 space radiation
120 starlight
121 suite
122 surface
123 surface ice
124 surface roughness
125 synthetic aperture radar
126 technology demonstration
127 telescope
128 temperature
129 tissue-equivalent plastic
130 topography
131 ultraviolet
132 vision
133 water ice
134 way
135 wide-angle images
136 years
137 years of operation
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