Athena Microscopic Imager investigation

被引:114
作者
Herkenhoff, KE
Squyres, SW
Bell, JF
Maki, JN
Arneson, HM
Bertelsen, P
Brown, DI
Collins, SA
Dingizian, A
Elliott, ST
Goetz, W
Hagerott, EC
Hayes, AG
Johnson, MJ
Kirk, RL
McLennan, S
Morris, RV
Scherr, LM
Schwochert, MA
Shiraishi, LR
Smith, GH
Soderblom, LA
Sohl-Dickstein, JN
Wadsworth, MV
机构
[1] US Geol Survey, Astrogeol Team, Flagstaff, AZ 86001 USA
[2] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA
[3] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[4] Univ Copenhagen, Niels Bohr Inst Astron Phys & Geophys, DK-2100 Copenhagen, Denmark
[5] SUNY Stony Brook, Dept Geosci, Stony Brook, NY 11794 USA
[6] NASA, Lyndon B Johnson Space Ctr, Houston, TX 77058 USA
[7] GHS Opt, Pasadena, CA 91101 USA
关键词
Mars Exploration Rover; Microscopic Imager; Athena; NASA; camera;
D O I
10.1029/2003JE002076
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
[1] The Athena science payload on the Mars Exploration Rovers ( MER) includes the Microscopic Imager ( MI). The MI is a fixed- focus camera mounted on the end of an extendable instrument arm, the Instrument Deployment Device ( IDD). The MI was designed to acquire images at a spatial resolution of 30 microns/ pixel over a broad spectral range ( 400 - 700 nm). The MI uses the same electronics design as the other MER cameras but has optics that yield a field of view of 31 x 31 mm across a 1024 x 1024 pixel CCD image. The MI acquires images using only solar or skylight illumination of the target surface. A contact sensor is used to place the MI slightly closer to the target surface than its best focus distance ( about 66 mm), allowing concave surfaces to be imaged in good focus. Coarse focusing ( similar to 2 mm precision) is achieved by moving the IDD away from a rock target after the contact sensor has been activated. The MI optics are protected from the Martian environment by a retractable dust cover. The dust cover includes a Kapton window that is tinted orange to restrict the spectral bandpass to 500 - 700 nm, allowing color information to be obtained by taking images with the dust cover open and closed. MI data will be used to place other MER instrument data in context and to aid in petrologic and geologic interpretations of rocks and soils on Mars.
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页数:23
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