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Operation of MRO's High Resolution Imaging Science Experiment (HiRISE): Maximizing Science ParticipationScience return from the Mars Reconnaissance Orbiter (MRO) High Resolution Imaging Science Experiment (HiRISE) will be optimized by maximizing science participation in the experiment. MRO is expected to arrive at Mars in March 2006, and the primary science phase begins near the end of 2006 after aerobraking (6 months) and a transition phase. The primary science phase lasts for almost 2 Earth years, followed by a 2-year relay phase in which science observations by MRO are expected to continue. We expect to acquire approx. 10,000 images with HiRISE over the course of MRO's two earth-year mission. HiRISE can acquire images with a ground sampling dimension of as little as 30 cm (from a typical altitude of 300 km), in up to 3 colors, and many targets will be re-imaged for stereo. With such high spatial resolution, the percent coverage of Mars will be very limited in spite of the relatively high data rate of MRO (approx. 10x greater than MGS or Odyssey). We expect to cover approx. 1% of Mars at approx. 1m/pixel or better, approx. 0.1% at full resolution, and approx. 0.05% in color or in stereo. Therefore, the placement of each HiRISE image must be carefully considered in order to maximize the scientific return from MRO. We believe that every observation should be the result of a mini research project based on pre-existing datasets. During operations, we will need a large database of carefully researched 'suggested' observations to select from. The HiRISE team is dedicated to involving the broad Mars community in creating this database, to the fullest degree that is both practical and legal. The philosophy of the team and the design of the ground data system are geared to enabling community involvement. A key aspect of this is that image data will be made available to the planetary community for science analysis as quickly as possible to encourage feedback and new ideas for targets.
Document ID
20030066806
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
E Eliason
(United States Geological Survey Reston, Virginia, United States)
C J Hansen
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
A McEwen
(University of Arizona Tucson, Arizona, United States)
W A Delamere
(Ball Aerospace and Technologies )
N Bridges
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
J Grant
(Smithsonian Institution Washington D.C., District of Columbia, United States)
V Gulick
(Ames Research Center Mountain View, California, United States)
Kenneth E Herkenhoff
(United States Geological Survey Reston, Virginia, United States)
L Keszthelyi
(United States Geological Survey Reston, Virginia, United States)
R Kirk
(United States Geological Survey Reston, Virginia, United States)
M Mellon
(University of Colorado Boulder Boulder, Colorado, United States)
P Smith
(University of Arizona Tucson, Arizona, United States)
S Squyres
(Cornell University Ithaca, New York, United States)
N Thomas
(University of Bern Bern, Switzerland)
C Weitz
(Planetary Science Institute Tucson, Arizona, United States)
Date Acquired
August 21, 2013
Publication Date
July 25, 2003
Publication Information
Publication: Sixth International Conference on Mars
Publisher: LPI
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
3212
Meeting Information
Meeting: Sixth International Conference on Mars
Location: Pasadena, CA
Country: US
Start Date: July 20, 2003
End Date: July 25, 2003
Sponsors: Lunar and Planetary Institute
Funding Number(s)
CONTRACT_GRANT: NCC5-679
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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