
Proceedings Paper
Lunar magnetic field measurements with a cubesatFormat | Member Price | Non-Member Price |
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Paper Abstract
We have developed a mission concept that uses 3-unit cubesats to perform new measurements of lunar magnetic fields,
less than 100 meters above the Moon’s surface. The mission calls for sending the cubesats on impact trajectories to
strongly magnetic regions on the surface, and transmitting measurements in real-time to a nearby spacecraft, or directly
to the Earth, up until milliseconds before impact. The cubesats and their instruments are partly based on the NSF-funded
CINEMA cubesat now in Earth orbit. Two methods of reaching the Moon as a secondary payload are discussed: 1) After
launching into geostationary transfer orbit with a communication satellite, a small mother-ship travels into lunar orbit
and releases the cubesats on impact trajectories, and 2) The cubesats travel to the Moon using their own propulsion after
release into geosynchronous orbit. This latter version would also enable other near-Earth missions, such as
constellations for studying magnetospheric processes, and observations of close-approaching asteroids.
Paper Details
Date Published: 21 May 2013
PDF: 26 pages
Proc. SPIE 8739, Sensors and Systems for Space Applications VI, 873903 (21 May 2013); doi: 10.1117/12.2015666
Published in SPIE Proceedings Vol. 8739:
Sensors and Systems for Space Applications VI
Khanh D. Pham; Joseph L. Cox; Richard T. Howard; Genshe Chen, Editor(s)
PDF: 26 pages
Proc. SPIE 8739, Sensors and Systems for Space Applications VI, 873903 (21 May 2013); doi: 10.1117/12.2015666
Show Author Affiliations
Ian Garrick-Bethell, Univ. of California, Santa Cruz (United States)
Kyung Hee Univ. (Korea, Republic of)
Robert P. Lin, Univ. of California, Berkeley (United States)
Kyung Hee Univ. (Korea, Republic of)
Hugo Sanchez, NASA Ames Research Ctr. (United States)
Belgacem A. Jaroux, NASA Ames Research Ctr. (United States)
Manfred Bester, Univ. of California, Berkeley (United States)
Patrick Brown, Imperial College London (United Kingdom)
Daniel Cosgrove, Univ. of California, Berkeley (United States)
Kyung Hee Univ. (Korea, Republic of)
Robert P. Lin, Univ. of California, Berkeley (United States)
Kyung Hee Univ. (Korea, Republic of)
Hugo Sanchez, NASA Ames Research Ctr. (United States)
Belgacem A. Jaroux, NASA Ames Research Ctr. (United States)
Manfred Bester, Univ. of California, Berkeley (United States)
Patrick Brown, Imperial College London (United Kingdom)
Daniel Cosgrove, Univ. of California, Berkeley (United States)
Michele K. Dougherty, Imperial College London (United Kingdom)
Jasper S. Halekas, Univ. of California, Berkeley (United States)
Doug Hemingway, Univ. of California, Santa Cruz (United States)
Paulo C. Lozano, Massachusetts Institute of Technology (United States)
Francois Martel, Espace Inc. (United States)
Caleb W. Whitlock, Massachusetts Institute of Technology (United States)
Jasper S. Halekas, Univ. of California, Berkeley (United States)
Doug Hemingway, Univ. of California, Santa Cruz (United States)
Paulo C. Lozano, Massachusetts Institute of Technology (United States)
Francois Martel, Espace Inc. (United States)
Caleb W. Whitlock, Massachusetts Institute of Technology (United States)
Published in SPIE Proceedings Vol. 8739:
Sensors and Systems for Space Applications VI
Khanh D. Pham; Joseph L. Cox; Richard T. Howard; Genshe Chen, Editor(s)
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