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Low frequency astronomy from lunar orbitAs part of preparation for establishing a permanently manned lunar outpost, a plan is proposed whereby relatively simple phased arrays of dipoles will be placed on individual lunar satellites to perform interferometry between the spacecraft. The dipole arrays will be deployed as inflatable structures. The experiment will function at 13 and 26 MHz. For a scenario in which two spacecraft are in perpendicular lunar polar orbits at altitudes of 100 km, the useful physical baselines will range from about 1 to about 1500 km. With a mission lifetime of one year, the two-element interferometer will produce synthetic aperture imaging with a resolution of about 2 arcsec.
Document ID
19930058144
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Basart, John P.
(Iowa State Univ. of Science and Technology, Ames, United States)
Burns, Jack O.
(New Mexico State Univ. Las Cruces, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1992
Publication Information
Publication: In: Engineering, construction, and operations in space - III: Space '92; Proceedings of the 3rd International Conference, Denver, CO, May 31-June 4, 1992. Vol. 2 (A93-41976 17-12)
Publisher: American Society of Civil Engineers
Subject Category
Astronomy
Accession Number
93A42141
Funding Number(s)
CONTRACT_GRANT: NAG9-396
Distribution Limits
Public
Copyright
Other

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