Mini-RF

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An example Mini-RF total radar backscatter image taken in the 12.6 cm band. It shows a fresh lunar impact crater with an ejecta blanket surrounding it.

The Miniature Radio-Frequency instrument (Mini-RF) is a synthetic aperture radar (SAR) instrument on the Lunar Reconnaissance Orbiter (LRO), which is currently in orbit around the Moon. It has a resolution of 30 m/pixel and two wavelength bands, a primary band at 12.6 cm and a secondary band at 4.2 cm.[1][2] The original principal investigator of Mini-RF, Stewart Nozette, was arrested for espionage, and the current principal investigator is Ben Bussey of the Applied Physics Laboratory, where Mini-RF was built. Previous SAR instruments, such as the radar on the Magellan mission to Venus, were large, massive, power-hungry, and expensive. Intended as a demonstration of cheap, lightweight SAR technology, the Mini-RF instrument was designed in response to these concerns. Because it was a technology demonstration, Mini-RF is sometimes not included in lists of LRO's instruments.

Radar is one of the few remote sensing tools capable of distinguishing water ice from other forms of water thought to be present of the Moon, such as hydrated minerals and water adsorbed onto the lunar surface. Although the LCROSS mission, which deliberately crashed a probe into the lunar surface to look for water, detected water in Cabeus Crater, Mini-RF did not detect water ice at the LCROSS impact site.[2]

In January, 2011, after completion of Mini-RF's primary mission objectives, NASA announced that the Mini-RF transmitter had suffered a critical failure. The receiver continues working, allowing occasional bistatic radar measurements, where the radar signal is transmitted from the Earth, reflected off the Moon, and received by the Mini-RF.

References[edit]

  1. ^ Nozette, Stewart; Spudis, Paul; Bussey, Ben; Jensen, Robert; Raney, Keith; et al. (January 2010). "The Lunar Reconnaissance Orbiter Miniature Radio Frequency (Mini-RF) Technology Demonstration". Space Science Reviews 150: 285–302. Bibcode:2010SSRv..150..285N. doi:10.1007/s11214-009-9607-5. 
  2. ^ a b C. D. Neish, D. B. J. Bussey, P. Spudis, W. Marshall, B. J. Thomson, et al. (January 2011). "The nature of lunar volatiles as revealed by Mini-RF observations of the LCROSS impact site". Journal of Geophysical Research. 

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