The feasibility of the orbital gamma spectrometry of the moon and Mars using semiconductor detectors

Details The feasibility of the orbital gamma spectrometry of the moon and Mars using semiconductor detectors The feasibility of the orbital gamma spectrometry of the moon and Mars using semiconductor detectors

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kosis..27..433s&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 27, May-June 1989, p. 433-437. In Russian.

Astronomy and Astrophysics

Astronomy

1

Gamma Ray Spectrometers, Lunar Surface, Mars Surface, Semiconductor Devices, Abundance, Planetary Mapping, Satellite-Borne Instruments, Spaceborne Astronomy

Scientific paper

The paper evaluates the feasibility of using semiconductor gamma spectrometers on orbital spacecraft for the element mapping of the moon and Mars. Estimates are made of the minimum concentrations that can be determined with a gamma spectrometer employing ultrapure germanium at a volume of 200 cu cm. The efficiency of the detector according to the total absorption peak and its resolution are equal to 0.1 and 2 keV, respectively, for an energy of 1 MeV.

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