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Modeling orbital gamma-ray spectroscopy experiments at carbonaceous asteroids

  • Published:2016-11-06 Issue:1 Volume:52 Page:174-190
  • ISSN:1086-9379
  • Container-title:Meteoritics & Planetary Science
  • language:en
  • Short-container-title:Meteorit Planet Sci

Author:

Lim Lucy F.1,Starr Richard D.12,Evans Larry G.13,Parsons Ann M.1,Zolensky Michael E.4,Boynton William V.5

Affiliation:

1. NASA Goddard Space Flight Center; Code 691 Greenbelt Maryland 20771 USA

2. Catholic University of America; Washington District of Columbia 20064 USA

3. Computer Sciences Corporation; Lanham-Seabrook Maryland 20706 USA

4. ARES; NASA Johnson Space Center; Houston Texas 77058 USA

5. Lunar and Planetary Laboratory; University of Arizona; Tucson Arizona 85721 USA

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Reference30 articles.

1. Use of the 27Al(p, γ) 28Si, Ep = 992 keV resonance as a gamma-ray intensity standard;Antilla;Nuclear Instruments and Methods,1977

2. The Mars Odyssey gamma-ray spectrometer instrument suite;Boynton;Space Science Reviews,2004

3. Concentration of H, Si, Cl, K, Fe, and Th in the low- and mid-latitude regions of Mars;Boynton;Journal of Geophysical Research (Planets),2007

4. The fall, recovery, orbit, and composition of the Tagish Lake meteorite: A new type of carbonaceous chondrite;Brown;Science,2000

5. Analysis of gamma ray spectra measured by Mars Odyssey;Evans;Journal of Geophysical Research (Planets),2006

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