Surface and downhole prospecting tools for planetary exploration: tests of neutron and gamma ray probes.
The ability to locate and characterize icy deposits and other hydrogenous materials on the Moon and Mars will help us understand the distribution of water and, therefore, possible habitats at Mars, and may help us locate primitive prebiotic compounds at the Moon's poles. We have developed a rover-borne neutron probe that localizes a near-surface icy deposit and provides information about its burial depth and abundance. We have also developed a borehole neutron probe to determine the stratigraphy of hydrogenous subsurface layers while operating within a drill string segment. In our field tests, we have used a neutron source to "illuminate" surrounding materials and gauge the instruments' efficacy, and we can simulate accurately the observed instrument responses using a Monte Carlo nuclear transport code (MCNPX). An active neutron source would not be needed for lunar or martian near-surface exploration: cosmic-ray interactions provide sufficient neutron flux to depths of several meters and yield better depth and abundance sensitivity than an active source. However, for deep drilling (>or=10 m depth), a source is required. We also present initial tests of a borehole gamma ray lithodensity tool and demonstrate its utility in determining soil or rock densities and composition.
Planetary Systems Branch, Space Science and Astrobiology Division, NASA Ames Research Center, Moffett Field, California 94035-1000, USA. richard.c.elphic@nasa.gov
R C
RC
Elphic
P
P
Chu
S
S
Hahn
M R
MR
James
D J
DJ
Lawrence
T H
TH
Prettyman
J B
JB
Johnson
R K
RK
Podgorney
D005720:Gamma Rays; D006859:Hydrogen / Q000032:analysis; D009502:Neutrons; D013026:Space Flight / Q000295:instrumentation*; D013499:Surface Properties
D006859:Hydrogen