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Science 4 September 1998: Vol. 281. no. 5382, pp. 1493 - 1496 DOI: 10.1126/science.281.5382.1493
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Reports
Lunar Fe and Ti Abundances: Comparison of Lunar Prospector and Clementine Data
R. C. Elphic,
*
D. J. Lawrence,
W. C. Feldman,
B. L. Barraclough,
S. Maurice,
A. B. Binder,
P. G. Lucey
The Lunar Prospector neutron spectrometer data correlate well with
iron and titanium abundances obtained through analysis of Clementine
spectral reflectance data. With the iron and titanium dependence
removed, the neutron spectrometer data also reveal regions with
enhanced amounts of gadolinium and samarium, incompatible rare earth
elements that are enriched in the final phases of magma crystallization. These regions are found mainly around the ramparts of
the Imbrium impact basin but not around the other basins, including the
much larger and deeper South Pole-Aitken basin. This result confirms
the compositional uniqueness of the surface and interior of the Imbrium
region.
R. C. Elphic, D. J. Lawrence, W. C. Feldman,
B. L. Barraclough, Space and Atmospheric Sciences, MS D466, Los
Alamos National Laboratory, Los Alamos, NM 87545, USA. S. Maurice,
Observatoire Midi-Pyrénées, 31400 Toulouse, France. A. B. Binder, Lunar Research Institute, Gilroy, CA 95020, USA. P. G. Lucey, Hawai'i Institute of Geophysics and Planetology, University of
Hawai'i, Honolulu, HI 96822, USA.
*
To whom correspondence should be addressed. E-mail:
relphic{at}lanl.gov
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