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Cited by 233

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Clementine images of the lunar sample‐return stations: Refinement of FeO and TiO2 mapping techniques

Blewett, David T., Lucey, Paul G., Hawke, B. Ray, Jolliff, Bradley L.·1997·Journal of Geophysical Research: Planets

Abstract

Clementine UVVIS images of the lunar sample‐return sites have been processed and used to produce refined calibrations for the iron and titanium determination algorithms of Lucey et al. [1995, 1996]. The high spatial resolution of the Clementine data permits individual sampling stations to be resolved at the Apollo 15, 16, and 17 landing sites. We find an excellent, linear correlation between the spectral Fe and Ti parameters and the average FeO and TiO 2 contents of soils sampled at each site or station. This correlation demonstrates that these techniques can confidently be applied to other areas of the Moon. The Luna 24 site does not fit the Ti relation found for other sites, suggesting that either its sample is nonrepresentative or the reported landing coordinates are incorrect.

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Metadata

Authors
Blewett, D. T., Lucey, P. G., Hawke, B. R., & Jolliff, B. L.
Venue
Journal of Geophysical Research: Planets
Published
1997-07
Volume
102
Issue
E7
Pages
16319-16325
ISSN
0148-0227 (ISSN-L)
OpenAlex
W2150371620
Cited by
233
References
1
FWCI
8.88
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Clementine images of the lunar sample‐return stations: Refinement of FeO and TiO2 mapping techniques. https://app.cochat.ai/papers/10.1029/97je01505
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Blewett, D. T., Lucey, P. G., Hawke, B. R., & Jolliff, B. L. (1997). Clementine images of the lunar sample‐return stations: Refinement of FeO and TiO2 mapping techniques. Journal of Geophysical Research: Planets. https://doi.org/10.1029/97je01505

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