Lunar iron and titanium abundance algorithms based on final processing of Clementine ultraviolet‐visible images

By Paul G. Lucey, D. Blewett, B. Jolliff. 2000

566 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/3ee88bebbcab07b7139ee29e7ae90637c125aad9

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In Astronomy and Astrophysics

1. L. Elkins‐Tanton
2. C. Shearer
3. P. C. Hess
4. Mark S. Robinson
5. Paul G. Lucey
6. D. Blewett
7. A. Halliday
8. Mark A. Wieczorek

Citations in the corpus

• The origin of lunar crater rays (2000, methodology): “The optical maturity values for fresh crater ejecta decrease systematically with age (Lucey et al., 2000b).”
• Thermal and Magmatic Evolution of the Moon (2006, methodology): “FeO and TiO2 abundances derived from Clementine remotely sensed data (Lucey et al. 2000) and Lunar Prospector Th abundances (Lawrence et al. 2000) are in good agreement with those derived from the Apollo data, and are consistent with Apollo 15 KREEP basalts (Blewett and Hawke 2001).”
• The Mercury Atmospheric and Surface Composition Spectrometer for the MESSENGER Mission (2007, background): “…should be on the order of 10% or better; although Warell and Blewett (2004) argued that differences in composition and rates of space weathering on Mercury and the Moon (Cintala 1992) may nullify many of the detailed retrieval algorithms for lunar materials (e.g. Lucey et al. 1998, 2000a, 2000b).”