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- W3006414977 abstract "Abstract The methods of deriving FeO and TiO 2 contents from the Clementine spacecraft data were discussed, and an approach was developed to derive the content from the measurements using the Moon Mineralogy Mapper (M 3 ) instrument on Chandrayaan‐1. The density of lunar bedrock was then modeled on the basis of the derived FeO and TiO 2 abundances. The FeO and TiO 2 abundances derived from the M 3 data were compared with the previous results of the Clementine data and were in good agreement. The FeO abundance data also agreed well with the Lunar Prospector data, which were used as an independent source. The previous Clementine and newly M 3 derived abundances were compared with the laboratory measured FeO and TiO 2 contents in the Apollo and Luna returned samples. The Clementine derived FeO content was systematically 1%–2% lower than the laboratory measurements in all the returned samples. The M 3 derived content agreed well with the returned Apollo samples and was within ±2.8% of the laboratory measurements. The Clementine derived TiO 2 abundance was systematically 0.1%–4% higher than the laboratory measurements of the returned samples. The M 3 derived TiO 2 agreed well (±0.6%) with the laboratory measurements of the returned samples, except for samples with high TiO 2 content. However, these results should be carefully interpreted because the error range requires verification. No error analysis was provided with the previous Clementine derived contents." @default.
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- W3006414977 date "2021-06-01" @default.
- W3006414977 modified "2023-10-17" @default.
- W3006414977 title "Lunar Subsurface Mineralogy and Density Profile Modelling based on Moon Mineralogy Mapper Observation" @default.
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- W3006414977 doi "https://doi.org/10.1111/1755-6724.14511" @default.
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