The great lunar hot spot and the composition and origin of the Apollo mafic (“LKFM”) impact‐melt breccias
By R. Korotev. 2000
140 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science
View Paper: https://www.semanticscholar.org/paper/df82188d280450e49003f4e638ca6db6cb5693a0
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In Astronomy and Astrophysics
In Atmospheric Science
Citations in the corpus
- Asymmetric thermal evolution of the Moon (2012, methodology): “4 ppm, which corresponds to the average uranium content of Apollo 15 KREEP basalts [Korotev, 2000].”
- Lunar rare earth element distribution and ramifications for FeO and TiO2: Lunar Prospector neutron spectrometer observations (2000, background): “A good correlation is expected for high concentrations of Th and the REEs, based on returned samples [Haskin and Warren, 1991; Lawrence et al., 1999; Korotev, 2000].”
- Thermal and Magmatic Evolution of the Moon (2006, background): “…terranes are the Procellarum KREEP Terrane (PKT) and the Feldspathic Highlands Terrane (FHT), and the rational for these divisions, as well as their properties and evolutionary histories are discussed in detail in Chapter 3 (see also Haskin et al. 2000; Korotev 2000; Wieczorek and Phillips 2000).”