Magmatic Evolution II: A New View of Post-Differentiation Magmatism

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00025798%3A_____%2F23%3A10169340" target="_blank" >RIV/00025798:_____/23:10169340 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1515/9781501519895-007" target="_blank" >https://doi.org/10.1515/9781501519895-007</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1515/9781501519895-007" target="_blank" >10.1515/9781501519895-007</a>

Result language
angličtina
Original language name
Magmatic Evolution II: A New View of Post-Differentiation Magmatism
Original language description
Just as the use of new tools revolutionized lunar science in 1610 (Galileo's telescope), 1840 (photography), and 1960s-1970s and 1990s (over 45 robotic and human missions to the Moon), data from science-driven, international lunar missions that have flown since 2000 (Gaddis et al. 2023, this volume) and technology-driven sample observations and computational methods have provided a 21st century perspective for the thermal and magmatic evolution of the Moon. In this chapter, we integrate all these observations to reexamine the steps forward that have been taken since publication of the New Views of the Moon 1 (NVM1) in 2006 (Jolliff et al. 2006). This chapter provides a summary of post-differentiation magmatism, describes new observations, and integrates and interprets these observations for renewed understanding of the thermal evolution of the Moon, the first stages of post-differentiation magmatism (Mg-suite, alkali-suite), continued periods of basaltic magmatism with an evolved trace element signature (i.e., elevated abundances of K, REE, P, U, Th, hereafter "KREEP"), mare magmatism, and felsic-silicic magmatism.
Czech name
—
Czech description
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Publication year
2023
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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