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Lunar Mare Basaltic Volcanism: Volcanic Features and Emplacement Processes

Research output: Contribution to Journal/MagazineJournal articlepeer-review

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  • James W. Head
  • Harald Hiesinger
  • Carolyn van der Bogert
  • Yuan Chen
  • James L. Dickson
  • Lisa R. Gaddis
  • Junichi Haruyama
  • Erica R. Jawin
  • Lauren M. Jozwiak
  • Chunlai Li
  • Jianzhong Liu
  • Tomokatsu Morota
  • Debra H. Needham
  • Lillian R. Ostrach
  • Carle M. Pieters
  • Tabb C. Prissel
  • Yuqi Qian
  • Le Qiao
  • Malcolm R. Rutherford
  • David R. Scott
  • Jennifer L. Whitten
  • Long Xiao
  • Feng Zhang
  • Ouyang Ziyuan
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<mark>Journal publication date</mark>1/12/2023
<mark>Journal</mark>Reviews in Mineralogy and Geochemistry
Issue number1
Volume89
Number of pages55
Pages (from-to)453-507
Publication StatusPublished
<mark>Original language</mark>English

Abstract

Volcanism is a fundamental process in the geological evolution of the Moon, providing clues to the composition and structure of the mantle, the location and duration of interior melting, the nature of convection and lunar thermal evolution. Progress in understanding volcanism has been remarkable in the short 60-year span of the Space Age. Before Sputnik 1 in 1957, the lunar farside was unknown, the origin of the dark lunar maria was debated (sedimentary or volcanic), and significant controversy surrounded the question of how the multitude of craters on the surface formed.