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Walter S. Kiefer Gravity constraints on the subsurface structure of the Marius Hills: The magmatic plumbing of the largest lunar volcanic dome complex Journal of Geophysical Research: Planets 118

Version of Record online: 15 APR 2013 | DOI: 10.1029/2012JE004111

Key Points

  • Surface topography explains less than half of the Marius Hills gravity anomaly
  • Buried basalt layers, more than 3-6 km thick, served as magma chambers
  • A source of high viscosity, crystal-rich lava that formed volcanic domes

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