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Plato Ejecta
Plato Ejecta (click to enlarge)
 
 

Plato Ejecta

Scientists would like to explore a possible pyroclastic deposit in this region. Radar studies of this region, along with spectroscopic evidence from the US Clementine mission indicate, that this region may be covered with pyroclastic materials. As an added bonus there is a large sinuous rille (above), possibly related to the pyroclastic deposit, just south of the site.

Pyroclastic deposits consist of small, glassy volcanic beads that subdue and mantle the surrounding terrain, produced by explosive fire-fountaining eruptions billions of years ago when the Moon was more geologically active. When magma cools rapidly (quenched), atoms do not have the time to form orderly structures (minerals) so a glass results.

Pyroclastic glasses are actually the most primitive (that is, unmodified by later geologic processes) materials in the lunar sample collection. The study of the pyroclastic materials in the Apollo collection has given geochemists valuable insights into the composition and evolution of the lunar interior. However, there are comparatively few pyroclastic materials in the current collection, and the Apollo sites themselves are not representative of all of the lunar surface from a geological standpoint. Human lunar exploration is needed to complete our understanding of the formation and history of the Moon.

Pyroclastic deposits are potentially some of the most valuable resources to support human lunar habitation. Processing pyroclastic materials can provide relatively easy access to oxygen and water for future lunar explorers. Human exploration of this location will enable access to these important resources, as well as provide key insights into the nature of these pyroclastic materials and the possible source regions of these volcanic eruptions.

Credit: NASA/Goddard Space Flight Center/Arizona State University



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Last Updated: 7 Jan 2013