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NASA NTRSDate not supplied

Volcanic Eruptions and Effects on our Climate

Volcanoes are an integral part of the Earth system and are formed by intrusions of magma that 'bubble up’ from Earth’s interior (e.g., lava lamp). They can form above thin areas of the Earth’s crust/ lithosphere known as ‘hot spots or mantle plumes’ such as the Hawaiian Islands or Yellowstone National Park. More commonly they form along ‘subduction zones’ where the thinner oceanic tectonic plates slide below the thicker continental plates. Many of the most active (and violent) volcanos lie along subduction zones known as the Pacific 'Ring of Fire’.

Volcanos↗
NASA NTRSDate not supplied

Sinus Viscositatis: Implications of Young, KREEPy Mare Eruptions for Lunar Volatile Abundances and Origins

Volatiles such as H 2 O and OH have been conclusively shown to exist across the Moon following over a decade of detailed sample analysis and remote sensing. Several mechanisms deliver volatiles to the lunar surface, including exogenous sources such as asteroid or comet bombardment (i.e., H 2 O, CO 2 , CH 4 , NH 3 , S), solar wind (i.e., H, He, Ne, Ar, Na, C, O), and galactic cosmic rays (i.e., noble gases like Xe), or endogenous sources such as outgassing from igneous lithologies (i.e., H 2 O, OH, CO 2 , S, Ar, Cl, F). Processes such as impact gardening and temperature-driven adsorption/desorption have likely supported further transport of species across the lunar surface, thus a mixture of sources is thought to be preserved. Nonetheless, volatile origins, abundances, and cycling on the Moon are not well understood and require further investigation.

A. J. Gawronska↗