Mathematics – Logic
Scientific paper
Dec 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufm.p43e..10h&link_type=abstract
American Geophysical Union, Fall Meeting 2011, abstract #P43E-10
Mathematics
Logic
[5480] Planetary Sciences: Solid Surface Planets / Volcanism, [6235] Planetary Sciences: Solar System Objects / Mercury
Scientific paper
Following the Mariner 10 flybys in 1974-75, the presence and importance of volcanism on Mercury was extensively debated. Uncertainty persisted until the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) flybys in 2008-2009 confirmed that volcanism had been widespread. Questions that remain after those flybys include the global extent of volcanic plains, their style and mode of emplacement, their temporal distribution, and their association with other geological features. MESSENGER high-resolution images of Mercury obtained from orbit are providing insight into these issues and reveal that a large contiguous area of smooth plains that exceeds ~6% of the surface of the planet occupies much of the high northern latitudes. Smooth surface morphology, embayment relationships, color data, candidate vents and flow fronts, and a population of partly to wholly buried (ghost) craters provide evidence for a volcanic origin for these plains and emplacement to depths in excess of a kilometer. Nearby is an unusual assemblage of 5-10 km-diameter pits, teardrop-shaped hills, rough plains, and distal lobate-margined smooth plains, interpreted to represent source vents, lava sculpting of underlying terrain, and distal emplacement of extensive flow lobes. MESSENGER X-Ray Spectrometer data of the northern plains and elsewhere provide evidence for compositions broadly similar to terrestrial komatiites. This volcanic assemblage is consistent with the rapid emplacement of high-temperature, low-viscosity komatiite-like flood lavas and the thermal erosion of subjacent terrain. The age of these plains is similar to those associated with and postdating the Caloris impact basin, confirming that volcanism was an important process in the post-heavy-bombardment era on Mercury. These extensive plains, in the context of global volcanic deposits, expand our understanding of the nature and history of volcanism on Mercury.
Baker Mark D.
Blewett Dave T.
Byrne Paul K.
Chabot Nancy Lynne
Chapman Clark R.
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