Mathematics – Logic
Scientific paper
Jan 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999misp.conf..115w&link_type=abstract
Workshop on Mars 2001: Integrated Science in Preparation for Sample Return and Human Exploration, p. 115
Mathematics
Logic
Geomorphology, Magma, Mars Surface, Mars Volcanoes, Planetary Geology, Volcanology, Mars Environment, Mars (Planet), Mars Exploration, Topography
Scientific paper
Volcanism is a fundamental process in transferring heat and volatiles from the interior and shaping the surfaces of planetary bodies. Basic magmatic processes on planetary bodies (magma generation, ascent, storage and eruption) are modulated by initial conditions and composition, thermal and chemical structure, and a variety of factors related to the fundamental properties of the body (gravity, presence and nature of an atmosphere, etc.). Volcanism in the geological and geomorphological record of a planet thus provides key information about the location, style and amount of heat loss with time, mantle convection patterns, the evolution of the interior, and the role of volatiles in the formation and evolution of the atmosphere. An assessment of the theory of magma ascent and eruption is an important aid in the interpretation of the planetary record. Planetary exploration missions provide key information to assess and understand volcanism in the geological and geomorphological record, and each type of mission (e.g., orbiter, lander, rover) provides significant and complementary insight. In this contribution we outline some of the major outstanding problems relative to magmatism (plutonism and volcanism) on Mars, describe the potential relevance to orbital and surface aspects of 2001, including landing site selection and mission operations, and then assess the implications of these questions for future Mars exploration program missions, including sample return and human exploration.
Head James W.
Wilson Leslie
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