The program in Planetary Science focuses on the origin and evolution of planets with an emphasis on understanding the formation of Earth-like planets in our solar system and in extra-solar systems. The planetary group combines expertise in geochemical studies of extraterrestrial materials, measurements of the physical properties of planetary materials, experiments and modeling of major geophysical processes, and characterizing planetary environments to understand the origin of life on Earth and to search for life on other planets. Current research includes timescales of planet formation, giant impacts and lunar origin, impact cratering mechanics and effects on climate, tectonic processes on icy satellites, the formation of the early terrestrial atmospheres, and reconstructing the geological history of the martian surface. Our work is supported by a novel set of laboratory facilities, including the Shock Compression Laboratory, Isotope Geochemistry Laboratories and the Noble Gas Laboratory.
firstname.lastname@example.org | 530-752-4711Early terrestrial atmospheres, magma oceans and the early volatile history of Earth, chemical evolution of the mantle-crust-atmosphere system, application of surface exposure dating to understanding land surface evolution, novel techniques for reconstructing mineral dust emission from continents and climatic effects of mineral dust, sediment mass accumulation rates from extraterrestrial helium-3.
Rudolph's research involves geological fluid mechanics, broadly defined. Recent and ongoing projects investigate controls on flow and melting in the mantle wedge, global-scale mantle dynamics, and eruptive processes in geysers, mud volcanoes (including the devastating eruption of Lusi in East Java, Indonesia) as analogues to magmatic volcanoes.
Planet formation and evolution with focus on collisional processes, including giant impacts and impact cratering. Laboratory measurements of the equation of state and rheological properties of planetary materials using shock wave techniques. Experimental and computational studies of impact processes to interpret the formation, resurfacing history, physical properties, and internal structure of planets and small bodies.
Sumner is a Co-Investigator and Long Term Planner on NASA’s Mars Science Laboratory mission, which runs the Curiosity rover in Gale Crater. She is involved in science planning for the rover as well as daily operations. Her lab group research focuses on understanding the past habitability of Mars by developing the regional context of rock and geomorphic units the rover characterizes, stratigraphic models for the rock units, and reconstructing ancient depositional environments. They also work closely with geochemists to understand provenance, chemical sedimentation, diagenesis and weathering of rocks in Gale Crater.
Using extinct radioactivity and general isotopic anomalies in the early solar system recorded in primitive meteorites as a tool to study the time scales and site of nucleosynthesis, the time of formation of the solar system and planetary differentiation. Isotope and trace element geochemistry with applications to crust-mantle evolution. Heavy metal stable isotope fractionation in low temperature environments on planetary surfaces or in biological systems using newly emerging high precision mass spectrometry techniques. The development of associated experimental techniques involving high precision mass spectrometry and ultra-clean sample processing in Class-100 clean laboratories for isotope analyses.
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Research relates microscopic features of structure and bonding to macroscopic thermodynamic behavior in minerals, ceramics, and other complex materials. She has published over 500 scientific papers.