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avatar for Qing-zhu Yin

Qing-zhu Yin

UC Davis - Earth and Planetary Sciences
Professor

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.

Yin publications: http://scholar.google.com/citations?user=gNXr8W8AAAAJ

Talk abstract: 

Planetary science is the ultimate applied science. Through the application and integration of physics, chemistry, applied math, geology and biology, planetary scientists study the origin of organic and inorganic matter in the universe and how this matter condenses and aggregates in molecular clouds and disks to form planetesimals, planetary embryos and ultimately planets. Planetary science spans the experimental, theoretical and observational study of planets (including Earth and exoplanets), moons, and space debris like asteroids and comets, and the processes that form them. It focuses on objects ranging in size from micrometeoroids to gas giants, aiming to determine their composition, dynamics, formation, and history.
We are currently experiencing a golden age of planetary exploration and discovery. New exploration of planetary bodies in our solar system (especially the Moon, Mars, and Mercury and other minor bodies), combined with the rapid and increasing discovery of planets outside our solar system, are revolutionizing the science and our understanding of the place of Earth and humans within the cosmos.
In this brief talk, I will introduce the current research activities by my UC Davis colleagues in this exciting field, ranging from UV, infrared, and microwave spectroscopy aimed at understanding formation and destruction of complex astromolecules; using collisions as means to study planetary properties, and as a mode of planet formation; how do we uncover chemical and isotopic finger prints of planet formation processes and its timescale; and finally what we have learned from Mars Science Laboratory, NASA’s flagship mission to Mars.  
 

My Speakers Sessions

Tuesday, May 12
 

13:50 GMT-03