Project Details
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A new chronology of the early solar system

Subject Area Mineralogy, Petrology and Geochemistry
Term from 2006 to 2011
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 18714276
 
Final Report Year 2015

Final Report Abstract

Recent analytical advances in isotope geochemistry have started to lead to a fundamental revision of our understanding of early solar system evolution. Our project has been investigating this topic by (1) dating of various early solar system materials and (2) by assessing homogenisation processes in the early protoplanetary disk through measurements of heavy p-process isotopes that were exclusively produced in supernova environments. In the past, sufficiently precise measurements were nearly impossible due to instrumental limitations. Our group at Cologne-Bonn therefore founded a state of the art isotope laboratory, including acquisition of a new generation Multicollector ICPMS with better detection limits and improved amplifying systems, where such challenging measurements are now possible. We performed Hf-W chronometry, nucleosynthetic isotope measurements and high precision trace element measurements on a variety of extraterrestrial samples such as iron meteorites, primitive achondrites, chondrites and even lunar samples. Beyond cosmochemistry, our new isotope laboratory set the stage for a wide range of studies by our group and collaborators, covering fields like early Earth evolution, magmatism, geochronology and even low temperature fields like analytical paleontology, soil science or oceanography.

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