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P13: Organics in Meteorites and Dust Particles: Composition, Distribution, Formation and Isotopic Anomalies
Sponsor: Planetary Sciences

CoSponsor: Biogeosciences

Convener: Max Bernstein
NASA
Office 3C25
  300 E street, SW
Washington, DC, USA  20546-001
Max.Bernstein@nasa.gov

George Cody
Carnegie Institution of Washington
USA
gcody@ciw.edu


5200 2129 6240 6213 6015 .

Description: Recent analyses of meteoritic matter, interplanetary dust particles, and samples returned by the Stardust Mission indicate that the relationship between structure and isotopic anomalies of the organic matter in meteorites is more complicated than had been previously realized. Conflicting extreme theories portray meteoritic carbon compounds as either captured interstellar molecules, as products of high-temperature nebular processes, or determined by reactions on minerals in liquid water in the parent asteroid or comet regardless of the pedigree of the starting materials. For this symposium we seek reports of measurements of the molecular and isotopic composition of asteroidal cometary matter, including distribution and regiochemistry of functional groups and isotopic enrichments, both of extractable and insoluble organic matter, and models and experiments that may shed light on such measurements, or the processes which may have created them.