| Literature DB >> 21659601 |
Christopher D K Herd1, Alexandra Blinova, Danielle N Simkus, Yongsong Huang, Rafael Tarozo, Conel M O'D Alexander, Frank Gyngard, Larry R Nittler, George D Cody, Marilyn L Fogel, Yoko Kebukawa, A L David Kilcoyne, Robert W Hilts, Greg F Slater, Daniel P Glavin, Jason P Dworkin, Michael P Callahan, Jamie E Elsila, Bradley T De Gregorio, Rhonda M Stroud.
Abstract
The complex suite of organic materials in carbonaceous chondrite meteorites probably originally formed in the interstellar medium and/or the solar protoplanetary disk, but was subsequently modified in the meteorites' asteroidal parent bodies. The mechanisms of formation and modification are still very poorly understood. We carried out a systematic study of variations in the mineralogy, petrology, and soluble and insoluble organic matter in distinct fragments of the Tagish Lake meteorite. The variations correlate with indicators of parent body aqueous alteration. At least some molecules of prebiotic importance formed during the alteration.Entities:
Year: 2011 PMID: 21659601 DOI: 10.1126/science.1203290
Source DB: PubMed Journal: Science ISSN: 0036-8075 Impact factor: 47.728