A dual origin for water in carbonaceous asteroids revealed by CM chondrites
Author:
Publisher
Springer Science and Business Media LLC
Subject
Astronomy and Astrophysics
Link
http://www.nature.com/articles/s41550-018-0413-4.pdf
Reference59 articles.
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2. Oba, Y. & Naraoka, H. Elemental and isotope behavior of macromolecular organic matter from CM chondrites during hydrous pyrolysis. Meteorit. Planet. Sci. 44, 943–953 (2009).
3. Alexander, C. M. O. ’D. et al. Deuterium enrichments in chondritic macromolecular material—implications for the origin and evolution of organics, water and asteroids. Geochim. Cosmochim. Acta 74, 4417–4437 (2010).
4. Remusat, L., Guan, Y., Wang, Y. & Eiler, J. M. Accretion and preservation of D-rich organic particles in carbonaceous chondrites: evidence for important transport in the early Solar System nebula. Astrophys. J 713, 1048–1058 (2010).
5. Gounelle, M. et al. Hydrogen isotopic composition of water from fossil micrometeorites in howardites. Geochim. Cosmochim. Acta 69, 3431–3443 (2005).
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