Deuterium enrichments in chondritic macromolecular material—Implications for the origin and evolution of organics, water and asteroids
By C. Alexander, S. Newsome, M. Fogel, L. Nittler, H. Busemann, G. Cody. 2010
207 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Ecology, Spectroscopy
View Paper: https://www.semanticscholar.org/paper/8a5180ed3fef2e5b733f810690f1473156f3120e
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In Astronomy and Astrophysics
In Spectroscopy
Citations in the corpus
- Astrophysics with Extraterrestrial Materials (2016, background): “Thus, whether the organics are interstellar, nebular, and/or planetary in origin remains hotly debated (Alexander et al. 2010, Cody et al. 2011).”
- The pH of Enceladus’ ocean (2015, background): “The presence of ferric (Fe+3) phases (e.g., magnetite, maghemite, cronstedtite) in aqueously altered chondrites (Brearley, 2006) demonstrates that this process can also occur in chondritic systems (Rosenberg et al., 2001; Alexander et al., 2010).”
- Origins of building blocks of life: A review (2017, background): “CR2s are the most primitive, least altered chondrites (Cody and Alexander, 2005; Alexander et al., 2010), and typically have a higher concentration of amino acids than chondrites that experienced more severe aqueous or thermal alteration in meteorite parent bodies (Burton et al., 2012).”