The Nature and Distribution of the Organic Material in Carbonaceous Chondrites and Interplanetary Dust Particles
By S. Pizzarello, G. Cooper, G. Flynn. 2006
266 citations recorded by the source corpus.
View Paper: https://www.semanticscholar.org/paper/a22e65c6b06cb599146504e7085d78582446c847
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
- L. Nittler
- C. Alexander
- H. Busemann
- J. Elsila
- S. Newsome
- M. Fogel
- D. Glavin
- G. Cody
Citations in the corpus
- Deuterium enrichments in chondritic macromolecular material—Implications for the origin and evolution of organics, water and asteroids (2010, background): “Primitive chondritic meteorites contain up to 2 wt% organic C, and interplanetary dust particles (IDPs) can contain even more (Gilmour, 2003; Pizzarello et al., 2006).”
- Cometary glycine detected in samples returned by Stardust (2009, background): “Glycine has not been previously detected in comets, although it has been identified in many carbonaceous meteorites (e.g., Ehrenfreund et al. 2001a; Pizzarello et al. 2006; Martins et al. 2007).”