The composition of cometary volatiles

By D. Bockelée-Morvan, J. Crovisier, M. Mumma, H. Weaver. 2004

293 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/e33d02b65284128b4740f498a84513acb5a6647b

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Citations in the corpus

• THE IMPRINT OF EXOPLANET FORMATION HISTORY ON OBSERVABLE PRESENT-DAY SPECTRA OF HOT JUPITERS (2016, background): “…of the ”dust” mass, carbon and silicates comprise 2/9 and 4/9 of the mass in refractories, respectively, the volatiles have a composition according to Bockelée-Morvan et al. (2004), the planetesimals contain ices with all volatile species captured in the water ice as clathrates, and the gas that…”
• Composition of Titan's lower atmosphere and simple surface volatiles as measured by the Cassini‐Huygens probe gas chromatograph mass spectrometer experiment (2010, methodology): “Results obtained from that experiment were reported and discussed separately [Israel et al., 2005; Biemann, 2006; Israel et al., 2006].”
• Ceres’ evolution and present state constrained by shape data (2010, background): “Comet observations indicate that that compound could represent a few percent of the volatile phase (e.g., Bockelee-Morvan et al., 2004 for a review).”
• Cometary glycine detected in samples returned by Stardust (2009, background): “2006), and more than two dozen organic molecules have been detected to date from spectroscopic observations of comets (Bockelee-Morvan et al. 2004).”
• Subsurface oceans and deep interiors of medium-sized outer planet satellites and large trans-neptunian objects (2006, unknown): “7% was inferred by Bockelée-Morvan et al. (2004). Mea-”
• Sulphur-bearing species in the coma of comet 67P/Churyumov–Gerasimenko (2016, methodology): “This table is based on table 1 in Rodgers & Charnley (2006) and on table 1 in Bockelée-Morvan et al. (2004a).”
• The origins and concentrations of water, carbon, nitrogen and noble gases on Earth (2014, background): “Measurements of the D/H ratios of water in 5 comets (Bockelée-Morvan et al., 2004) show a ~two-fold enrichment in D compared to the chondritic signatures (Fig.”
• Water and astrobiology (2007, background): “Dynamical and chemical evidence suggests that comets had source regions in the low-temperature regions of the outer Solar System, forming in the giant-planet region out to the Kuiper belt (Mumma et al., 2002, Bockelee-Morvan et al., 2004).”
• Origin and evolution of the atmospheres of early Venus, Earth and Mars (2018, background): “…that organics of variable complexity, in amounts comparable to the mass of today’s biosphere (≈1.15×1019g), could have been delivered by impactors, which originated in the outer Solar System between the later Hadean and the LHB (Anders 1989; Bockelée-Morvan et al. 2004; Marty and Meibom 2007).”