The Chemical Composition of Comets—Emerging Taxonomies and Natal Heritage
By M. Mumma, Steven B. Charnley. 2011
789 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Spectroscopy
View Paper: https://www.semanticscholar.org/paper/fca23fbe138ad5694aa147e42f068e426459d3dd
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Citations in the corpus
- Inventory of the volatiles on comet 67P/Churyumov-Gerasimenko from Rosetta/ROSINA (2015, background): “The most extensive list of identified molecules up to now has been established from observations of C/1995 O1 (Hale-Bopp) and C/1996 B2 (Hyakutake) (Bockelée-Morvan et al. 2004; Mumma & Charnley 2011).”
- Carbon-rich dust in comet 67P/Churyumov-Gerasimenko measured by COSIMA/Rosetta (2017, background): “The dust particles ejected from comet nuclei are therefore expected to be among the most pristine material within the Solar System, remaining almost unmodified and stored at low temperatures since their co-accretion with ices to form the icy bodies (Mumma & Charnley 2011).”
- Separating gas-giant and ice-giant planets by halting pebble accretion (2014, background): “Dependence on the (bulk) composition of the accreted material and opacity We assume the bulk composition of the material accreted by the planet to correspond to the bulk composition of cometary material (Mumma & Charnley 2011).”
- Molecules with ALMA at Planet-forming Scales (MAPS). I. Program Overview and Highlights (2021, result): “For nitriles, this is in good agreement with Solar System comet values (Mumma & Charnley 2011; Altwegg et al. 2019; Drozdovskaya et al. 2019).”
- Our astrochemical heritage (2012, methodology): “Here we briefly summarise which species have been detected and recommend to the interested reader the reviews by Mumma and Charnley (2011) and Bockelée-Morvan (2011), and Brown (2012) on the comets and KBOs, respectively.”
- Origins of volatile elements (H, C, N, noble gases) on Earth and Mars in light of recent results from the ROSETTA cometary mission (2016, neutral): “Comets are made of refractory silicates and metal, refractory and non-refractory organics, and ices (Jessberger et al., 1988; Kissel and Krueger, 1987; Mumma and Charnley, 2011; Bockelée-Morvan, 2011).”
- Observations of the Icy Universe (2015, methodology): “Comets, believed to contain the most pristine remnant ices from the formation of the solar system (e.g., Mumma & Charnley 2011), are key in answering this question.”
- EVIDENCE OF FAST PEBBLE GROWTH NEAR CONDENSATION FRONTS IN THE HL TAU PROTOPLANETARY DISK (2015, background): “…ice. References: (1) Mart́ın-Doménech et al. (2014), (2) Luna et al. (2014), (3) Sandford & Allamandola (1993), (4) Hasegawa & Herbst (1993), (5) Mumma & Charnley (2011), (6) Iro et al. (2003), (7) Lunine & Stevenson (1985) major carriers of N as predicted by chemical models of disks…”
- Complex organic molecules in protoplanetary disks (2013, background): “…CH3CHO, NH2CHO, HCOOCH3, and (HOCH2)2 have been observed in only a single object, comet Hale-Bopp, with percentage abundances of 0.02 %, 0.015 %, 0.08 %, and 0.25 % (relative to H2O), respectively (see, e.g., Bockelée-Morvan et al. 2004; Crovisier et al. 2004a,b, 2006; Mumma & Charnley 2011).”
- Astrochemistry and compositions of planetary systems (2020, background): “Other species, such as water, CH3OH, CO2, and NH3 can be denoted as volatiles.”
- The Disk Substructures at High Angular Resolution Project (DSHARP). II. Characteristics of Annular Substructures (2018, background): “…CH3OH are other volatiles expected to be abundant in disks based on cometary measurements and ice observations toward star-forming regions (e.g., Mumma & Charnley 2011; Öberg et al. 2011a), their binding energies are so high that their snowline locations are expected to be below the resolution…”