FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4308198936> ?p ?o ?g. }

• W4308198936 endingPage "247" @default.
• W4308198936 startingPage "247" @default.
• W4308198936 abstract "Abstract CO and CO 2 are the two dominant carbon-bearing molecules in comae and have major roles in driving activity. Their relative abundances also provide strong observational constraints to models of solar system formation and evolution but have never been studied together in a large sample of comets. We carefully compiled and analyzed published measurements of simultaneous CO and CO 2 production rates for 25 comets. Approximately half of the comae have substantially more CO 2 than CO, about one-third are CO-dominated, and about 1/10 produce a comparable amount of both. There may be a heliocentric dependence to this ratio with CO dominating comae beyond 3.5 au. Eight out of nine of the Jupiter Family Comets in our study produce more CO 2 than CO. The six dynamically new comets produce more CO 2 relative to CO than the eight Oort Cloud comets that have made multiple passes through the inner solar system. This may be explained by long-term cosmic-ray processing of a comet nucleus’s outer layers. We find ( Q CO / Q <?CDATA ${}_{{{rm{H}}}_{2}{rm{O}}}$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:msub> <mml:mrow /> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi mathvariant=normal>H</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>2</mml:mn> </mml:mrow> </mml:msub> <mml:mi mathvariant=normal>O</mml:mi> </mml:mrow> </mml:msub> </mml:math> ) median = 3 ± 1% and ( Q <?CDATA ${}_{{mathrm{CO}}_{2}}$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:msub> <mml:mrow /> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi>CO</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>2</mml:mn> </mml:mrow> </mml:msub> </mml:mrow> </mml:msub> </mml:math> / Q <?CDATA ${}_{{{rm{H}}}_{2}{rm{O}}}$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:msub> <mml:mrow /> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi mathvariant=normal>H</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>2</mml:mn> </mml:mrow> </mml:msub> <mml:mi mathvariant=normal>O</mml:mi> </mml:mrow> </mml:msub> </mml:math> ) median = 12 ± 2%. The inorganic volatile carbon budget was estimated to be ( Q CO + Q <?CDATA ${}_{{mathrm{CO}}_{2}}$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:msub> <mml:mrow /> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi>CO</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>2</mml:mn> </mml:mrow> </mml:msub> </mml:mrow> </mml:msub> </mml:math> )/ Q <?CDATA ${}_{{{rm{H}}}_{2}{rm{O}}}$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:msub> <mml:mrow /> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi mathvariant=normal>H</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>2</mml:mn> </mml:mrow> </mml:msub> <mml:mi mathvariant=normal>O</mml:mi> </mml:mrow> </mml:msub> </mml:math> ∼ 18% for most comets. Between 0.7 and 4.6 au, CO 2 outgassing appears to be more intimately tied to the water production in a way that the CO is not. The volatile carbon/oxygen ratio for 18 comets is C/O median ∼ 13%, which is consistent with a comet formation environment that is well within the CO snow line." @default.
• W4308198936 created "2022-11-09" @default.
• W4308198936 creator A5026487577 @default.
• W4308198936 creator A5030237029 @default.
• W4308198936 creator A5075563134 @default.
• W4308198936 creator A5088468878 @default.
• W4308198936 date "2022-11-01" @default.
• W4308198936 modified "2023-10-18" @default.
• W4308198936 title "A Survey of CO, CO₂, and H₂O in Comets and Centaurs" @default.
• W4308198936 cites W1569667652 @default.
• W4308198936 cites W1588399065 @default.
• W4308198936 cites W1605619447 @default.
• W4308198936 cites W1731276149 @default.
• W4308198936 cites W1757157316 @default.
• W4308198936 cites W180509433 @default.
• W4308198936 cites W1927333103 @default.
• W4308198936 cites W1966409944 @default.
• W4308198936 cites W1967904481 @default.
• W4308198936 cites W1970397964 @default.
• W4308198936 cites W1971665788 @default.
• W4308198936 cites W1973820365 @default.
• W4308198936 cites W1976290853 @default.
• W4308198936 cites W1979668037 @default.
• W4308198936 cites W1981042627 @default.
• W4308198936 cites W1988094355 @default.
• W4308198936 cites W1990628291 @default.
• W4308198936 cites W1992329824 @default.
• W4308198936 cites W1996151675 @default.
• W4308198936 cites W1998367509 @default.
• W4308198936 cites W2005370799 @default.
• W4308198936 cites W2005878095 @default.
• W4308198936 cites W2006753204 @default.
• W4308198936 cites W2007479666 @default.
• W4308198936 cites W2012538764 @default.
• W4308198936 cites W2017171309 @default.
• W4308198936 cites W2018813327 @default.
• W4308198936 cites W2019037646 @default.
• W4308198936 cites W2019323263 @default.
• W4308198936 cites W2019858160 @default.
• W4308198936 cites W2020747216 @default.
• W4308198936 cites W2021173216 @default.
• W4308198936 cites W2021710389 @default.
• W4308198936 cites W2022414649 @default.
• W4308198936 cites W2023671303 @default.
• W4308198936 cites W2026705112 @default.
• W4308198936 cites W2028596155 @default.
• W4308198936 cites W2028755602 @default.
• W4308198936 cites W2033677921 @default.
• W4308198936 cites W2034182837 @default.
• W4308198936 cites W2040091043 @default.
• W4308198936 cites W2041775599 @default.
• W4308198936 cites W2042070050 @default.
• W4308198936 cites W2042745022 @default.
• W4308198936 cites W2044028692 @default.
• W4308198936 cites W2047421713 @default.
• W4308198936 cites W2054343995 @default.
• W4308198936 cites W2055103834 @default.
• W4308198936 cites W2062784711 @default.
• W4308198936 cites W2065613880 @default.
• W4308198936 cites W2068616791 @default.
• W4308198936 cites W2074775973 @default.
• W4308198936 cites W2075170866 @default.
• W4308198936 cites W2075950193 @default.
• W4308198936 cites W2077736421 @default.
• W4308198936 cites W2079947449 @default.
• W4308198936 cites W2079958881 @default.
• W4308198936 cites W2080139342 @default.
• W4308198936 cites W2081913356 @default.
• W4308198936 cites W2085344882 @default.
• W4308198936 cites W2086166607 @default.
• W4308198936 cites W2089661396 @default.
• W4308198936 cites W2091933599 @default.
• W4308198936 cites W2094528250 @default.
• W4308198936 cites W2095203252 @default.
• W4308198936 cites W2095900042 @default.
• W4308198936 cites W2096471541 @default.
• W4308198936 cites W2098359476 @default.
• W4308198936 cites W2102531911 @default.
• W4308198936 cites W2104149407 @default.
• W4308198936 cites W2105419182 @default.
• W4308198936 cites W2112635069 @default.
• W4308198936 cites W2113372437 @default.
• W4308198936 cites W2119153098 @default.
• W4308198936 cites W2122590090 @default.
• W4308198936 cites W2123913162 @default.
• W4308198936 cites W2130350225 @default.
• W4308198936 cites W2131839574 @default.
• W4308198936 cites W2133828938 @default.
• W4308198936 cites W2133851153 @default.
• W4308198936 cites W2134099876 @default.
• W4308198936 cites W2139028326 @default.
• W4308198936 cites W2140717182 @default.
• W4308198936 cites W2146348165 @default.
• W4308198936 cites W2147402624 @default.
• W4308198936 cites W2151248829 @default.
• W4308198936 cites W2153256222 @default.
• W4308198936 cites W2156573163 @default.
• W4308198936 cites W2157143763 @default.

• next