Tentative detection of cyclopropenylidene in comets

ABSTRACT We report the tentative detection of the ring molecule cyclopropenylidene (c-C$_3$H$_2$) in cometary comae. We observed three short-period comets: 73P/Schwassmann–Wachmann 3, 17P/Holmes, 103P Hartley 2, and two Oort Cloud comets: C/2007 N3 (Lulin) and C/2012 F6 (Lemmon) with the Arizona Radio Observatory Submillimeter Telescope (SMT) and the Atacama Large Millimeter/submillimeter Array (ALMA). We tentatively detected c-C$_3$H$_2$ in three of the comets, with molecule production rates in the range of $(0.2\!-\!3.8)\times 10^{25}$ molecules s$^{-1}$, and c-C$_3$H$_2$/H$_2$O mixing ratios of 0.01–0.19 per cent. Evidence from both the single-dish and interferometric data points to the presence of c-C$_3$H$_2$ being of a discrete transient nature and exhibiting an extended spatial distribution, indicating production from the decomposition of organic dust particles in the coma.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2024-10-16
DOI
https://doi.org/10.1093/mnras/stae2105
Citations
2
Primary Topic
Organoboron and organosilicon chemistry
Type
article
Field-Weighted Citation Impact
0.50

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article

Tentative detection of cyclopropenylidene in comets

Steven B. Charnley, Yo-Ling Chuang, Yi‐Jehng Kuan
2 citations
Monthly Notices of the Royal Astronomical Society
Organoboron and organosilicon chemistry
0.50
article

Tentative detection of cyclopropenylidene in comets

Steven B. Charnley, Yo-Ling Chuang, Yi‐Jehng Kuan
article en
2 citations

Abstract

ABSTRACT We report the tentative detection of the ring molecule cyclopropenylidene (c-C$_3$H$_2$) in cometary comae. We observed three short-period comets: 73P/Schwassmann–Wachmann 3, 17P/Holmes, 103P Hartley 2, and two Oort Cloud comets: C/2007 N3 (Lulin) and C/2012 F6 (Lemmon) with the Arizona Radio Observatory Submillimeter Telescope (SMT) and the Atacama Large Millimeter/submillimeter Array (ALMA). We tentatively detected c-C$_3$H$_2$ in three of the comets, with molecule production rates in the range of $(0.2\!-\!3.8)\times 10^{25}$ molecules s$^{-1}$, and c-C$_3$H$_2$/H$_2$O mixing ratios of 0.01–0.19 per cent. Evidence from both the single-dish and interferometric data points to the presence of c-C$_3$H$_2$ being of a discrete transient nature and exhibiting an extended spatial distribution, indicating production from the decomposition of organic dust particles in the coma.

Monthly Notices of the Royal Astronomical SocietyVol. 534(4)
Goddard Space Flight Center (US), Institute of Astronomy and Astrophysics, Academia Sinica (TW), National Taiwan Normal University (TW)
National Science Foundation, National Aeronautics and Space Administration, U.S. Nuclear Regulatory Commission, Ministry of Education, European School of Oncology, Alberta Livestock and Meat Agency, Korea Astronomy and Space Science Institute, National Institutes of Natural Sciences
Openalex Percentile: Top 38%
Organoboron and organosilicon chemistry
0.50
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Tentative detection of cyclopropenylidene in comets — Steven B. Charnley, Yo-Ling Chuang, et al. · Monthly Notices of the Royal Astronomical Society (2024) | TGRS Research Map | TGRS