Article (Scientific journals)
N2/CO ratio in comets insensitive to orbital evolution
Anderson, S. E.; Rousselot, P.; Noyelles, B. et al.
2023In Monthly Notices of the Royal Astronomical Society, 524, p. 5182-5195
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Keywords :
Comets: general; Comets: individual: C/2016 R2 (PANSTARRS) -; protoplanetary discs
Abstract :
[en] Comets are seen as depleted in nitrogen compared to the protosolar value, but a small number exhibit significantly higher than typical N2/CO ratios: C/1908 R1 (Morehouse), C/1940 R2 (Cunningham), C/1947 S1 (Bester), C/1956 R1 (Arend-Roland), C/1957 P1 (Mrkos), C/1961 R1 (Humason), C/1969 Y1 (Bennett), C/1973 E1 (Kohoutek), C/1975 V1-A (West), C/1986 P1 (Wilson), C/1987 P1 (Bradfield), C/2001 Q4 (NEAT), C/2002 VQ94 (LINEAR), C/2016 R2 (PanSTARRS), and periodic comets 1P/Halley, 29P/Schwassmann-Wachmann 1, and 67P/Churyumov-Gerasimenko. This study examines the composition and dynamical histories of these N2-'rich' comets to unearth insights into their formation processes. Using updated N2 fluorescence factors, we re-estimate the N2/CO ratios of this sample and find that they are consistent with the expected values for comets based on estimations of the protosolar nebula. These also often display larger nucleus sizes and show rapid tail morphology variations due to their ionic nature. Numerical simulations reveal no common dynamical history, suggesting that the N2/CO ratio is independent of the number of inner Solar System passages and that N2 is homogeneously distributed within these comets. These volatile-rich comets share an Oort Cloud origin which is consistent with their survival over the past 4.5 Gyr. Our study also suggests that there may be a bias using modern high-resolution spectrometers with narrow slits, which could potentially overlook the ion tail of comets. We advocate for the use of long-slit spectroscopy to potentially detect a wider range of N2-rich comets, thereby enriching our understanding of comet compositions and origins.
Disciplines :
Mathematics
Author, co-author :
Anderson, S. E.;  Institut UTINAM UMR 6213 / CNRS, Université de Franche-Comté, OSU THETA, BP 1615, 25010 Besançon Cedex, France, Aix-Marseille Université, CNRS, CNES, Institut Origines, LAM, 13013 Marseille, France
Rousselot, P.;  Institut UTINAM UMR 6213 / CNRS, Université de Franche-Comté, OSU THETA, BP 1615, 25010 Besançon Cedex, France
Noyelles, B.;  Institut UTINAM UMR 6213 / CNRS, Université de Franche-Comté, OSU THETA, BP 1615, 25010 Besançon Cedex, France
Jehin, Emmanuel  ;  Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Origines Cosmologiques et Astrophysiques (OrCa)
Mousis, O.;  Aix-Marseille Université, CNRS, CNES, Institut Origines, LAM, 13013 Marseille, France, Institut Universitaire de France (IUF), France
Language :
English
Title :
N2/CO ratio in comets insensitive to orbital evolution
Publication date :
01 October 2023
Journal title :
Monthly Notices of the Royal Astronomical Society
ISSN :
0035-8711
eISSN :
1365-2966
Publisher :
Oxford University Press, Oxford, Gb
Volume :
524
Pages :
5182-5195
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 22 August 2023

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