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Hydrogen isocyanide in comet 73P/Schwassmann-Wachmann (fragment B)

Lis, D. C. and Bockelée-Morvan, D. and Boissier, J. and Crovisier, J. and Biver, N. and Charnley, S. B. (2008) Hydrogen isocyanide in comet 73P/Schwassmann-Wachmann (fragment B). Astrophysical Journal, 675 (1). pp. 931-936. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:LISapj08a

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Abstract

We present a sensitive 3 sigma upper limit of 1.1% for the HNC/HCN abundance ratio in comet 73P/SchwassmannWachmann (fragment B), obtained on 2006 May 10-11, using Caltech Submillimeter Observatory (CSO). This limit is a factor of ~7 lower than the values measured previously in moderately active comets at 1 AU from the Sun. Comet 73P/Schwassmann-Wachmann was depleted in most volatile species, except of HCN. The low HNC/HCN ratio thus argues against HNC production from polymers produced from HCN. However, thermal degradation of macromolecules, or polymers, produced from ammonia and carbon compounds, such as acetylene, methane, or ethane appears a plausible explanation for the observed variations of the HNC/HCN ratio in moderately active comets, including the very low ratio in comet 73P/Schwassmann-Wachmann reported here. Similar polymers have been invoked previously to explain anomalous N-14/N-15 ratios measured in cometary CN.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/527345DOIArticle
http://www.iop.org/EJ/abstract/0004-637X/675/1/931/PublisherArticle
ORCID:
AuthorORCID
Lis, D. C.0000-0002-0500-4700
Additional Information:© 2008 American Astronomical Society. Received 2007 May 4; accepted 2007 November 28. Print publication: Issue 1 (2008 March 1). This research has been supported by NSF grant AST 05-40882 to the Caltech Submillimeter Observatory. D.C.L. acknowledges support from the Observatoire de Paris during his stay in Meudon. S.B.C. acknowledges support from NASA’s Planetary Atmospheres Program. We thank N. Fray for useful discussions and the referee, M. DiSanti, for a thorough and helpful review of the manuscript.
Funders:
Funding AgencyGrant Number
NSFAST 05-40882
Observatoire de ParisUNSPECIFIED
NASAUNSPECIFIED
Subject Keywords:comets: individual (73P/Schwassmann-Wachmann); molecular processes; radio lines: solar system
Issue or Number:1
Record Number:CaltechAUTHORS:LISapj08a
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:LISapj08a
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:12598
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:12 Jan 2009 19:47
Last Modified:03 Oct 2019 00:30

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