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Sublimation from icy jets as a probe of the interstellar volatile content of comets

Blake, Geoffrey A. and Qi, C. and Hogerheijde, Michiel R. and Gurwell, M. A. and Muhleman, D. O. (1999) Sublimation from icy jets as a probe of the interstellar volatile content of comets. Nature, 398 (6724). pp. 213-216. ISSN 0028-0836. http://resolver.caltech.edu/CaltechAUTHORS:20120914-080828318

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Abstract

Comets are some of the most primitive bodies left over from the Solar System's early history. They may preserve both interstellar material and material from the proto-solar nebula, and so studies of their volatile components can provide clues about the evolution of gases and ices, as a collapsing molecular cloud transforms into a mature planetary system. Previous observations of emission from rotational transitions in molecules have averaged over large areas of the inner coma, and therefore include both molecules that sublimed from the nucleus and those that result from subsequent chemical processes in the coma. Here we present high-resolution observations of emission from the molecules HNC, DCN and HDO associated with comet Hale–Bopp. Our data reveal arc-like structures—icy jets—offset from (but close to) the nucleus. The measured abundance ratios on 1–3" scales are substantially different from those on larger scales, and cannot be accounted for by models of chemical processes in the coma; they are, however, similar to the values observed in the cores of dense interstellar clouds and young stellar objects. We therefore propose that sublimation from millimetre-sized icy grains ejected from the nucleus provides access to relatively unaltered volatiles. The D/H ratios inferred from our data suggest that, by mass, Hale–Bopp (and by inference the outer regions of the early solar nebula) consists of ≥15–40% of largely unprocessed interstellar material.


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http://dx.doi.org/10.1038/18372DOIUNSPECIFIED
http://www.nature.com/nature/journal/v398/n6724/abs/398213a0.htmlPublisherUNSPECIFIED
Additional Information:© 1999 Macmillan Magazines Ltd. Received 28 October 1998; accepted 27 January 1999. We thank the staff at OVRO and D. K. Yeomans at JPL for support of our Hale-Bopp observations. The OVRO Millimeter Array is operated by the California Institute of Technology under funding from the US NSF. M.R.H. was supported by the Miller Institute for Basic Research in Science. G.A.B. was a Visiting Fellow at the University of Colorado; additional support to G.A.B. from the NASA Exobiology and Origins of Solar Systems programs is acknowledged.
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Miller Institute for Basic Research in ScienceUNSPECIFIED
NASA Exobiology and Origins of Solar SystemsUNSPECIFIED
Record Number:CaltechAUTHORS:20120914-080828318
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20120914-080828318
Official Citation:Sublimation from icy jets as a probe of the interstellar volatile content of comets p213 Geoffrey A. Blake, C. Qi, Michiel R. Hogerheijde, M. A. Gurwell and D. O. Muhleman doi:10.1038/18372
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:34079
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:14 Sep 2012 15:51
Last Modified:14 Sep 2012 15:51

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