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Surface photometry of comet P/Encke

Djorgovski, S. and Spinrad, Hyron (1985) Surface photometry of comet P/Encke. Astronomical Journal, 90 (5). pp. 869-876. ISSN 0004-6256. doi:10.1086/113795. https://resolver.caltech.edu/CaltechAUTHORS:20190731-080907206

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Abstract

We have developed a scheme to clean cometary digital images from offending background-star trails, and applied this technique to a pair of deep Kitt Peak 4-m plates of comet P/Encke, taken in October 1980. Simultaneous and subsequent digital spectra have been obtained at Lick Observatory. The non-polluted coma images show a strong asymmetric sunward-oriented fan/jet, and an extended and rounder (mostly gaseous) main coma, out to ~ 10^5 km radius. The stellar-trail point-spread function has a narrow width (σ7~0.6 arcsec), so that spatial resolution better than ~300 km is achieved at the comet. The photometric gradient near the nucleus is very steep, strongly suggesting an icy-grain component which evaporates quickly (at radii ⩽ 500 km) in the sunlight. Further from the nucleus, the profile becomes shallower, bluer, and more gas dominated. The effect of solar radiation pressure on C_2, CN, and other molecules is probably responsible for the rounding of the outer, faint isophotes. The source of the molecules is likely to be larger than the nucleus itself, and a substantial fraction may originate in the jet. The technique described here may also be applicable in surface photometry of galaxies, in cases where the heavy image pollution by foreground stars is present.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1086/113795DOIArticle
ORCID:
AuthorORCID
Djorgovski, S.0000-0002-0603-3087
Additional Information:© 1985 American Astronomical Society. Provided by the NASA Astrophysics Data System. Received 27 December 1984. We would like to thank to Dr. J. Stauffer for help with the Kitt Peak observations. We acknowledge valuable discussions with Drs. Z. Sekanina, M. Manner, and D. Schleicher. Dr. Z. Sekanina provided most valuable comments and critical reading of the manuscript. H. S. has been supported by the grants from NSF, NASA, and the California Space Institute. S. D. has been supported in part by the University of California Moore and Regents Fellowships.
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Funding AgencyGrant Number
NSFUNSPECIFIED
NASAUNSPECIFIED
California Space InstituteUNSPECIFIED
University of California, BerkeleyUNSPECIFIED
Issue or Number:5
DOI:10.1086/113795
Record Number:CaltechAUTHORS:20190731-080907206
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190731-080907206
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:97543
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:31 Jul 2019 15:23
Last Modified:16 Nov 2021 17:32

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