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EPOXI: Comet 103P/Hartley 2 Observations from a Worldwide Campaign
Stockholm University, Faculty of Science, Department of Astronomy.
Stockholm University, Faculty of Science, Department of Astronomy.
2011 (English)In: Astrophysical Journal, ISSN 0004-637X, E-ISSN 1538-4357, Vol. 734, no L1, 1-9 p.Article in journal (Refereed) Published
Abstract [en]

Earth- and space-based observations provide synergistic information for space mission encounters by providing data over longer timescales, at different wavelengths and using techniques that are impossible with an in situ flyby. We report here such observations in support of the EPOXI spacecraft flyby of comet 103P/Hartley 2. The nucleus is small and dark, and exhibited a very rapidly changing rotation period. Prior to the onset of activity, the period was ~16.4 hr. Starting in 2010 August the period changed from 16.6 hr to near 19 hr in December. With respect to dust composition, most volatiles and carbon and nitrogen isotope ratios, the comet is similar to other Jupiter-family comets. What is unusual is the dominance of CO2-driven activity near perihelion, which likely persists out to aphelion. Near perihelion the comet nucleus was surrounded by a large halo of water-ice grains that contributed significantly to the total water production.

Place, publisher, year, edition, pages
London: IOP , 2011. Vol. 734, no L1, 1-9 p.
Keyword [en]
comets: individual (103P/Hartley 2)
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:su:diva-57823DOI: 10.1088/2041-8205/734/1/L1OAI: oai:DiVA.org:su-57823DiVA: diva2:418209
Available from: 2011-05-20 Created: 2011-05-20 Last updated: 2017-12-11Bibliographically approved

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