Sökning: WFRF:(Vidal M) > (2010-2014) > EPOXI: Comet 103P/H...
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000 | 09542naa a2202689 4500 | |
001 | oai:research.chalmers.se:ae4f0d6c-c8d6-4757-8549-3669c6f50cad | |
003 | SwePub | |
008 | 171007s2011 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:su-57823 | |
024 | 7 | a https://research.chalmers.se/publication/1420672 URI |
024 | 7 | a https://doi.org/10.1088/2041-8205/734/1/L12 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-578232 URI |
040 | a (SwePub)cthd (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a art2 swepub-publicationtype |
072 | 7 | a ref2 swepub-contenttype |
100 | 1 | a Meech, K. J.4 aut |
245 | 1 0 | a EPOXI: Comet 103P/Hartley 2 Observations from a Worldwide Campaign |
264 | 1 | a London :b IOP,c 2011 |
520 | a 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 CO 2 -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. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
653 | a comets: individual (103P/Hartley 2) | |
653 | a Astronomy and astrophysics | |
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710 | 2 | a Stockholms universitetb Institutionen för astronomi4 org |
773 | 0 | t Astrophysical Journal Lettersd London : IOPg 734:L1, s. 1-9q 734:1x 2041-8213x 2041-8205 |
773 | 0 | t Astrophysical Journald London : IOPg 734:L1, s. 1-9q 734:L1<1-9x 0004-637Xx 1538-4357 |
856 | 4 | u http://dx.doi.org/10.1088/2041-8205/734/1/L1y FULLTEXT |
856 | 4 8 | u https://research.chalmers.se/publication/142067 |
856 | 4 8 | u https://doi.org/10.1088/2041-8205/734/1/L1 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-57823 |
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