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DOI10.1126/science.1204054
EPOXI at comet Hartley 2
A'Hearn M.F.; Belton M.J.S.; Delamere W.A.; Feaga L.M.; Hampton D.; Kissel J.; Klaasen K.P.; McFadden L.A.; Meech K.J.; Jay Melosh H.; Schultz P.H.; Sunshine J.M.; Thomas P.C.; Veverka J.; Wellnitz D.D.; Yeomans D.K.; Besse S.; Bodewits D.; Bowling T.J.; Carcich B.T.; Collins S.M.; Farnham T.L.; Groussin O.; Hermalyn B.; Kelley M.S.; Li J.-Y.; Lindler D.J.; Lisse C.M.; McLaughlin S.A.; Merlin F.; Protopapa S.; Richardson J.E.; Williams J.L.
发表日期2011
ISSN0036-8075
起始页码1396
结束页码1400
卷号332期号:6036
英文摘要Understanding how comets work - what drives their activity - is crucial to the use of comets in studying the early solar system. EPOXI (Extrasolar Planet Observation and Deep Impact Extended Investigation) flew past comet 103P/Hartley 2, one with an unusually small but very active nucleus, taking both images and spectra. Unlike large, relatively inactive nuclei, this nucleus is outgassing primarily because of CO2, which drags chunks of ice out of the nucleus. It also shows substantial differences in the relative abundance of volatiles from various parts of the nucleus.
英文关键词carbon dioxide; ice; volatile agent; carbon dioxide; comet; ice; image analysis; solar system; spectral analysis; volatile substance; article; astronomy; density; extrasolar planet observation and deep impact extended investigation; hartley 2; image analysis; priority journal; space flight; spectroscopy; surface property; topography
语种英语
来源期刊Science
文献类型期刊论文
条目标识符http://gcip.llas.ac.cn/handle/2XKMVOVA/242780
作者单位Department of Astronomy, University of Maryland, College Park, MD 20742-2421, United States; Belton Space Exploration Initiatives LLC, 430 South Randolph Way, Tucson, AZ 85716, United States; Delamere Support Services, 525 Mapleton Avenue, Boulder, CO 80304, United States; Geophysical Institute, University of Alaska-Fairbanks, 903 Koyukuk Drive, Fairbanks, AK 99775-7320, United States; Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany; Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, United States; Code 600, NASA Goddard Space Flight Center, Greenbelt, MD 20771, United States; Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, United States; Lunar and Planetary Library, University of Arizona, 1629 East University Boulevard, Tucson, AZ 85721-0092, United States; Department of Earth and Atmospheric Sciences, Purdue University, 550 Stadium Mall Drive, West Lafayette, IN 47907, United States; Departmen...
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A'Hearn M.F.,Belton M.J.S.,Delamere W.A.,et al. EPOXI at comet Hartley 2[J],2011,332(6036).
APA A'Hearn M.F..,Belton M.J.S..,Delamere W.A..,Feaga L.M..,Hampton D..,...&Williams J.L..(2011).EPOXI at comet Hartley 2.Science,332(6036).
MLA A'Hearn M.F.,et al."EPOXI at comet Hartley 2".Science 332.6036(2011).
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