GSTDTAP  > 地球科学
DOI10.1126/science.aal2108
Jupiter's interior and deep atmosphere: The initial pole-to-pole passes with the Juno spacecraft
Bolton, S. J.1; Adriani, A.2; Adumitroaie, V.3; Allison, M.4; Anderson, J.1; Atreya, S.5; Bloxham, J.6; Brown, S.3; Connerney, J. E. P.7,8; DeJong, E.3; Folkner, W.3; Gautier, D.3,9; Grassi, D.2; Gulkis, S.3; Guillot, T.10; Hansen, C.11; Hubbard, W. B.12; Iess, L.13; Ingersoll, A.14; Janssen, M.3; Jorgensen, J.15; Kaspi, Y.16; Levin, S. M.3; Li, C.14; Lunine, J.17; Miguel, Y.10; Mura, A.2; Orton, G.3; Owen, T.18; Ravine, M.19; Smith, E.3; Steffes, P.20; Stone, E.14; Stevenson, D.14; Thorne, R.21; Waite, J.1; Durante, D.13; Ebert, R. W.1; Greathouse, T. K.1; Hue, V.1; Parisi, M.3; Szalay, J. R.1; Wilson, R.22
2017-05-26
发表期刊SCIENCE
ISSN0036-8075
EISSN1095-9203
出版年2017
卷号356期号:6340页码:821-825
文章类型Article
语种英语
国家USA; Italy; France; Denmark; Israel
英文摘要

On 27 August 2016, the Juno spacecraft acquired science observations of Jupiter, passing less than 5000 kilometers above the equatorial cloud tops. Images of Jupiter's poles show a chaotic scene, unlike Saturn's poles. Microwave sounding reveals weather features at pressures deeper than 100 bars, dominated by an ammonia-rich, narrow low-latitude plume resembling a deeper, wider version of Earth's Hadley cell. Near-infrared mapping reveals the relative humidity within prominent downwelling regions. Juno's measured gravity field differs substantially from the last available estimate and is one order of magnitude more precise. This has implications for the distribution of heavy elements in the interior, including the existence and mass of Jupiter's core. The observed magnetic field exhibits smaller spatial variations than expected, indicative of a rich harmonic content.


领域地球科学 ; 气候变化 ; 资源环境
收录类别SCI-E
WOS记录号WOS:000401957900033
WOS关键词MAGNETIC-FIELD ; HYDROGEN ; ABUNDANCE ; IMAGES ; MODELS ; STATE
WOS类目Multidisciplinary Sciences
WOS研究方向Science & Technology - Other Topics
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引用统计
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/196131
专题地球科学
资源环境科学
气候变化
作者单位1.Southwest Res Inst San Antonio, San Antonio, TX 78238 USA;
2.Natl Inst Astrophys, Inst Space Astrophys & Planetol, I-00133 Rome, Italy;
3.CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA;
4.Goddard Inst Space Studies, New York, NY 10025 USA;
5.Univ Michigan, Ann Arbor, MI 48109 USA;
6.Harvard Univ, Cambridge, MA 02138 USA;
7.Space Res Corp, Annapolis, MD 21403 USA;
8.NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA;
9.Observat Paris, Lab Etud Spati & Instrumentat Astrophys, F-92195 Meudon, France;
10.Univ Cote Azur, Lab Lagrange, Observat Cote Azur, CNRS, F-06304 Nice, France;
11.Planetary Sci Inst, Tucson, AZ 85719 USA;
12.Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA;
13.Sapienza Univ Rome, I-00185 Rome, Italy;
14.CALTECH, Pasadena, CA 91125 USA;
15.Tech Univ Denmark, Nat Space Inst, DK-2800 Lyngby, Denmark;
16.Weizmann Inst Sci, Dept Earth & Planetary Sci, IL-76100 Rehovot, Israel;
17.Cornell Univ, Ithaca, NY 14853 USA;
18.Univ Hawaii Manoa, Inst Astron, Honolulu, HI 96822 USA;
19.Malin Space Sci Syst, San Diego, CA 92121 USA;
20.Georgia Inst Technol Atlanta, Ctr Space Technol & Res, Atlanta, GA 30332 USA;
21.Univ Calif Los Angeles, Dept Atmospher Ocean Sci, Los Angeles, CA 90095 USA;
22.Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO 80303 USA
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Bolton, S. J.,Adriani, A.,Adumitroaie, V.,et al. Jupiter's interior and deep atmosphere: The initial pole-to-pole passes with the Juno spacecraft[J]. SCIENCE,2017,356(6340):821-825.
APA Bolton, S. J..,Adriani, A..,Adumitroaie, V..,Allison, M..,Anderson, J..,...&Wilson, R..(2017).Jupiter's interior and deep atmosphere: The initial pole-to-pole passes with the Juno spacecraft.SCIENCE,356(6340),821-825.
MLA Bolton, S. J.,et al."Jupiter's interior and deep atmosphere: The initial pole-to-pole passes with the Juno spacecraft".SCIENCE 356.6340(2017):821-825.
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