木星
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/ˈdʒuːpɪtər/ (![]() | |||||||||||||||
104 | |||||||||||||||
429 | |||||||||||||||
267 | |||||||||||||||
775 0.048 | |||||||||||||||
13.07 | |||||||||||||||
18.818° | |||||||||||||||
100.492° | |||||||||||||||
275.066° | |||||||||||||||
95 (截至2023 | |||||||||||||||
911±6 km 69[6][b] | |||||||||||||||
87±0.00015 0.064 | |||||||||||||||
1.326 g/cm3[3][b] | |||||||||||||||
m/s2 24.79 [3][b] 2.528 g | |||||||||||||||
逃逸 | 59.5 km/s[3][b] | ||||||||||||||
9.925 h[9] (9 h 55 m 30 s) | |||||||||||||||
12.6 km/s 300 km/h 45 | |||||||||||||||
3.13°[3] | |||||||||||||||
268.057° 17 | |||||||||||||||
64.496°[6] | |||||||||||||||
0.343 (Bond) 0.52 (geom.)[3] | |||||||||||||||
| |||||||||||||||
−1.6 | |||||||||||||||
29.8″ | |||||||||||||||
20–200 kPa[10] (cloud layer) | |||||||||||||||
27 km | |||||||||||||||
by volume:
冰: | |||||||||||||||
名
[喺希臘同
形成 同 遷徙
[物理 性質
[成分
[跟質
質量 同大 細
[![see caption](https://upload.wikimedia.org/wikipedia/commons/thumb/9/90/Jupiter_and_Europa_2020.tiff/lossy-page1-220px-Jupiter_and_Europa_2020.tiff.jpg)
內部結構
[![](https://upload.wikimedia.org/wikipedia/commons/thumb/b/b5/Jupiter_diagram.svg/300px-Jupiter_diagram.svg.png)
喺
氦同氖嘅雨
大氣 層
[![](https://upload.wikimedia.org/wikipedia/commons/thumb/a/a3/790106-0203_Voyager_58M_to_31M_reduced.gif/220px-790106-0203_Voyager_58M_to_31M_reduced.gif)
雲 層
[大 紅 斑 同 其他氣 旋
[![](https://upload.wikimedia.org/wikipedia/commons/thumb/c/c8/Jupiter_from_Voyager_1.jpg/250px-Jupiter_from_Voyager_1.jpg)
2000
2017
磁層
[行 星 環
[![](https://upload.wikimedia.org/wikipedia/commons/thumb/2/29/PIA01627_Ringe.jpg/220px-PIA01627_Ringe.jpg)
軌道 和 自轉
[![](https://upload.wikimedia.org/wikipedia/commons/thumb/c/c1/Solar_system_orrery_outer_planets.gif/220px-Solar_system_orrery_outer_planets.gif)
觀測
[探測 史
[1610
1670
![](https://upload.wikimedia.org/wikipedia/commons/thumb/7/75/Portrait_of_Jupiter_from_Cassini.jpg/220px-Portrait_of_Jupiter_from_Cassini.jpg)
1892
1955
1973 |
130,000 | |
1974 |
34,000 | |
1979 |
349,000 | |
1979 |
570,000 | |
1992 |
408,894 | |
2004 |
120,000,000 | |
卡西 |
2000 |
10,000,000 |
2007 |
2,304,535 |
1979
衛星
[伽 利 略 衛星
[佢哋嘅軌
| |||||||||||||||||||||||||||||||||||||||||||||||||||||
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分類
[內側 |
喺內 |
撒米斯圖 |
|
卡普 |
|
帕西 |
文化
[喺
註
[參考
[- ↑ Jupiter, entry in the Oxford English Dictionary, prepared by J. A. Simpson and E. S. C. Weiner, vol. 8, second edition, Oxford: Clarendon Press, 1989. ISBN 0-19-861220-6 (vol. 8), ISBN 0-19-861186-2 (set.)
- ↑ 2.0 2.1 Seligman, Courtney. "Rotation Period and Day Length". 喺2009
年 8月 13號 搵到. - ↑ 3.00 3.01 3.02 3.03 3.04 3.05 3.06 3.07 3.08 3.09 3.10 3.11 3.12 3.13 3.14 3.15 3.16 3.17 Williams, David R. (2004
年 11月16號 ). "Jupiter Fact Sheet". NASA.原著 喺2011年 10月 5號 歸 檔. 喺2007年 8月 8號 搵到. - ↑ "The MeanPlane (Invariable plane) of the Solar System passing through the barycenter". April 3, 2009.
原著 喺2009年 4月 20號 歸 檔. 喺2009年 4月 10號 搵到. (produced with Solex 10 互聯網 檔案館 嘅歸 檔,歸 檔日期 2008年 12月20號 ,. written by Aldo Vitagliano; see also Invariable plane) - ↑ Yeomans, Donald K. (2006
年 7月 13號 ). "HORIZONS Web-Interface for Jupiter Barycenter (Major Body=5)". JPL Horizons On-Line Ephemeris System. 喺2007年 8月 8號 搵到. – Select "Ephemeris Type: Orbital Elements", "Time Span: January 1, 2000 12:00到 2000-01-02". ("Target Body: Jupiter Barycenter" and "Center: Sun" should be defaulted to.) - ↑ 6.0 6.1 6.2 6.3 6.4
本 引用 來 源 將 會 喺幾十 分 鐘 後 自動 完成 。您可以檢 查英文 對應 模 或 手動 擴充 - ↑ "Solar System Exploration: Jupiter: Facts & Figures". NASA. 2008
年 5月 7號 .原著 喺2002年 12月16號 歸 檔. 喺2015年 7月 26號 搵到. - ↑ "Astrodynamic Constants". JPL Solar System Dynamics. 2009
年 2月 27號 . 喺2009年 8月 8號 搵到. - ↑ 9.0 9.1 Seidelmann, P. K.; Abalakin, V. K.; Bursa, M.; Davies, M. E.; de Burgh, C.; Lieske, J. H.; Oberst, J.; Simon, J. L.; Standish, E. M.; Stooke, P.; Thomas, P. C. (2001). "Report of the IAU/IAG Working Group on Cartographic Coordinates and Rotational Elements of the Planets and Satellites: 2000". HNSKY Planetarium Program.
原著 喺2020年 5月 12號 歸 檔. 喺2007年 2月 2號 搵到. - ↑ Anonymous (1983
年 3月 ). "Probe Nephelometer". Galileo Messenger. NASA/JPL (6).原著 喺2009年 7月 19號 歸 檔. 喺2007年 2月 12號 搵到. - ↑ "What Is Jupiter?". NASA. 2014.
原 先 內容歸 檔喺March 18, 2015. 喺April 1, 2015搵到. - ↑ "The biggest single object we can see in our galaxy, with the unaided eye". NASA.
原著 喺2009-06-05歸 檔. 喺2013-09-26搵到. - ↑ Lang, Kenneth R. (2011). The Cambridge Guide to the Solar System (
第 Second版 ). Cambridge University Press. p. 285. ISBN 978-0-521-19857-8. - ↑ 张鹏 (2005
年 ). 〈探 索 太 岁之 谜〉. 《《科 学 画 报》》 (第 11期 ). - ↑ Stuart Ross Taylor (2001). Solar system evolution: a new perspective : an inquiry into the chemical composition, origin, and evolution of the solar system (
第 2nd, illus., revised版 ). Cambridge University Press. p. 208. ISBN 0-521-64130-6. - ↑ Hamilton, Calvin (2015). "The Solar System". solarviews.com.
原 先 內容歸 檔喺April 17, 2015. 喺April 1, 2015搵到. - ↑ 17.0 17.1 17.2 Sheppard, Scott S. "Moons of Jupiter". Earth & Planets Laboratory. Carnegie Institution for Science. 喺December 20, 2022搵到.
- ↑ de Pater, Imke; Showalter, Mark R.; Burns, Joseph A.; Nicholson, Philip D.; Liu, Michael C.; Hamilton, Douglas P.; Graham, James R. (1999-04-01). "Keck Infrared Observations of Jupiter's Ring System near Earth's 1997 Ring Plane Crossing". Icarus (
英文 ). 138 (2). Bibcode:1999Icar..138..214D. doi:10.1006/icar.1998.6068. ISSN 0019-1035.原著 喺2017-02-14歸 檔. 喺2022-11-20搵到.{{cite journal}}
: Unknown parameter|dead-url=
ignored (|url-status=
suggested) (help) - ↑ 19.0 19.1 Chang, Kenneth (December 13, 2017). "The Great Red Spot Descends Deep into Jupiter". The New York Times. 喺December 15, 2017搵到.
- ↑ Rachel Alexander (2015). Myths, Symbols and Legends of Solar System Bodies. New York, NY: Springer. pp. 141–159. doi:10.1007/978-1-4614-7067-0. ISBN 978-1-4614-7066-3.
- ↑ "Naming of Astronomical Objects". International Astronomical Union. 喺2022-03-23搵到.
- ↑ 22.0 22.1 22.2 Kruijer, Thomas S.; Burkhardt, Christoph; Budde, Gerrit; Kleine, Thorsten (June 2017). "Age of Jupiter inferred from the distinct genetics and formation times of meteorites". Proceedings of the National Academy of Sciences. 114 (26): 6712–6716. Bibcode:2017PNAS..114.6712K. doi:10.1073/pnas.1704461114. PMC 5495263. PMID 28607079.
- ↑ D'Angelo, G.; Weidenschilling, S. J.; Lissauer, J. J.; Bodenheimer, P. (2021). "Growth of Jupiter: Formation in disks of gas and solids and evolution to the present epoch". Icarus. 355: 114087. arXiv:2009.05575. Bibcode:2021Icar..35514087D. doi:10.1016/j.icarus.2020.114087. S2CID 221654962.
- ↑ Bosman, A. D.; Cridland, A. J.; Miguel, Y. (December 2019). "Jupiter formed as a pebble pile around the N2 ice line". Astronomy & Astrophysics. 632: 5. arXiv:1911.11154. Bibcode:2019A&A...632L..11B. doi:10.1051/0004-6361/201936827. S2CID 208291392. L11.
- ↑ Walsh, K. J.; Morbidelli, A.; Raymond, S. N.; O'Brien, D. P.; Mandell, A. M. (2011). "A low mass for Mars from Jupiter's early gas-driven migration". Nature. 475 (7355): 206–209. arXiv:1201.5177. Bibcode:2011Natur.475..206W. doi:10.1038/nature10201. PMID 21642961. S2CID 4431823.
- ↑ Raúl O Chametla; Gennaro D’Angelo; Mauricio Reyes-Ruiz; F Javier Sánchez-Salcedo (March 2020). "Capture and migration of Jupiter and Saturn in mean motion resonance in a gaseous protoplanetary disc". Monthly Notices of the Royal Astronomical Society. 492 (4): 6007–6018. arXiv:2001.09235. doi:10.1093/mnras/staa260.
- ↑ Batygin, Konstantin (2015). "Jupiter's decisive role in the inner Solar System's early evolution". Proceedings of the National Academy of Sciences. 112 (14): 4214–4217. arXiv:1503.06945. Bibcode:2015PNAS..112.4214B. doi:10.1073/pnas.1423252112. PMC 4394287. PMID 25831540.
- ↑ Fazekas, Andrew (March 24, 2015). "Observe: Jupiter, Wrecking Ball of Early Solar System". National Geographic.
原 先 內容歸 檔喺March 14, 2017. 喺April 18, 2021搵到. - ↑ Denecke, Edward J. (January 7, 2020). Regents Exams and Answers: Earth Science—Physical Setting 2020. Barrons Educational Series. p. 419. ISBN 978-1-5062-5399-2.
- ↑ Allen, Clabon Walter; Cox, Arthur N. (2000). Allen's Astrophysical Quantities. Springer. pp. 295–296. ISBN 978-0-387-98746-0.
- ↑ Polyanin, Andrei D.; Chernoutsan, Alexei (October 18, 2010). A Concise Handbook of Mathematics, Physics, and Engineering Sciences. CRC Press. p. 1041. ISBN 978-1-4398-0640-1.
- ↑ Guillot, Tristan; Gautier, Daniel; Hubbard, William B (December 1997). "NOTE: New Constraints on the Composition of Jupiter from Galileo Measurements and Interior Models". Icarus. 130 (2): 534–539. arXiv:astro-ph/9707210. Bibcode:1997Icar..130..534G. doi:10.1006/icar.1997.5812. S2CID 5466469.
- ↑ Fran Bagenal, Timothy E. Dowling, William B. McKinnon, William McKinnon,
編 (2006). Jupiter: The Planet, Satellites and Magnetosphere. Cambridge University Press. pp. 59–75. ISBN 0521035457.{{cite book}}
: CS1 maint: multiple names:編者 名 單 (link) - ↑ Vdovichenko, V. D.; Karimov, A. M.; Kirienko, G. A.; Lysenko, P. G.; Tejfel’, V. G.; Filippov, V. A.; Kharitonova, G. A.; Khozhenets, A. P. (2021). "Zonal Features in the Behavior of Weak Molecular Absorption Bands on Jupiter". Solar System Research. 55: 35–46. doi:10.1134/S003809462101010X. S2CID 255069821.
{{cite journal}}
: Check|s2cid=
value (help) - ↑ Kim, S. J.; Caldwell, J.; Rivolo, A. R.; Wagner, R. (1985). "Infrared Polar Brightening on Jupiter III. Spectrometry from the Voyager 1 IRIS Experiment". Icarus. 64 (2): 233–248. Bibcode:1985Icar...64..233K. doi:10.1016/0019-1035(85)90201-5.
- ↑ Gautier, D.; Conrath, B.; Flasar, M.; Hanel, R.; Kunde, V.; Chedin, A.; Scott, N. (1981). "The helium abundance of Jupiter from Voyager". Journal of Geophysical Research. 86 (A10): 8713–8720. Bibcode:1981JGR....86.8713G. doi:10.1029/JA086iA10p08713. hdl:2060/19810016480. S2CID 122314894.
- ↑ 37.0 37.1 Kunde, V. G.; Flasar, F. M.; Jennings, D. E.; Bézard, B.; Strobel, D. F.;
等 (September 10, 2004). "Jupiter's Atmospheric Composition from the Cassini Thermal Infrared Spectroscopy Experiment". Science. 305 (5690): 1582–1586. Bibcode:2004Sci...305.1582K. doi:10.1126/science.1100240. PMID 15319491. S2CID 45296656. 喺April 4, 2007搵到. - ↑ "Solar Nebula Supermarket" (PDF). nasa.gov. 喺2023-07-10搵到.
- ↑ Niemann, H. B.; Atreya, S. K.; Carignan, G. R.; Donahue, T. M.; Haberman, J. A.;
等 (1996). "The Galileo Probe Mass Spectrometer: Composition of Jupiter's Atmosphere". Science. 272 (5263): 846–849. Bibcode:1996Sci...272..846N. doi:10.1126/science.272.5263.846. PMID 8629016. S2CID 3242002. - ↑ 40.0 40.1 von Zahn, U.; Hunten, D. M.; Lehmacher, G. (1998). "Helium in Jupiter's atmosphere: Results from the Galileo probe Helium Interferometer Experiment". Journal of Geophysical Research. 103 (E10): 22815–22829. Bibcode:1998JGR...10322815V. doi:10.1029/98JE00695.
- ↑ 41.0 41.1 Stevenson, David J. (May 2020). "Jupiter's Interior as Revealed by Juno". Annual Review of Earth and Planetary Sciences. 48: 465–489. Bibcode:2020AREPS..48..465S. doi:10.1146/annurev-earth-081619-052855. S2CID 212832169.
原著 喺May 7, 2020歸 檔. 喺2022-03-18搵到. - ↑ Ingersoll, A. P.; Hammel, H. B.; Spilker, T. R.; Young, R. E. (June 1, 2005). "Outer Planets: The Ice Giants" (PDF). Lunar & Planetary Institute.
原 先 內容歸 檔 (PDF)喺2022-10-09. 喺February 1, 2007搵到. - ↑ Hofstadter, Mark (2011), "The Atmospheres of the Ice Giants, Uranus and Neptune" (PDF), White Paper for the Planetary Science Decadal Survey, US National Research Council, pp. 1–2, 喺18 January 2015搵到
- ↑ MacDougal, Douglas W. (2012). "A Binary System Close to Home: How the Moon and Earth Orbit Each Other". Newton's Gravity. Undergraduate Lecture Notes in Physics (
英文 ). Springer New York. pp. 193–211. doi:10.1007/978-1-4614-5444-1_10. ISBN 978-1-4614-5443-4.the barycentre is 743,000 km from the centre of the Sun. The Sun's radius is 696,000 km, so it is 47,000 km above the surface.
- ↑ 45.0 45.1 45.2 45.3 45.4 45.5 Burgess, Eric (1982). By Jupiter: Odysseys to a Giant. New York: Columbia University Press. ISBN 978-0-231-05176-7.
- ↑ Shu, Frank H. (1982). The physical universe: an introduction to astronomy. Series of books in astronomy (
第 12版 ). University Science Books. p. 426. ISBN 978-0-935702-05-7. - ↑ Davis, Andrew M.; Turekian, Karl K. (2005). Meteorites, comets, and planets. Treatise on geochemistry.
第 1卷 . Elsevier. p. 624. ISBN 978-0-08-044720-9. - ↑ Schneider, Jean (2009). "The Extrasolar Planets Encyclopedia: Interactive Catalogue". Paris Observatory.
- ↑ Feng, Fabo; Butler, R. Paul;
等 (August 2022). "3D Selection of 167 Substellar Companions to Nearby Stars". The Astrophysical Journal Supplement Series. 262 (21): 21. arXiv:2208.12720. Bibcode:2022ApJS..262...21F. doi:10.3847/1538-4365/ac7e57. S2CID 251864022. - ↑ Seager, S.; Kuchner, M.; Hier-Majumder, C. A.; Militzer, B. (2007). "Mass-Radius Relationships for Solid Exoplanets". The Astrophysical Journal. 669 (2): 1279–1297. arXiv:0707.2895. Bibcode:2007ApJ...669.1279S. doi:10.1086/521346. S2CID 8369390.
- ↑ How the Universe Works 3.
第 Jupiter: Destroyer or Savior?卷 . Discovery Channel. 2014. - ↑ Guillot, Tristan (1999). "Interiors of Giant Planets Inside and Outside the Solar System" (PDF). Science. 286 (5437): 72–77. Bibcode:1999Sci...286...72G. doi:10.1126/science.286.5437.72. PMID 10506563.
原 先 內容歸 檔 (PDF)喺2022-10-09. 喺2022-04-24搵到. - ↑ Burrows, Adam; Hubbard, W. B.; Lunine, J. I.; Liebert, James (July 2001). "The theory of brown dwarfs and extrasolar giant planets". Reviews of Modern Physics. 73 (3): 719–765. arXiv:astro-ph/0103383. Bibcode:2001RvMP...73..719B. doi:10.1103/RevModPhys.73.719. S2CID 204927572.
Hence the HBMM at solar metallicity and Y
α = 50.25 is 0.07 – 0.074 M☉, ... while the HBMM at zero metallicity is 0.092 M☉ - ↑ von Boetticher, Alexander; Triaud, Amaury H. M. J.; Queloz, Didier; Gill, Sam; Lendl, Monika; Delrez, Laetitia; Anderson, David R.; Collier Cameron, Andrew; Faedi, Francesca; Gillon, Michaël; Gómez Maqueo Chew, Yilen; Hebb, Leslie; Hellier, Coel; Jehin, Emmanuël; Maxted, Pierre F. L.; Martin, David V.; Pepe, Francesco; Pollacco, Don; Ségransan, Damien; Smalley, Barry; Udry, Stéphane; West, Richard (August 2017). "The EBLM project. III. A Saturn-size low-mass star at the hydrogen-burning limit". Astronomy & Astrophysics. 604: 6. arXiv:1706.08781. Bibcode:2017A&A...604L...6V. doi:10.1051/0004-6361/201731107. S2CID 54610182. L6.
- ↑ Bodenheimer, P. (1974). "Calculations of the early evolution of Jupiter". Icarus. 23. 23 (3): 319–325. Bibcode:1974Icar...23..319B. doi:10.1016/0019-1035(74)90050-5.
- ↑ 56.0 56.1 56.2 56.3 56.4 56.5 Elkins-Tanton, Linda T. (2011). Jupiter and Saturn (
修訂 版 ). New York: Chelsea House. ISBN 978-0-8160-7698-7. - ↑ Irwin, Patrick (2003). Giant Planets of Our Solar System: Atmospheres, Composition, and Structure. Springer Science & Business Media. p. 62. ISBN 978-3-540-00681-7.
- ↑ Irwin, Patrick G. J. (2009) [2003]. Giant Planets of Our Solar System: Atmospheres, Composition, and Structure (
第 Second版 ). Springer. p. 4. ISBN 978-3-642-09888-8.the radius of Jupiter is estimated to be currently shrinking by approximately 1 mm/yr
. - ↑ 59.0 59.1 Guillot, Tristan; Stevenson, David J.; Hubbard, William B.; Saumon, Didier (2004). "Chapter 3: The Interior of Jupiter".
出自 Bagenal, Fran; Dowling, Timothy E.; McKinnon, William B. (編 ). Jupiter: The Planet, Satellites and Magnetosphere. Cambridge University Press. ISBN 978-0-521-81808-7. - ↑ Smoluchowski, R. (1971). "Metallic interiors and magnetic fields of Jupiter and Saturn". The Astrophysical Journal. 166: 435. Bibcode:1971ApJ...166..435S. doi:10.1086/150971.
- ↑ Wahl, S. M.; Hubbard, William B.; Militzer, B.; Guillot, Tristan; Miguel, Y.; Movshovitz, N.; Kaspi, Y.; Helled, R.; Reese, D.; Galanti, E.; Levin, S.; Connerney, J. E.; Bolton, S. J. (2017). "Comparing Jupiter interior structure models to Juno gravity measurements and the role of a dilute core". Geophysical Research Letters. 44 (10): 4649–4659. arXiv:1707.01997. Bibcode:2017GeoRL..44.4649W. doi:10.1002/2017GL073160.
- ↑ Shang-Fei Liu;
等 (15 August 2019). "The Formation of Jupiter's Diluted Core by a Giant Impact". Nature. 572 (7769): 355–357. arXiv:2007.08338. Bibcode:2019Natur.572..355L. doi:10.1038/s41586-019-1470-2. PMID 31413376. S2CID 199576704. - ↑ 63.0 63.1 Chang, Kenneth (July 5, 2016). "NASA's Juno Spacecraft Enters Jupiter's Orbit". The New York Times. 喺July 5, 2016搵到.
- ↑ Wall, Mike (May 26, 2017). "More Jupiter Weirdness: Giant Planet May Have Huge, 'Fuzzy' Core". space.com. 喺April 20, 2021搵到.
- ↑ Weitering, Hanneke (January 10, 2018). "'Totally Wrong' on Jupiter: What Scientists Gleaned from NASA's Juno Mission". space.com. 喺February 26, 2021搵到.
- ↑ Trachenko, K.; Brazhkin, V. V.; Bolmatov, D. (March 2014). "Dynamic transition of supercritical hydrogen: Defining the boundary between interior and atmosphere in gas giants". Physical Review E. 89 (3): 032126. arXiv:1309.6500. Bibcode:2014PhRvE..89c2126T. doi:10.1103/PhysRevE.89.032126. PMID 24730809. S2CID 42559818. 032126.
- ↑ Coulter, Dauna. "A Freaky Fluid inside Jupiter?". NASA.
原著 喺2021年 12月9號 歸 檔. 喺8 December 2021搵到. - ↑ Bwaldwin, Emily. "Oceans of diamond possible on Uranus and Neptune". Astronomy Now. 喺8 December 2021搵到.
- ↑ "NASA System Exploration Jupiter". NASA. 喺8 December 2021搵到.
- ↑ Guillot, T. (1999). "A comparison of the interiors of Jupiter and Saturn". Planetary and Space Science. 47 (10–11): 1183–1200. arXiv:astro-ph/9907402. Bibcode:1999P&SS...47.1183G. doi:10.1016/S0032-0633(99)00043-4. S2CID 19024073.
- ↑ Lang, Kenneth R. (2003). "Jupiter: a giant primitive planet". NASA.
原著 喺May 14, 2011歸 檔. 喺January 10, 2007搵到. - ↑ Lodders, Katharina (2004). "Jupiter Formed with More Tar than Ice" (PDF). The Astrophysical Journal. 611 (1): 587–597. Bibcode:2004ApJ...611..587L. doi:10.1086/421970. S2CID 59361587.
原著 (PDF)喺April 12, 2020歸 檔. - ↑ Brygoo, S.; Loubeyre, P.; Millot, M.; Rygg, J. R.; Celliers, P. M.; Eggert, J. H.; Jeanloz, R.; Collins, G. W. (2021). "Evidence of hydrogen−helium immiscibility at Jupiter-interior conditions". Nature. 593 (7860): 517–521. Bibcode:2021Natur.593..517B. doi:10.1038/s41586-021-03516-0. OSTI 1820549. PMID 34040210. S2CID 235217898.
- ↑ Kramer, Miriam (October 9, 2013). "Diamond Rain May Fill Skies of Jupiter and Saturn". Space.com. 喺August 27, 2017搵到.
- ↑ Kaplan, Sarah (August 25, 2017). "It rains solid diamonds on Uranus and Neptune". The Washington Post. 喺August 27, 2017搵到.
- ↑ 76.0 76.1 Guillot, Tristan; Stevenson, David J.; Hubbard, William B.; Saumon, Didier (2004). "The interior of Jupiter".
出自 Bagenal, Fran; Dowling, Timothy E.; McKinnon, William B. (編 ). Jupiter. The planet, satellites and magnetosphere. Cambridge planetary science.第 1卷 . Cambridge, UK: Cambridge University Press. p. 45. Bibcode:2004jpsm.book...35G. ISBN 0-521-81808-7. - ↑ Seiff, A.; Kirk, D.B.; Knight, T.C.D.;
等 (1998). "Thermal structure of Jupiter's atmosphere near the edge of a 5-μ m hot spot in the north equatorial belt". 《Journal of Geophysical Research》. 103 (E10): 22857–22889. Bibcode:1998JGR...10322857S. doi:10.1029/98JE01766. - ↑ Steve Miller, Alan Aylward, George Millward (2005-01-01). "Giant Planet Ionospheres and Thermospheres: The Importance of Ion-Neutral Coupling". Space Science Reviews (
英文 ). 116 (1–2): 319–343. doi:10.1007/s11214-005-1960-4. ISSN 0038-6308.原著 喺2018-06-11歸 檔. 喺2018-04-02搵到.{{cite journal}}
: Unknown parameter|dead-url=
ignored (|url-status=
suggested) (help)CS1 maint: multiple names:作者 名 單 (link) - ↑ Loeffler, Mark J.; Hudson, Reggie L. (March 2018). "Coloring Jupiter's clouds: Radiolysis of ammonium hydrosulfide (NH4SH)" (PDF). Icarus. 302: 418–425. Bibcode:2018Icar..302..418L. doi:10.1016/j.icarus.2017.10.041.
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ignored (|url-status=
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: Unknown parameter|dead-url=
ignored (|url-status=
suggested) (help) - ↑ "Greek Names of the Planets".
原著 喺2010-05-09歸 檔. 喺2012-07-14搵到.In Greek the name of the planet Jupiter is Dias, the Greek name of god Zeus.
{{cite web}}
: Unknown parameter|dead-url=
ignored (|url-status=
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第 10卷 . G. P. Putnam's Sons. p. 300.原著 喺2011-07-22歸 檔. 喺2010-01-08搵到.{{cite book}}
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ignored (|url-status=
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ignored (|url-status=
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: Unknown parameter|dead-url=
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suggested) (help)