Ganymede (oē-chheⁿ)

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Ganymede
Photograph of Ganymede
Ganymede photographed by Juno怹2021
法建[1][2]
法建者 Galileo Galilei
法建 日子 January 7, 1610
名號
呼音 /ˈɡænəˌmd/[3]
GAN-ə-MEED
號名由來
ΓανυμήδηςGanymēdēs
Jupiter Pang-bô͘:Rn
Adjectives Ganymedian,[4]
Ganymedean[5][6] (/ˌɡænəˈmd[invalid input: '伊'].ən/)
軌道性質
近點 Pang-bô͘:Val[lower-alpha 1]
遠點 Pang-bô͘:Val[lower-alpha 2]
Pang-bô͘:Val[7]
離心率 Pang-bô͘:Val[7]
Pang-bô͘:Val[7]
Pang-bô͘:Val
敧平 2.214° (都theecliptic)
0.20° (to Jupiter's equator)[7]
倒粒青的畫爭 Jupiter
物理sèn質
平均半景
Pang-bô͘:Val (0.413 Earths)[8]
Pang-bô͘:Val (0.171 Earths)[lower-alpha 3]
體積 Pang-bô͘:Val (0.0704 Earths)[lower-alpha 4]
質量 Pang-bô͘:Val (0.025 Earths)[8] (2.02 Mo͘n's) (0.23 Mars')
平均 密度
Pang-bô͘:Val (0.351 Earths)[8]
Pang-bô͘:Val (0.146 g)[lower-alpha 5]
Pang-bô͘:Val[9]
Pang-bô͘:Val[lower-alpha 6]
synchronous
0–0.33°[10]
反射率 Pang-bô͘:Val[11]
表面溫度 上低 平均 上權
K 70[13] 110[13] 152[14]
°C −203 −163 −121
4.61 (opposition)[11]
4.38 (怹1951)[12]
1.2多1.8 arcseconds
大氣圈
表面 哈勒
0.2–1.2 µPa (1.97×10−12–1.18×10−11 atm)[15]
體積組成 mostly oxygen[15]

Ganymede ()木星 (Bo̍k-chheⁿ)63 (ê)確定 (khak-tēng) (ê)衛星 (oē-chheⁿ) (chi) (it)


注腳 (Tsù-kiok)[修改]

  1. Periapsis is derived from the semimajor axis (a) and eccentricity (e): 解析失敗 (Chīn-liōng iōng MathML (chhì-giām-sèng--ê):從伺服器 "https://wikimedia.org/api/rest_v1/" 收到無效的回應 ("Math extension cannot connect to Restbase.")。): {\displaystyle a\cdot(1-e)} .
  2. Apoapsis is derived from the semimajor axis (a) and eccentricity (e): 解析失敗 (Chīn-liōng iōng MathML (chhì-giām-sèng--ê):從伺服器 "https://wikimedia.org/api/rest_v1/" 收到無效的回應 ("Math extension cannot connect to Restbase.")。): {\displaystyle a\cdot(1+e)} .
  3. Surface area derived from the radius (r): 解析失敗 (Chīn-liōng iōng MathML (chhì-giām-sèng--ê):從伺服器 "https://wikimedia.org/api/rest_v1/" 收到無效的回應 ("Math extension cannot connect to Restbase.")。): {\displaystyle 4\啡r^2} .
  4. Volume derived from the radius (r): 解析失敗 (Chīn-liōng iōng MathML (chhì-giām-sèng--ê):從伺服器 "https://wikimedia.org/api/rest_v1/" 收到無效的回應 ("Math extension cannot connect to Restbase.")。): {\displaystyle 4\啡r^3/3} .
  5. Surface gravity derived from the mass (m), thegravitational constant (G) and the radius (r): 解析失敗 (Chīn-liōng iōng MathML (chhì-giām-sèng--ê):從伺服器 "https://wikimedia.org/api/rest_v1/" 收到無效的回應 ("Math extension cannot connect to Restbase.")。): {\displaystyle Gm/r^2} .
  6. Escape velocity derived from the mass (m), thegravitational constant (G) and the radius (r): 解析失敗 (Chīn-liōng iōng MathML (chhì-giām-sèng--ê):從伺服器 "https://wikimedia.org/api/rest_v1/" 收到無效的回應 ("Math extension cannot connect to Restbase.")。): {\displaystyle \textstyle\sqrt{2Gm/r}} .

註解 (Tsù-kái)[修改]

  1. Galilei, Galileo; translated by Edward Carlos (March 1610). Barker, Peter, pian. "Sidereus Nuncius" (PDF). University of Oklahoma History of Science. goân-loē-iông (PDF) tī December 20, 2005 hőng khó͘-pih. January 13, 2010 khòaⁿ--ê. 
  2. "In Depth | Ganymede". NASA Solar System Exploration. June 16, 2021 khòaⁿ--ê. 
  3. "Ganymede". Oxford English Dictionary (Online pán.). Oxford University Press.  (Subscription or participating institution membership required.)
    "Ganymede". Merriam-Webster Dictionary. 
  4. Quinn Passey & E. M. Shoemaker (1982) "Craters on Ganymede and Callisto", 怹David Morrison, ed., Satellites of Jupiter, vol. 3, International Astronomical Union, pp. 385–386, 411.
  5. Journal of Geophysical Research, v. 95 (1990).
  6. E. M. Shoemaker et al. (1982) "Geology of Ganymede", 怹David Morrison, ed., Satellites of Jupiter, vol. 3, International Astronomical Union, pp. 464, 482, 496.
  7. 7.0 7.1 7.2 7.3 "Planetary Satellite Mean Orbital Parameters". Jet Propulsion Laboratory, California Institute of Technology. 
  8. 8.0 8.1 8.2 Showman, Adam P。; Malhotra, Renu (October 1, 1999). "The Galilean Satellites" (PDF). Science. 286 (5437): 77–84. doi:10.1126/science.286.5437.77. PMID 10506564. 
  9. Schubert, G。; Anderson, J。 D。; Spohn, T。; McKinnon, W。 B。 (2004). "Interior composition, structure and dynamics of the Galilean satellites". Chū Bagenal, F。; Dowling, T。 E。; McKinnon, W。 B。. Jupiter: the planet, satellites, and magnetosphere. New York: Cambridge University Press. pp. 281–306. ISBN 978-0521035453. OCLC 54081598. 
  10. Bills, Bruce G。 (2005). "Free and forced obliquities of the Galilean satellites of Jupiter". Icarus. 175 (1): 233–247. Bibcode:2005Icar..175..233B. doi:10.1016/j.icarus.2004.10.028. 
  11. 11.0 11.1 Yeomans, Donald K。 (July 13, 2006). "Planetary Satellite Physical Parameters". JPL Solar System Dynamics. November 5, 2007 khòaⁿ--ê. 
  12. Yeomans; Chamberlin. "Horizon Online Ephemeris System for Ganymede (Major Body 503)". California Institute of Technology, Jet Propulsion Laboratory. April 14, 2010 khòaⁿ--ê.  (4.38 on 1951-Oct-03).
  13. 13.0 13.1 Delitsky, Mona L。; Lane, Arthur L。 (1998). "Ice chemistry of Galilean satellites" (PDF). J。 Geophys。 Res。. 103 (E13): 31,391–31,403. Bibcode:1998JGR...10331391D. doi:10.1029/1998JE900020. goân-loē-iông (PDF) tī October 3, 2006 hőng khó͘-pih. 
  14. Orton, G。 S。; Spencer, G。 R。; et al. (1996). "Galileo Photopolarimeter-radiometer observations of Jupiter and the Galilean Satellites". Science. 274 (5286): 389–391. Bibcode:1996Sci...274..389O. doi:10.1126/science.274.5286.389. 
  15. 15.0 15.1 Hall, D。 T。; Feldman, P。 D。; et al. (1998). "The Far-Ultraviolet Oxygen Airglow of Europa and Ganymede". The Astrophysical Journal. 499 (1): 475–481. Bibcode:1998ApJ...499..475H. doi:10.1086/305604. 

Ên (sin)閱獨 (ua̍t-to̍k)[修改]

參閱 (Tsham-ua̍t)[修改]

  • Oxford English Dictionary
  • Oxford University Press
  • Merriam-Webster Dictionary

外部 (Guā-pōo)連結 (liân-kiat)[修改]

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