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WikipediaChū-iû ê Pek-kho-choân-su
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Goe̍h-niû

Wikipedia (chū-iû ê pek-kho-choân-su) beh kā lí kóng...
khu-pia̍t:Goe̍h mā-sī chi̍t-chióng sî-kan ê tan-ūi.
Goe̍h-niûGoe̍h-miû hû-hō
Àm-sî thiⁿ téng ê Goe̍h-îⁿ
Tī Pak Bí-chiu khòaⁿ--tio̍h êGoe̍h-îⁿ
Kúi-tō sèng-chit
Goân-kîJ2000
Kīn-tiám362600 km
(356400–370400 km)
Hn̄g-tiám405400 km
(404000–406700 km)
7008384399000000000♠384399 km  (7008384466527698999♠0.00257 AU)[1]
Lî-sim-lu̍t6998549000000000000♠0.0549[1]
7006236059151040000♠27.321661 d
(27 d 7 h 43 min 11.5 s[1])
7006255144288960000♠29.530589 d
(29 d 12 h 44 min 2.9 s)
7003102200000000000♠1.022 km/s
Khi-pêng5.145° to theecliptic[2]
Regressing by onerevolution in 18.61 years
Progressing by one
revolution in 8.85 years
Tò lia̍p chheⁿ ê ōe-cheⁿTē-kiû[3]
Bu̍t-lí sèn-chit
Pêng-kin poàn-kéng
7006173710000000000♠1737.1 km  
(Tē-kiû ê 0.2727)[1][4][5]
Chhiah-tō poàn-kéng
7006173810000000000♠1738.1 km  
(Tē-kiû ê 0.2725)[4]
Ke̍k-tē poàn-kéng
7006173600000000000♠1736.0 km  
(Tē-kiû ê 0.2731)[4]
Píⁿ-pêⁿ-lu̍t6997119999999999999♠0.0012[4]
Îⁿ-chiu7007109210000000000♠10921 km  (equatorial)
7013379300000000000♠3.793×107 km2  
(Tē-kiû ê 0.074)
Thé-chek7019219580000000000♠2.1958×1010 km3  
(Tē-kiû ê 0.020)[4]
Chit-liōng7022734200000000000♠7.342×1022 kg  
(Tē-kiû ê6998123000000000000♠0.012300)[1][4][6]
Pêng-kinbi̍t-tō͘
7003334400000000000♠3.344 g/cm3[1][4]
6999606000000000000♠0.606 × Tē-kiû
7000162000000000000♠1.62 m/s2  (6999165400000000000♠0.1654 g)[4]
6999392900000000000♠0.3929±0.0009[7]
7003238000000000000♠2.38 km/s
7006236059151040000♠27.321661 d  (synchronous)
Chhiah-tō chū-choán sok-tō͘
4.627 m/s
Pak-ke̍kchhiah-keng
  • 17h 47m 26s
  • 266.86°[9]
Pak-ke̍kchhiah-hūi
65.64°[9]
Hoán-siā-lu̍t0.136[10]
Piáu-bīnun-tō͘siōng-kēpêng-kinsiōng-koân
Chhiah-tō100K220 K390 K
85°N 150 K230 K[11]
29.3 to 34.1kak-hun[4]
Tāi-khì-khoan[12]
Piáu-bīnap-le̍k
  • 10−7Pa (1picobar)  (ē-chá)
  • 10−10 Pa (1 femtobar)  
    (ē-àm)
Thé-chek cho͘-sêng

Goe̍h-niû (月娘;Eng-gí:moon; thian-bûn hû-hō:☾), he̍k-chiágoe̍h-kiû (月球), sīTē-kiû î-it ê thian-jiânoē-chheⁿ.

Chham-chiàu

[siu-kái |kái goân-sí-bé]

Chù-kha

[siu-kái |kái goân-sí-bé]
  1. ↑1.01.11.21.31.41.5Wieczorek, Mark A.; et al. (2006). "The constitution and structure of the lunar interior".Reviews in Mineralogy and Geochemistry.60 (1): 221–364.Bibcode:2006RvMG...60..221W.doi:10.2138/rmg.2006.60.3. 
  2. ↑2.02.1Lang, Kenneth R. (2011),The Cambridge Guide to the Solar SystemArchived 1 January 2016 at theWayback Machine., 2nd ed., Cambridge University Press.
  3. ↑Morais, M.H.M.; Morbidelli, A. (2002). "The Population of Near-Earth Asteroids in Coorbital Motion with the Earth".Icarus.160 (1): 1–9.Bibcode:2002Icar..160....1M.doi:10.1006/icar.2002.6937. 
  4. ↑4.004.014.024.034.044.054.064.074.084.09Williams, Dr. David R. (2 February 2006)."Moon Fact Sheet". NASA/National Space Science Data Center. Goân-pún bāng-ia̍hPó-chûn tī 23 March 2010.31 December 2008 khòaⁿ--ê. 
  5. ↑Smith, David E.; Zuber, Maria T.; Neumann, Gregory A.; Lemoine, Frank G. (1 January 1997). "Topography of the Moon from the Clementine lidar".Journal of Geophysical Research.102 (E1): 1601.Bibcode:1997JGR...102.1591S.doi:10.1029/96JE02940. 
  6. ↑Terry 2013, p. 226.
  7. ↑Williams, James G.; Newhall, XX; Dickey, Jean O. (1996). "Lunar moments, tides, orientation, and coordinate frames".Planetary and Space Science.44 (10): 1077–1080.Bibcode:1996P&SS...44.1077W.doi:10.1016/0032-0633(95)00154-9. 
  8. ↑Makemson, Maud W. (1971);"Determination of Selenographic Positions", inThe Moon, volume 2, issue 3, pp. 293-308,doi:10.1007/BF00561882, BibCode: 1971Moon....2..293M
  9. ↑9.09.1Archinal, Brent A.; A'Hearn, Michael F.; Bowell, Edward G.; Conrad, Albert R.; Consolmagno, Guy J.; et al. (2010)."Report of the IAU Working Group on Cartographic Coordinates and Rotational Elements: 2009"(PDF).Celestial Mechanics and Dynamical Astronomy.109 (2): 101–135.Bibcode:2011CeMDA.109..101A.doi:10.1007/s10569-010-9320-4.goân-loē-iông(PDF) tī 4 March 2016 hőng khó͘-pih.24 September 2018 khòaⁿ--ê. 
  10. ↑Matthews, Grant (2008). "Celestial body irradiance determination from an underfilled satellite radiometer: application to albedo and thermal emission measurements of the Moon using CERES".Applied Optics.47 (27): 4981–4993.Bibcode:2008ApOpt..47.4981M.doi:10.1364/AO.47.004981.PMID 18806861. 
  11. ↑A.R. Vasavada; D.A. Paige & S.E. Wood (1999). "Near-Surface Temperatures on Mercury and the Moon and the Stability of Polar Ice Deposits".Icarus.141 (2): 179–193.Bibcode:1999Icar..141..179V.doi:10.1006/icar.1999.6175. 
  12. ↑Lucey, Paul; Korotev, Randy L.; et al. (2006). "Understanding the lunar surface and space-Moon interactions".Reviews in Mineralogy and Geochemistry.60 (1): 83–219.Bibcode:2006RvMG...60...83L.doi:10.2138/rmg.2006.60.2. 

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Bu̍t-lí ê te̍k-sèng
Goe̍h-niû ê kúi-tō
Goe̍h-niû ê piáu-bīn
Goe̍h-niû ê kho-ha̍k
Goe̍h-niû ê thàm-chhek
HāmTē-kiû ê koan-hē
Le̍k-hoat kap bûn-hoà
Thài-iông-hē
Chheⁿ:Ji̍t-thâu
He̍k-chheⁿ:Chúi-chheⁿ |Kim-chheⁿ |Tē-kiû |Hóe-chheⁿ |Bo̍k-chheⁿ |Thó͘-chheⁿ |Thian-ông-chheⁿ |Hái-ông-chheⁿ
É-he̍k-chheⁿ:Ceres |Mê-ông-chheⁿ |Haumea |Makemake |Eris
Sió-bu̍t-thé:Sió-he̍k-chheⁿ |Hái-ông-chheⁿ goā chheⁿ-thé |Tn̂g-boé-chheⁿ
Oē-chheⁿ:Goe̍h-niû |Hoé-chheⁿ ê |Bo̍k-chheⁿ ê |Thó͘-chheⁿ ê |Thian-ông-chheⁿ ê |Hái-ông-chheⁿ ê
Tīn:Sió-he̍k-chheⁿ-toà |Kuiper-toà |Sàn-loān îⁿ-poâⁿ |Oort-hûn
Chhiáⁿ chham-khóthian-bûn bu̍t-thé,thài-iông-hē êchheⁿ-thé lia̍t-toaⁿ, chiàupoàⁿ-kèng pâi iah sī chiàuchit-liōng pâi
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