Goe̍h-niû

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(Tùi Go̍eh-niû choán--lâi)
跳至導覽 跳至搜尋
khu-pia̍t: Goe̍h mā-sī chi̍t-chióng sî-kan ê tan-ūi.
Goe̍h-niû Goe̍h-miû hû-hō
Àm-sî thiⁿ téng ê Goe̍h-îⁿ
Tī Pak Bí-chiu khòaⁿ--tio̍h ê Goe̍h-îⁿ
Kúi-tō sèng-chit
Epoch J2000
Kīn-tiám 362 600 km
(356 400370 400 km)
Hn̄g-tiám 405 400 km
(404 000406 700 km)
384399 km  (0.00257 AU)[1]
Lî-sim-lu̍t 0.0549[1]
27.321661 d
(27 d 7 h 43 min 11.5 s[1])
29.530589 d
(29 d 12 h 44 min 2.9 s)
1.022 km/s
Khi-pêng 5.145° to the ecliptic[2]
Regressing by one revolution in 18.61 years
Progressing by one
revolution in 8.85 years
Tò lia̍p chheⁿ ê ōe-cheⁿ Tē-kiû[3]
Bu̍t-lí sèn-chit
Pêng-kin poàn-kéng
1737.1 km  
(Tē-kiû ê 0.2727)
[1][4][5]
Chhiah-tō poàn-kéng
1738.1 km  
(Tē-kiû ê 0.2725)
[4]
Ke̍k-tē poàn-kéng
1736.0 km  
(Tē-kiû ê 0.2731)
[4]
Píⁿ-pêⁿ-lu̍t 0.0012[4]
Îⁿ-chiu 10921 km  (equatorial)
3.793×107 km2  
(Tē-kiû ê 0.074)
Thé-chek 2.1958×1010 km3  
(Tē-kiû ê 0.020)[4]
Chit-liōng 7.342×1022 kg  
(Tē-kiû ê 0.012300)[1][4]
[6]
Pêng-kin bi̍t-tō͘
3.344 g/cm3[1][4]
0.606 × Tē-kiû
1.62 m/s2  (0.1654 g)[4]
0.3929±0.0009[7]
2.38 km/s
Hêng-chheⁿ chū-choán chiu-kî
27.321661 d  (synchronous)
Chhiah-tō chū-choán sok-tō͘
4.627 m/s
Pak-ke̍k chhiah-keng
  •  17h 47m 26s
  • 266.86°[9]
Pak-ke̍k chhiah-hūi
65.64°[9]
Albedo 0.136[10]
Piáu-bīn ūn-tō͘ siōng-kē pêng-kin siōng-koân
Chhiah-tō 100 K 220 K 390 K
85°N  150 K 230 K[11]
29.3 to 34.1 kak-hun[4]
Tāi-khì-khoan[12]
Piáu-bīn ap-le̍k
  • 10−7 Pa (1 picobar)  (ē-chá)
  • 10−10 Pa (1 femtobar)   
    (ē-àm)
Thé-chek cho͘-sêng

Goe̍h-niû (月娘; Eng: moon), he̍k-chiá goe̍h-kiû (月球), sī Tē-kiû î-it ê thian-jiân oē-chheⁿ.

Chham-chiàu[siu-kái | kái goân-sú-bé]

Chù-kha[siu-kái | kái goân-sú-bé]

  1. 1.0 1.1 1.2 1.3 1.4 1.5 Wieczorek, 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. 2.0 2.1 Lang, Kenneth R. (2011), The Cambridge Guide to the Solar System Archived 1 January 2016 at the Wayback 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. 4.0 4.1 4.2 4.3 4.4 4.5 4.6 4.7 4.8 4.9 Williams, Dr. David R. (2 February 2006). "Moon Fact Sheet". NASA/National Space Science Data Center. Goân-pún bāng-ia̍h Pó-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", in The Moon, volume 2, issue 3, pp. 293-308, doi:10.1007/BF00561882, BibCode: 1971Moon....2..293M
  9. 9.0 9.1 Archinal, 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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Wikimedia Commons téng ê siong-koan tóng-àn: Moon

Thài-iông-hē
Eight Planets.png
Chheⁿ: Ji̍t-thâu
He̍k-chheⁿ: Chúi-chheⁿ | Kim-chheⁿ | Tē-kiû | Hoé-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-khó thian-bûn bu̍t-thé, thài-iông-hē ê chheⁿ-thé lia̍t-toaⁿ, chiàu poàⁿ-kèng pâi iah sī chiàu chit-liōng pâi