Goe̍h-niû

月娘
	; 佇北美洲看著的月圓
軌道性質
	原其 J2000
近點	362 600 km; (356 400–370 400 km)
遠點	405 400 km; (404 000–406 700 km)
半長車心	Pang-bô͘:ValPang-bô͘:Nbsp(Pang-bô͘:Val)
離心率	Pang-bô͘:Val
軌道週期	Pang-bô͘:Val; (27 d 7 h 43 min 11.5 s)
會合週期	Pang-bô͘:Val; (29 d 12 h 44 min 2.9 s)
平均軌道速力	Pang-bô͘:Val
敧平	5.145° to the ecliptic
升交點的經度	Regressing by one revolution 怹18.61 years
遠點的引數	Progressing by one; revolution怹8.85 years
倒粒青的畫爭	地球
物理sèn質
平均半景	Pang-bô͘:ValPang-bô͘:Nbsp; (Tē-kiû ê 0.2727)
赤道半景	Pang-bô͘:ValPang-bô͘:Nbsp; (Tē-kiû ê 0.2725)
極地半景	Pang-bô͘:ValPang-bô͘:Nbsp; (Tē-kiû ê 0.2731)
扁平率	Pang-bô͘:Val
ÎNN州	Pang-bô͘:ValPang-bô͘:Nbsp(equatorial)
表面積	Pang-bô͘:ValPang-bô͘:Nbsp; (地球的0.074)
體積	Pang-bô͘:ValPang-bô͘:Nbsp; (Tē-kiû ê 0.020)
質量	Pang-bô͘:ValPang-bô͘:Nbsp; (地球的 Pang-bô͘:Val)
平均密度	Pang-bô͘:Val; Pang-bô͘:Val × 地球
表面重力	Pang-bô͘:ValPang-bô͘:Nbsp(Pang-bô͘:Val)
慣性因子的能率	Pang-bô͘:Val
脫走so̍k度	Pang-bô͘:Val
行星自轉週期	Pang-bô͘:ValPang-bô͘:Nbsp(synchronous)
赤道自轉速度	4.627 m/s
車心敧平	Pang-bô͘:Ublist
北極赤經	17h 47m 26s; 266.86°;
北極赤緯	65.64°
反射率	0.136
明顯度	Pang-bô͘:Ublist
角直徑	29.3多34.1 kak-hun
大氣圈
表面哈勒	Pang-bô͘:Ublist
體積組成	彼; Ar; 奶; 焦; K; H; Rn;

區別 (khu-pia̍t): 月 (Goe̍h)嘛是 (mā-sī)一種 (chi̍t-chióng)時間 (sî-kan)的 (ê)單位 (tan-ūi).

月娘 (Goe̍h-niû) (月娘; 英語: mo͘n; thian-bûn hû-hō: )，或者 (he̍k-chiá)月球 (goe̍h-kiû) (月球)，是 (sī)地球 (Tē-kiû)唯一 (î-it)个 (ê)天然 (thian-jiân)衛星 (oē-chheⁿ)。

參照 (Chham-chiàu)[修改]

注跤 (Chù-kha)[修改]

↑ ^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.
↑ Ín-iōng chhò-gō͘: Bû-hāu ê <ref> tag; chhōe bô chí-miâ ê ref bûn-jī 郎2011
↑ 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.
↑ ^4.0 ^4.1 ^4.2 ^4.3 ^4.4 ^4.5 ^4.6 ^4.7 ^4.8 Williams, Dr。 David R。 (2 February 2006). "Mo͘n Fact Sheet". NASA/National Space Science Data Center. Goân-pún bāng-ia̍h Pó-chûn tī 23 March 2010. 31 December 2008 khòaⁿ--ê.
↑ Smith, David E。; Zuber, Maria T。; Neumann, Gregory A。; Lemoine, Frank G。 (1 January 1997). "Topography of推Mo͘n from the Clementine lidar". Journal of Geophysical Research. 102 (E1): 1601. Bibcode:1997JGR...102.1591S. doi:10.1029/96JE02940.
↑ Terry 2013, p. 226.
↑ 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.
↑ ^8.0 ^8.1 Archinal, Brent A。; A'Hearn, Michael F。; Bowell, Edward G。; Conrad, Albert R。; Consolmagno, Guy J。; et al. (2010). "Report of the要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.
↑ Matthews, Grant (2008). "Celestial body irradiance determination from an underfilled satellite radiometer: application to albedo and thermal emission measurements of推Mo͘n using CERES". Applied Optics. 47 (27): 4981–4993. Bibcode:2008ApOpt..47.4981M. doi:10.1364/AO.47.004981. PMID 18806861.
↑ A.R。 Vasavada; D.A。 Paige & S.E。 Wood (1999). "Near-Surface Temperatures on Mercury and推Mo͘n and the Stability of Polar Ice Deposits". Icarus. 141 (2): 179–193. Bibcode:1999Icar..141..179V. doi:10.1006/icar.1999.6175.
↑ Lucey, Paul; Korotev, Randy L.; et al. (2006). "Understanding the lunar surface and space-Mo͘n interactions". Reviews in Mineralogy and Geochemistry. 60 (1): 83–219. Bibcode:2006RvMG...60...83L. doi:10.2138/rmg.2006.60.2.

Ín-iōng chhò-gō͘: 在 <references> 中定義的 <ref> 標籤設定 name 屬性為 "Lang2011"，但在前文中並未使用。

佇Wikimedia Commons等的相關檔案: Mo͘n

Pún 文章 sī chi̍t phiⁿ phí-á-kiáⁿ. Lí thang tàu khok-chhiong lâi pang-chō͘ Wikipedia.

太陽系

青: 日頭
惑星: 水星 \| 金星 \| 地球 \| 火星 \| 木星 \| 土星 \| 天王星 \| 海王星
矮惑星: Ceres \| 明王星 \| Haumea \| Makemake \| Eris
小物體: 小惑星 \| 海王星外星體 \| 長尾青
衛星: 月娘 \| 火星的 \| 木星的 \| 土星的 \| 天王星的 \| 海王星的
陳: 小惑星帶 \| Kuiper帶 \| 散亂圓盤 \| Oort雲
請參考天文物體，太陽系的星體列單，照半徑排猶是照質量排

[W06-1] 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.

[郎2011-2] Ín-iōng chhò-gō͘: Bû-hāu ê <ref> tag; chhōe bô chí-miâ ê ref bûn-jī 郎2011

[Morais2002-3] 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.

[NSSDC-4] 4.0 ^4.1 ^4.2 ^4.3 ^4.4 ^4.5 ^4.6 ^4.7 ^4.8 Williams, Dr。 David R。 (2 February 2006). "Mo͘n 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推Mo͘n from the Clementine lidar". Journal of Geophysical Research. 102 (E1): 1601. Bibcode:1997JGR...102.1591S. doi:10.1029/96JE02940.

[FOOTNOTETerry2013226-6] Terry 2013, p. 226.

[Williams1996-7] 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.

[report-8] 8.0 ^8.1 Archinal, Brent A。; A'Hearn, Michael F。; Bowell, Edward G。; Conrad, Albert R。; Consolmagno, Guy J。; et al. (2010). "Report of the要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.

[Saari-9] Matthews, Grant (2008). "Celestial body irradiance determination from an underfilled satellite radiometer: application to albedo and thermal emission measurements of推Mo͘n using CERES". Applied Optics. 47 (27): 4981–4993. Bibcode:2008ApOpt..47.4981M. doi:10.1364/AO.47.004981. PMID 18806861.

[Vasavada1999-10] A.R。 Vasavada; D.A。 Paige & S.E。 Wood (1999). "Near-Surface Temperatures on Mercury and推Mo͘n and the Stability of Polar Ice Deposits". Icarus. 141 (2): 179–193. Bibcode:1999Icar..141..179V. doi:10.1006/icar.1999.6175.

[L06-11] Lucey, Paul; Korotev, Randy L.; et al. (2006). "Understanding the lunar surface and space-Mo͘n 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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Goe̍h-niû

參照 (Chham-chiàu)[修改]

注跤 (Chù-kha)[修改]

巡覽me-niú

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