Goe̍h-niû
Guā-māu
- khu-pia̍t: Goe̍h mā-sī chi̍t-chióng sî-kan ê tan-ūi.
Tī Pak Bí-chiu khòaⁿ--tio̍h ê Goe̍h-îⁿ | |||||||||||||
Kúi-tō sèng-chit | |||||||||||||
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Goân-kî J2000 | |||||||||||||
Kīn-tiám |
362 600 km (356 400–370 400 km) | ||||||||||||
Hn̄g-tiám |
405 400 km (404 000–406 700 km) | ||||||||||||
399 km 384 (57 AU) 0.002[1] | |||||||||||||
Lî-sim-lu̍t | 0.0549[1] | ||||||||||||
589 d 29.530 (29 d 12 h 44 min 2.9 s) | |||||||||||||
Pêng-kin kúi-tō sok-le̍k | km/s 1.022 | ||||||||||||
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 |
737.1 km 1 (Tē-kiû ê 0.2727)[1][4][5] | ||||||||||||
Chhiah-tō poàn-kéng |
738.1 km 1 (Tē-kiû ê 0.2725)[4] | ||||||||||||
Ke̍k-tē poàn-kéng |
736.0 km 1 (Tē-kiû ê 0.2731)[4] | ||||||||||||
Píⁿ-pêⁿ-lu̍t | 0.0012[4] | ||||||||||||
Îⁿ-chiu | 921 km 10 (equatorial) | ||||||||||||
×107 km2 3.793 (Tē-kiû ê 0.074) | |||||||||||||
Thé-chek |
×1010 km3 2.1958 (Tē-kiû ê 0.020)[4] | ||||||||||||
Chit-liōng |
×1022 kg 7.342 (Tē-kiû ê 300) 0.012[1][4] [6] | ||||||||||||
Pêng-kin bi̍t-tō͘ |
g/cm3 3.344 [1][4] × Tē-kiû 0.606 | ||||||||||||
m/s2 1.62 (g) 0.1654 [4] | |||||||||||||
±0.0009 0.3929[7] | |||||||||||||
km/s 2.38 | |||||||||||||
Hêng-chheⁿ chū-choán chiu-kî | 661 d 27.321 (synchronous) | ||||||||||||
Chhiah-tō chū-choán sok-tō͘ | 4.627 m/s | ||||||||||||
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Pak-ke̍k chhiah-keng |
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Pak-ke̍k chhiah-hūi | 65.64°[9] | ||||||||||||
Hoán-siā-lu̍t | 0.136[10] | ||||||||||||
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29.3 to 34.1 kak-hun[4] | |||||||||||||
Tāi-khì-khoan[12] | |||||||||||||
Piáu-bīn ap-le̍k | |||||||||||||
Thé-chek cho͘-sêng | |||||||||||||
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Goe̍h-niû (月娘; Eng-gí: moon; thian-bûn hû-hō: ), he̍k-chiá goe̍h-kiû (月球), sī Tē-kiû î-it ê thian-jiân oē-chheⁿ.
Chham-chiàu
[siu-kái | kái goân-sí-bé]Chù-kha
[siu-kái | kái goân-sí-bé]- ↑ 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.
- ↑ 2.0 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.
- ↑ 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.
- ↑ 4.00 4.01 4.02 4.03 4.04 4.05 4.06 4.07 4.08 4.09 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.
- ↑ 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.
- ↑ 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.
- ↑ 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
- ↑ 9.0 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.
- ↑ 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.
- ↑ 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.
- ↑ 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.
Pún bûn-chiuⁿ sī chi̍t phiⁿ phí-á-kiáⁿ. Lí thang tàu khok-chhiong lâi pang-chō͘ Wikipedia. |
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Thài-iông-hē |
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Chheⁿ: Ji̍t-thâu |
He̍k-chheⁿ: Chúi-chheⁿ | Kim-chheⁿ | Tē-kiû | Hóe-chheⁿ | Bo̍k-chheⁿ | Thó͘-chheⁿ | Thian-ông-chheⁿ | Hái-ông-chheⁿ |
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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 |
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