1 Ceres (hû-hō: [17] 是 ( sī ) 粒 ( lia̍p ) 踮 ( tiàm ) 佇 ( tī ) 小惑星帶 ( sió-he̍k-chheⁿ-toà ) 的 ( ê ) 矮惑星 ( é-he̍k-chheⁿ ) 發現人 ( hoat-hiān-jîn ) Giuseppe Piazzi ，佇1801年 ( nî ) 。Ceres 是羅馬 ( Lô-má ) 查某 ( cha-bó͘ ) 神明 ( sîn-bêng ) 名 ( miâ )
19世紀 ( sè-kí ) 侵 ( chhím ) 發現 ( hoat-hiān ) 時 ( sî ) 人 ( lâng ) 掠準 ( lia̍h-chún ) 伊 ( i ) 和 ( hām ) 其他 ( kî-thaⁿ ) 惑星 ( he̍k-chheⁿ ) 相 ( sio ) 所以 ( só͘-í ) 共 ( kā ) 當做 ( tòng-chò ) 惑星 。尾仔 ( Boé--á ) 卡 ( khah ) 了解 ( liáu-kái ) 性質 ( sèng-chit ) 了後 ( liáu-aū ) 就 ( tō ) 列 ( lia̍t ) 做 ( chò ) 小惑星 ( sió-he̍k-chheⁿ ) 雖罔 ( Sui-bóng ) 直徑 ( ti̍t-kèng ) 才 ( chiah ) km ，伊實在 ( si̍t-chāi ) 太陽系 ( Thài-iông-hē ) 萬 ( bān ) 當中 ( tang-tiong ) 上 ( siōng ) 蓋 ( kài ) 大 ( toā ) 質量 ( chit-liōng ) 濟 ( chē ) 形 ( hêng ) 象 ( siōng ) îⁿ 的1粒，會使 ( ē-sái ) 講 ( kóng ) 小惑星帶 有 ( ū ) 份 ( hūn ) 个 ( ê ) 遐 ( hia ) 因為 ( In-ūi ) 按呢 ( án-ne ) 月 ( goe̍h ) 天文學界 ( thian-bûn-ha̍k-kài ) 閣 ( koh ) 改 ( kái ) 熱 ( lia̍t ) 矮惑星 "。
註釋 ( Tsù-sik ) [ 修改 ]
↑ The value given for Ceres is the mean moment of inertia, which is thought to better represent its interior structure than the polar moment of inertia, due to its high polar flattening.[8]
註解 ( Tsù-kái ) [ 修改 ]
↑ Schmadel, Lutz (2003). Dictionary of minor planet names ISBN 978-3540002383 . goân-loē-iông tī 16 February 2021 hőng khó͘-pih. 21 January 2021 khòaⁿ--ê . ↑ "On推New Planet Ceres" . A Journal of Natural Philosophy, Chemistry, and the Arts (ēng Eng-gí). 1802. goân-loē-iông tī 29 May 2022 hőng khó͘-pih. 29 May 2022 khòaⁿ--ê . ↑ Souami, D。; Souchay, J。 (July 2012). "The solar system's invariable plane". Astronomy & Astrophysics . 543 : 11. Bibcode :2012A&A...543A.133S . doi :10.1051/0004-6361/201219011 . A133. ↑ 4.0 4.1 4.2 4.3 4.4 4.5 4.6 引用錯誤: 無效的 <ref> tag;
揣無指名的ref文字 jpl_sbdb ↑ "AstDyS-2 Ceres Synthetic Proper Orbital Elements" . Department of Mathematics， University of Pisa， Italy. goân-loē-iông tī 21 November 2011 hőng khó͘-pih. 1 October 2011 khòaⁿ--ê . ↑ 6.0 6.1 "Asteroid Ceres P_constants (PcK) SPICE kernel file" . NASA Navigation and Ancillary Information Facility. goân-loē-iông tī 28 July 2020 hőng khó͘-pih. 8 September 2019 khòaⁿ--ê . ↑ Mao, X。; McKinnon, W。 B。 (2018). "Faster paleospin and deep-seated uncompensated mass as possible explanations for Ceres' present-day shape and gravity". Icarus . 299 : 430–442. Bibcode :2018Icar..299..430M . doi :10.1016/j.icarus.2017.08.033 . ↑ 引用錯誤: 無效的 <ref> tag;
揣無指名的ref文字 Park2016 ↑ 引用錯誤: 無效的 <ref> tag;
揣無指名的ref文字 Schorghofer2016 ↑ Konopliv, A.S。; Park, R.S。; Vaughan, A.T。; Bills, B.G。; Asmar, S.W。; Ermakov, A.伊。; Rambaux, N。; Raymond, C.A。; Castillo-Rogez, J.C。; Russell, C.T。; Smith, D.E。; Zuber, M.T. (2018). "The Ceres gravity field， spin pole， rotation period and orbit from the Dawn radiometric tracking and optical data". Icarus . 299 : 411–429. Bibcode :2018Icar..299..411K . doi :10.1016/j.icarus.2017.08.005 . ↑ 引用錯誤: 無效的 <ref> tag;
揣無指名的ref文字 Li2006 ↑ Rivkin, A。 S。; Volquardsen， E。 L。; Clark， B。 E。 (2006). "The surface composition of Ceres: Discovery of carbonates and iron-rich clays" (PDF) . Icarus . 185 (2): 563–567. Bibcode :2006Icar..185..563R . doi :10.1016/j.icarus.2006.08.022 . goân-loē-iông (PDF) tī 28 November 2007 hőng khó͘-pih. 8 December 2007 khòaⁿ--ê . ↑ 經, Bob (5 August 2015). "Let's Get Serious About Ceres" . Sky & Telescope . 25 July 2022 khòaⁿ--ê . ↑ 引用錯誤: 無效的 <ref> tag;
揣無指名的ref文字 AstDys-object ↑ 引用錯誤: 無效的 <ref> tag;
揣無指名的ref文字 Dawn2017 ↑ Tosi, F.; Capria, M. T.; et al. (2015). "Surface temperature of dwarf planet Ceres: Preliminary results from Dawn" . 46th Lunar and Planetary Science Conference : 11960. Bibcode :2015EGUGA..1711960T . 25 May 2021 khòaⁿ--ê . ↑ JPL/NASA (2015-04-22). "What is a Dwarf Planet?" . Jet Propulsion Laboratory . 2022-01-19 khòaⁿ--ê .
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