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^ a b c d e f g h i j k l m Clabon Walter Allen and Arthur N. Cox (2000). Allen's Astrophysical Quantities. Springer. pp. 296. .mw-parser-output cite.citation{font-style:inherit;word-wrap:break-word}.mw-parser-output .citation q{quotes:"\"""\"""'""'"}.mw-parser-output .citation.cs-ja1 q,.mw-parser-output .citation.cs-ja2 q{quotes:"「""」""『""』"}.mw-parser-output .citation:target{background-color:rgba(0,127,255,0.133)}.mw-parser-output .id-lock-free a,.mw-parser-output .citation .cs1-lock-free a{background:url("//upload.wikimedia.org/wikipedia/commons/6/65/Lock-green.svg")right 0.1em center/9px no-repeat}.mw-parser-output .id-lock-limited a,.mw-parser-output .id-lock-registration a,.mw-parser-output .citation .cs1-lock-limited a,.mw-parser-output .citation .cs1-lock-registration a{background:url("//upload.wikimedia.org/wikipedia/commons/d/d6/Lock-gray-alt-2.svg")right 0.1em center/9px no-repeat}.mw-parser-output .id-lock-subscription a,.mw-parser-output .citation .cs1-lock-subscription a{background:url("//upload.wikimedia.org/wikipedia/commons/a/aa/Lock-red-alt-2.svg")right 0.1em center/9px no-repeat}.mw-parser-output .cs1-ws-icon a{background:url("//upload.wikimedia.org/wikipedia/commons/4/4c/Wikisource-logo.svg")right 0.1em center/12px no-repeat}.mw-parser-output .cs1-code{color:inherit;background:inherit;border:none;padding:inherit}.mw-parser-output .cs1-hidden-error{display:none;color:#d33}.mw-parser-output .cs1-visible-error{color:#d33}.mw-parser-output .cs1-maint{display:none;color:#3a3;margin-left:0.3em}.mw-parser-output .cs1-format{font-size:95%}.mw-parser-output .cs1-kern-left{padding-left:0.2em}.mw-parser-output .cs1-kern-right{padding-right:0.2em}.mw-parser-output .citation .mw-selflink{font-weight:inherit}ISBN 0387987460
^ a b c This rotation is negative because the pole which points north of the ecliptic rotates in the opposite direction to most other planets.
^ Reference adds about 1 ms to Earth's stellar day given in mean solar time to account for the length of Earth's mean solar day in excess of 86400 SI seconds.
^ Clabon Walter Allen and Arthur N. Cox (2000). Allen's Astrophysical Quantities. Springer. pp. 308. ISBN 0387987460
^ Chamberlain, Matthew A.; Sykes, Mark V.; Esquerdo, Gilbert A. (2007). “Ceres lightcurve analysis ? Period determination”. Icarus 188: 451–456. doi:10.1016/j.icarus.2006.11.025. https://ui.adsabs.harvard.edu/abs/2007Icar..188..451C/abstract.
^ a b c d Rotation period of the deep interior is that of the planet's magnetic field.
^ Pedro Lacerda, David Jewitt and Nuno Peixinho (2008-04-02). ⇒“High-Precision Photometry of Extreme KBO 2003 EL61”. The Astronomical Journal 135: 1749?1756. doi:10.1088/0004-6256/135/5/1749. ⇒http://www.iop.org/EJ/abstract/1538-3881/135/5/1749 2008年9月22日閲覧。.
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