Lihat sumber Periode rotasi

'''Periode rotasi''' suatu [[benda astronomi|benda]] [[astronomi]]s adalah waktu yang dibutuhkan untuk menyelesaikan satu revolusi mengitari [[sumbu rotasi]]nya relatif terhadap bintang di belakangnya. Periode ini berbeda dengan [[hari sinodis|hari matahari]] planet, yang mencakup rotasi tambahan untuk memenuhi bagian [[periode orbit]] planet selama satu hari.

== Periode rotasi beberapa benda angkasa ==
{|class="wikitable"
!Planet ||colspan=2| Periode rotasi
|-
|[[Matahari]]|| 25.379995 hari (khatulistiwa)<ref>[http://astrogeology.usgs.gov/Projects/WGCCRE/constants/iau2000_table1.html Rotation and pole position for the Sun and planets] Rotation period in days is 360° divided by the coefficient of ''d''.</ref><ref>pp7–8</ref> <br> 35 hari (lintang tinggi) || 25 9 7 11.6 <br> 35
|-
|[[Merkurius]]|| 58.6462 hari<ref>Clabon Walter Allen and Arthur N. Cox. [http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA296 ''Allen's Astrophysical Quantities'']. Springer. 2000. hlm. 296. ISBN 0387987460.</ref> || 58 15 30 30
|-
|[[Venus]]|| –243.0187 hari<ref>Clabon Walter Allen and Arthur N. Cox. [http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA296 ''Allen's Astrophysical Quantities'']. Springer. 2000. hlm. 296. ISBN 0387987460.</ref><ref>This rotation is negative because the pole which points north of the ecliptic rotates in the opposite direction to most other planets.</ref> || –243 0 26
|-
|[[Bumi]]|| 0.99726968 hari<ref>Clabon Walter Allen and Arthur N. Cox. [http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA296 ''Allen's Astrophysical Quantities'']. Springer. 2000. hlm. 296. ISBN 0387987460.</ref><ref>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.</ref> || 0 23 56 4.100
|-
|[[Bulan]]|| 27.321661 hari<ref>Clabon Walter Allen and Arthur N. Cox. [http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA308 ''Allen's Astrophysical Quantities'']. Springer. 2000. hlm. 308. ISBN 0387987460.</ref> <br> ([[Rotasi sinkronis|sinkronis]] terhadap Bumi) || 27 7 43 11.5 <br> &nbsp;
|-
|[[Mars]]|| 1.02595675 hari<ref>Clabon Walter Allen and Arthur N. Cox. [http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA296 ''Allen's Astrophysical Quantities'']. Springer. 2000. hlm. 296. ISBN 0387987460.</ref> || 1 0 37 22.663
|-
|[[1 Ceres|Ceres]]|| 0.37809 hari<ref>Matthew A. Chamberlain. ''Ceres lightcurve analysis – Period determination''. ''Icarus''. 2007. Vol. 188 (2). hlm. 451–456. doi:10.1016/j.icarus.2006.11.025.</ref> || 0 9 4 27.0
|-
|[[Jupiter]]|| 0.4135344 hari (interior dalam)<ref>Rotation period of the deep interior is that of the planet's magnetic field.</ref> <br> 0.41007 hari (khatulistiwa) <br> 0.41369942 hari (lintang tinggi) || 0 9 55 29.37<ref>Clabon Walter Allen and Arthur N. Cox. [http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA296 ''Allen's Astrophysical Quantities'']. Springer. 2000. hlm. 296. ISBN 0387987460.</ref> <br> 0 9 50 30<ref>Clabon Walter Allen and Arthur N. Cox. [http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA296 ''Allen's Astrophysical Quantities'']. Springer. 2000. hlm. 296. ISBN 0387987460.</ref> <br> 0 9 55 43.63<ref>Clabon Walter Allen and Arthur N. Cox. [http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA296 ''Allen's Astrophysical Quantities'']. Springer. 2000. hlm. 296. ISBN 0387987460.</ref>
|-
|[[Saturnus]]|| 0.44403 hari (interior dalam)<ref>Rotation period of the deep interior is that of the planet's magnetic field.</ref> <br> 0.426 hari (khatulistiwa) <br> 0.443 hari (lintang tinggi) || 0 10 39 24<ref>Clabon Walter Allen and Arthur N. Cox. [http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA296 ''Allen's Astrophysical Quantities'']. Springer. 2000. hlm. 296. ISBN 0387987460.</ref> <br> 0 10 14<ref>Clabon Walter Allen and Arthur N. Cox. [http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA296 ''Allen's Astrophysical Quantities'']. Springer. 2000. hlm. 296. ISBN 0387987460.</ref> <br> 0 10 38<ref>Clabon Walter Allen and Arthur N. Cox. [http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA296 ''Allen's Astrophysical Quantities'']. Springer. 2000. hlm. 296. ISBN 0387987460.</ref>
|-
|[[Uranus]]|| –0.71833 hari<ref>Clabon Walter Allen and Arthur N. Cox. [http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA296 ''Allen's Astrophysical Quantities'']. Springer. 2000. hlm. 296. ISBN 0387987460.</ref><ref>This rotation is negative because the pole which points north of the ecliptic rotates in the opposite direction to most other planets.</ref><ref>Rotation period of the deep interior is that of the planet's magnetic field.</ref> || –0 17 14 24
|-
|[[Neptunus]]|| 0.67125 hari<ref>Clabon Walter Allen and Arthur N. Cox. [http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA296 ''Allen's Astrophysical Quantities'']. Springer. 2000. hlm. 296. ISBN 0387987460.</ref><ref>Rotation period of the deep interior is that of the planet's magnetic field.</ref> || 0 16 6 36
|-
|[[Pluto]]||–6.38718 hari<ref>Clabon Walter Allen and Arthur N. Cox. [http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA296 ''Allen's Astrophysical Quantities'']. Springer. 2000. hlm. 296. ISBN 0387987460.</ref><ref>This rotation is negative because the pole which points north of the ecliptic rotates in the opposite direction to most other planets.</ref> <br> (sinkronis dengan [[Charon (satelit)|Charon]]) || –6 9 17 32 <br> &nbsp;
|-
|[[Haumea (planet kerdil)|Haumea]]||0.163145 days<ref>Pedro Lacerda, David Jewitt and Nuno Peixinho. [http://www.iop.org/EJ/abstract/1538-3881/135/5/1749 High-Precision Photometry of Extreme KBO 2003 EL61]. ''The Astronomical Journal''. 2008-04-02. Vol. 135 (5). hlm. 1749–1756. doi:10.1088/0004-6256/135/5/1749.</ref> || 0 3 54 56
|}

== Lihat pula ==
* [[Kutub benda astronomi]]
* [[Gerakan menghulu]]
* [[Gerakan langsung]]

== Pranala luar ==
*  Rotation periods of Mercury and Earth are wrong.

== Referensi ==
<references />

== Sumber dan atribusi ==

Konten artikel ini diadaptasi dari [https://id.wikipedia.org/w/index.php?title=Periode+rotasi&oldid=28061346 Wikipedia bahasa Indonesia], revisi 28061346 (2025-10-17T09:55:37Z), yang tersedia berdasarkan lisensi Creative Commons Atribusi-BerbagiSerupa (CC BY-SA). Mohon gunakan konten ini secara bijak serta sesuai dengan ketentuan lisensi yang berlaku.

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