Periode rotasi: Perbedaan antara revisi

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'''Periode rotasi''' suatu [[benda astronomi|benda]] [[astronomi|astronomis]]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
Baris 7:
|[[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>{{pdflink|[http://astrogeology.usgs.gov/Projects/ISPRS/PREPRINTS/IAU2000/IAU2000_preprint.pdf Report of the IAU/IAG Working Group on Cartographic Coordinates and Rotational Elements of the Planets and Satellites: 2000]|215KB}} pp7–8</ref> <br> 35 hari (lintang tinggi) || 25{{smallsup|d}} 9{{smallsup|h}} 7{{smallsup|m}} 11.6{{smallsup|s}} <br> 35{{smallsup|d}}
|-
|[[Merkurius]]|| 58.6462 hari<ref name=Allen296>{{cite book |title=''Allen's Astrophysical Quantities'' |url=http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA296 |author=Clabon Walter Allen and Arthur N. Cox |publisher=Springer |year=2000 |isbn=0387987460 |pages=296}}</ref> || 58{{smallsup|d}} 15{{smallsup|h}} 30{{smallsup|m}} 30{{smallsup|s}}
|-
|[[Venus]]|| –243.0187 hari<ref name=Allen296/><ref name=negative>This rotation is negative because the pole which points north of the [[ecliptic]] rotates in the opposite direction to most other planets.</ref> || –243{{smallsup|d}} 0{{smallsup|h}} 26{{smallsup|m}}
Baris 13:
|[[Bumi]]|| 0.99726968 hari<ref name=Allen296/><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{{smallsup|d}} 23{{smallsup|h}} 56{{smallsup|m}} 4.100{{smallsup|s}}
|-
|[[Bulan]]|| 27.321661 hari<ref name=Allen>{{cite book |title=''Allen's Astrophysical Quantities'' |url=http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA308 |author=Clabon Walter Allen and Arthur N. Cox |publisher=Springer |year=2000 |isbn=0387987460 |pages=308}}</ref> <br> ([[Rotasi sinkronis|sinkronis]] terhadap Bumi) || 27{{smallsup|d}} 7{{smallsup|h}} 43{{smallsup|m}} 11.5{{smallsup|s}} <br> &nbsp;
|-
|[[Mars]]|| 1.02595675 hari<ref name=Allen296/> || 1{{smallsup|d}} 0{{smallsup|h}} 37{{smallsup|m}} 22.663{{smallsup|s}}
Baris 22:
|title=Ceres lightcurve analysis – Period determination
|journal=Icarus|volume=188
|issue=2|pages=451&ndash;456451–456|year=2007
|doi=10.1016/j.icarus.2006.11.025
|bibcode=2007Icar..188..451C }}</ref> || 0{{smallsup|d}} 9{{smallsup|h}} 4{{smallsup|m}} 27.0{{smallsup|s}}
|-
|[[YupiterJupiter]]|| 0.4135344 hari (interior dalam)<ref name=mag>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{{smallsup|d}} 9{{smallsup|h}} 55{{smallsup|m}} 29.37{{smallsup|s}}<ref name=Allen296/> <br> 0{{smallsup|d}} 9{{smallsup|h}} 50{{smallsup|m}} 30{{smallsup|s}}<ref name=Allen296/> <br> 0{{smallsup|d}} 9{{smallsup|h}} 55{{smallsup|m}} 43.63{{smallsup|s}}<ref name=Allen296/>
|-
|[[Saturnus]]|| 0.44403 hari (interior dalam)<ref name=mag/> <br> 0.426 hari (khatulistiwa) <br> 0.443 hari (lintang tinggi) || 0{{smallsup|d}} 10{{smallsup|h}} 39{{smallsup|m}} 24{{smallsup|s}}<ref name=Allen296/> <br> 0{{smallsup|d}} 10{{smallsup|h}} 14{{smallsup|m}}<ref name=Allen296/> <br> 0{{smallsup|d}} 10{{smallsup|h}} 38{{smallsup|m}}<ref name=Allen296/>
Baris 36:
|[[Pluto]]||–6.38718 hari<ref name=Allen296/><ref name=negative/> <br> (sinkronis dengan [[Charon (satelit)|Charon]]) || –6{{smallsup|d}} 9{{smallsup|h}} 17{{smallsup|m}} 32{{smallsup|s}} <br> &nbsp;
|-
|[[Haumea (planet kerdil)|Haumea]]||0.163145 days<ref name="hour">{{cite journal
|title = High-Precision Photometry of Extreme KBO 2003 EL61
{{cite journal
|author = Pedro Lacerda, David Jewitt and Nuno Peixinho
|title=High-Precision Photometry of Extreme KBO 2003 EL61
|date = 2008-04-02
|author=Pedro Lacerda, David Jewitt and Nuno Peixinho
|journal |date=2008-04-02 |journal= The Astronomical Journal
|volume = 135
|issue=5 |pages =1749–1756 5
|pages = 1749–1756
|url = http://www.iop.org/EJ/abstract/1538-3881/135/5/1749
|accessdate=2008-09-22 |doi=10.1088/0004-6256/135/5/1749 |bibcode=2008AJ....135.1749L}}</ref> || 0{{smallsup|d}} 3{{smallsup|h}} 54{{smallsup|m}} 56{{smallsup|s}}
|accessdate = 2008-09-22
|doi = 10.1088/0004-6256/135/5/1749
|bibcode = 2008AJ....135.1749L
|archive-date = 2020-05-11
|archive-url = https://web.archive.org/web/20200511174835/https://hkvalidate.perfdrive.com/captcha?ssa=d100e089-e0a8-46b1-b2bf-689b5365ec41&ssb=64zm3m0dgdh6im44klgchgzmd&ssc=http%3A%2F%2Fiopscience.iop.org%2F%2Fabstract%2F1538-3881%2F135%2F5%2F1749&ssd=166792861026451&sse=jf%40f%40ammepjkppb&ssf=6b72fa3c9f612d4213d2ff4654a1c777486333c1&ssg=b9f568f8-7538-44de-a6f6-6f8dfec8c12a&ssh=a51051be-6ae4-4b87-997d-7dd6b66dbeac&ssi=d39da3c3-8427-4549-84d4-28b15eafb1bc&ssj=01a53d23-c7ea-4372-a930-84997b7470ec&ssk=support%40shieldsquare.com&ssl=006665034040&ssm=04074166802434092108065763560772&ssn=3ea2b7d835b51d06c85308b990308f630022a1d567bb-d922-4e12-b7c008&sso=1c586636-44737ddebefab59c4296944173171afd3b424b9846579d88&ssp=92848774861589221168158922803833385&ssq=21665731931443509724419314921061671828681&ssr=MjA3LjI0MS4yMjUuMTYw&sss=Chrome%2F5.0%20%28iPhone%3B%20U%3B%20CPU%20iPhone%20OS%203_0%20like%20Mac%20OS%20X%3B%20en-us%29%20AppleWebKit%2F528.18%20%28KHTML%2C%20like%20Gecko%29%20Version%2F4.0%20Mobile%2F7A341%20Safari%2F528.16&sst=Mozilla%2F5.0%20%28Windows%20NT%2010.0%3B%20Win64%3B%20x64%29%20AppleWebKit%2F537.36%20%28KHTML%2C%20like%20Gecko%29%20Chrome%2F74.0.3729.169%20Safari%2F537.36&ssu=Mozilla%2F4.0%20%28Windows%20NT%205.1%29%20AppleWebKit%2F535.7%20%28KHTML%2Clike%20zeco%29%20Chrome%2F33.0.1750.154%20Safari%2F536.7&ssv=3tmsrmq1lsnqmvm&ssw=&ssx=393044951461425&ssy=chdgnchdcajkidhbnhkjgmp%40lboiheflopndkp%40n&ssz=0d4e9450ffb2729
|dead-url = yes
|accessdate=2008-09-22 |doi=10.1088/0004-6256/135/5/1749 |bibcode=2008AJ....135.1749L}}</ref> || 0{{smallsup|d}} 3{{smallsup|h}} 54{{smallsup|m}} 56{{smallsup|s}}
|}
 
== Lihat pula ==
* [[Kutub benda astronomi]]
* [[Gerakan menghulu]]
* [[Gerakan langsung]]
 
== Catatan kaki ==
{{reflist}}
 
== Pranala luar ==
* {{cite book |title=Solar System Dynamics |url=http://books.google.com/books?id=aU6vcy5L8GAC&pg=PP1#PPA531,M1 |author=Murray, Carl D. and Stanley F. Dermott |publisher=Cambridge UP |year=1999 |pages=531 |isbn=0-521-57295-9}} Rotation periods of Mercury and Earth are wrong.
 
[[Kategori:Mekanika benda langit]]
[[Kategori:Waktu dalam astronomi]]
 
[[ast:Periodu de rotación]]
[[bg:Период на въртене]]
[[ca:Període de rotació]]
[[de:Rotationsperiode]]
[[en:Rotation period]]
[[eo:Rotacia periodo]]
[[es:Periodo de rotación]]
[[eu:Biraketa periodo]]
[[fr:Période de rotation]]
[[he:זמן סיבוב עצמי]]
[[hi:घूर्णन काल]]
[[hr:Period rotacije]]
[[it:Periodo di rotazione]]
[[ja:自転周期]]
[[kk:Айналыс кезеңі]]
[[ko:자전 주기]]
[[la:Periodus rotationis]]
[[lb:Rotatiounsperiod]]
[[lv:Rotācijas periods]]
[[mk:Период на ротација]]
[[mr:परिवलन काळ]]
[[nl:Rotatieperiode]]
[[nn:Rotasjonsperiode]]
[[no:Rotasjonsperiode]]
[[oc:Periòde de rotacion]]
[[pl:Okres obrotu]]
[[pt:Período de rotação]]
[[ru:Период вращения]]
[[simple:Rotation period]]
[[sk:Rotačná perióda]]
[[sl:Vrtilna doba]]
[[sv:Rotationsperiod]]
[[ta:சுழற்சிக் காலம்]]
[[th:คาบการหมุนรอบตัวเอง]]
[[uk:Період обертання]]
[[vi:Chu kỳ tự quay]]
[[zh:自轉週期]]