Planet: Perbedaan antara revisi
Konten dihapus Konten ditambahkan
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Baris 418:
:{{note label|d|d|d}} Seperti Pluto, saat berada di [[Apsis|perihelion]], atmosfer sementara terbentuk.
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==Periode rotasi==
{{utama|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>{{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}}
|-
|[[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 />
|-
|[[Mars]]|| 1.02595675 hari<ref name=Allen296/> || 1{{smallsup|d}} 0{{smallsup|h}} 37{{smallsup|m}} 22.663{{smallsup|s}}
|-
|[[1 Ceres|Ceres]]|| 0.37809 hari<ref name="Chamberlain2007">{{cite journal
|last=Chamberlain |first=Matthew A.
|coauthors=Sykes, Mark V.; Esquerdo, Gilbert A.
|title=Ceres lightcurve analysis – Period determination
|journal=Icarus|volume=188
|issue=2|pages=451–456|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}}
|-
|[[Yupiter]]|| 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/>
|-
|[[Uranus]]|| –0.71833 hari<ref name=Allen296/><ref name=negative/><ref name=mag/> || –0{{smallsup|d}} 17{{smallsup|h}} 14{{smallsup|m}} 24{{smallsup|s}}
|-
|[[Neptunus]]|| 0.67125 hari<ref name=Allen296/><ref name=mag/> || 0{{smallsup|d}} 16{{smallsup|h}} 6{{smallsup|m}} 36{{smallsup|s}}
|-
|[[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 />
|-
|[[Haumea (planet kerdil)|Haumea]]||0.163145 days<ref name="hour">
{{cite journal
|title=High-Precision Photometry of Extreme KBO 2003 EL61
|author=Pedro Lacerda, David Jewitt and Nuno Peixinho
|date=2008-04-02 |journal=The Astronomical Journal
|volume= 135
|issue=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}}
|}
== Planet luar surya ==
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