Rotation period

In astronomy, a rotation period is the time an astronomical object takes to complete one revolution around its rotation axis relative to the background stars. For the Earth this is a sidereal day. It is different from a solar day, which is measured by the passage of the Sun across the local meridian.

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Other websites

  • "MIRA". Jupiter. Retrieved 2005-5-24. Check date values in: |accessdate= (help)

Other Languages
العربية: فترة التناوب
azərbaycanca: Fırlanma periodu
беларуская: Перыяд вярчэння
Esperanto: Rotacia periodo
فارسی: دوره چرخش
한국어: 자전 주기
हिन्दी: घूर्णन काल
Bahasa Indonesia: Periode rotasi
Lëtzebuergesch: Rotatiounsperiod
македонски: Вртежен период
Bahasa Melayu: Tempoh putaran
Nederlands: Rotatieperiode
日本語: 自転周期
norsk nynorsk: Rotasjonsperiode
polski: Okres obrotu
slovenčina: Rotačná perióda
slovenščina: Vrtilna doba
српски / srpski: Период ротације
srpskohrvatski / српскохрватски: Period rotacije
українська: Період обертання
中文: 自轉週期