Перыяд вярчэння: Розніца паміж версіямі

Перыяд вярчэння Зямлі адносна кропкі вясновага раўнадзенства называецца [[Зорныя суткі|зорнымі суткамі]]<ref>{{cite web|url=http://www.astronet.ru/db/msg/1225962|title=Вращение Земли и продолжительность суток|author=К. В. Куимов|date=2008-02-06|publisher=[[ГАИШ]], Москва|lang=ru|accessdate=2010-07-20|archiveurl=http://www.webcitation.org/65t42crCf|archivedate=2012-03-03}}</ref>.

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|[[Сонца]]||{{bartable| 25.379995| дня<ref>{{cite journal|title=Report of the IAU/IAG Working Group on Cartographic Coordinates and Rotational Elements of the Planets and Satellites: 2000|author=P. K. Seidelmann, V. K. Abalakin, M. Bursa, M. E. Davies, C. de Bergh, J. H. Lieske, J. Oberst, J. L. Simon, E. M. Standish, P. Stooke, P. C. Thomas|journal=Celestial Mechanics and Dynamical Astronomy|year=2002|volume=82|issue=1|pages=86|url=http://link.springer.com/article/10.1023%2FA%3A1013939327465}}</ref><ref>Равен 360° делить на коэффициент при d в выражении для W.</ref>|2|1em|background:blue}}

|[[Планета Меркурый|Меркурый]]||{{bartable| 58.6462| дня<ref name=Allen296>{{cite book |title=''Allen's Astrophysical Quantities'' |url=http://books.google.com/books?id=w8PK2XFLLH8C&pg=PA296 |author=Clabon Walter Allen, Arthur N. Cox|publisher=Springer |date=2000 |isbn=0-387-98746-0 |pages=296}}</ref>|3|1em|background:blue}}

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|[[Планета Зямля|Зямля]]||{{bartable| 0.99726968| дня<ref name=Allen296/>|3|1em|background:blue}}