File:Equinox path.png

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English: Path of the point of vernal equinox along the ecliptic over a 6000 year period. The tradition of take the point of vernal equinox as defining the "sign of Aries" dates to Babylonian astrology, ca. 600 BC. It is apparent in this image that the main star of Aries, Hamal, was closest to the point of vernal equinox in ca. the 7th century BC.
Polski: Ścieżka przemieszczania się punktu równonocy wiosennej, wzdłuż ekliptyki w ciągu 6000 lat. Tradycja przyjęła punkt równonocy wiosennej, definijąc go jako określenie "punkt Barana" i pochodzi z babilońskiej astrologii, z okresu 600 lat przed naszą erą. Jak widać na tym zdjęciu, główna gwiazda punktu Barana, Hamal, była najbliżej punktu równonocy wiosennej w 7 wieku pn.
Italiano: Percorso del punto dell'equinozio di primavera lungo l'eclittica durante gli ultimi 6000 anni. Oggi esso si trova nella costellazione dei Pesci; nel 700 a.C. era vicino ad Hamal, la principale stella della costellazione dell'Ariete. Nel 3000 a.C. era vicino ad Aldebaran del Toro: l'"era del toro" è durata dal 4480 al 2320 a.C.
Source Own work
Author Dbachmann
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File:Equinox positions.png

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current15:42, 1 April 2009Thumbnail for version as of 15:42, 1 April 2009638 × 373 (25 KB)Dbachmann{{Information |Description={{en|1=path of the point of vernal equinox along the ecliptic over the past 6000 years}} |Source=Own work by uploader |Author=Dbachmann |Date= |Permission= |other_versions= }} [[Category:Precession of the equi

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