Sicut ergo prius sol a medio procedens orientis aequinoctium vernale suo praefixit exortu; deinde luna, sole ad vesperam occidente, et ipsa plena a medio secuta est orientis: ita omnibus annis idem primus lunae mensis eodem necesse est ordine servari, ut non ante aequinoctium, sed vel ipso aequinoctii die, sicut in principio factum est, vel eo transcenso plenilunium habere debeat.
Therefore as first the sun coming forth from the midst of the east made by that his rising the equality of day and night in the spring; and after, the moon (the sun going down at evening) followed itself also at the full from the midst of the east; so every year the same first month of the moon must be observed after the same order, so that she should be at the full not before the day and night be of one length, but either on the very day of that equality, as was done in the beginning, or when it is past.
final_alignments\Bede_Ecclesiastical_Book5.json