The pre-Nectarian period of the lunar geologic timescale runs from 4.533 billion years ago (the time of the initial formation of the Moon) to 3.920 billion years ago, when the Nectaris Basin was formed by a large impact. It is followed by the Nectarian period.
Pre-Nectarian rocks are rare in the lunar sample suite; they are mostly composed of lunar highlands material which have been heavily churned, brecciated, and thermally affected by subsequent impacts, particularly during the Heavy Bombardment Eon[1][2] (HBE; a period of 0.6-1 Gy from the formation of the Moon until at least the formation of the Imbrium Basin ~3.9 Ga, or even later with the formation of Orientale Basin) that marks the approximate beginning of the Nectarian period. The primary pre-Nectarian lunar highland material is dominated by the rock type anorthosite, which suggests that the early stage of lunar crustal formation occurred via mineral crystallization of a global magma ocean.
This geologic period has been informally subdivided into the Cryptic Era (4.533 - 4.172 Ga ago) and Basin Groups 1-9 (4.172 - 3.92 Ga ago),[3] but these divisions are not used on any geologic maps. Similarly the later period has also been called the Aitkenian period.
Dado que existe poca o ninguna evidencia geológica en la Tierra del tiempo comprendido por el período prenectario de la Luna, el prenectario ha sido utilizado como guía por al menos un trabajo científico notable [5] para subdividir el eón terrestre no oficial del Hadeano. . En particular, a veces se encuentra que el eón Hadeano se subdivide en la era Críptica , Grupos de Cuenca 1-9, Nectárico e Imbrio Inferior , aunque las dos primeras de estas divisiones lunares son informales y colectivamente constituyen el prenectario.