Wp/nas/Stære þer Erðe

Þie Stære þer Erðe

Þie Stære þer Erðe gebyrþ þie Andfaldung þes Planeten Erðe fram herer Geschapennes oþ þem nuteidlicen Daȝ.[1][2] Genaȝhe alle Boges gekynder Frœde habeþ tom Andgitt þer hefdlicen Towyrden þer Forþgewittennes þer Erðe geforþt, getakned be singallicer Wendung and leiffrœdlicer Utwælwung.

Þie erþfrœdlice Teidschale (ETS), als geswitteld fram betwuxþeedlicem Efenkyme,[3] depicts the large spans of time from the beginning of the Earth to the present, and its divisions chronicle some definitive events of Earth history. (In the graphic, Ma means "million years ago".) Erðe schoop schie selfe um foor 4.54 Billionen Ȝæren, approximately one-third the age of the universe, by accretion from the solar nebula.[4][5][6] Volcanic outgassing probably created the primordial atmosphere and then the ocean, but the early atmosphere contained almost no oxygen. Micel þer Erðe was for geloomlicen Belemmungen mid oðeren Bodies gemolten uch of the Earth was molten because of frequent collisions with other bodies which led to extreme volcanism. While the Earth was in its earliest stage (Early Earth), a giant impact collision with a planet-sized body named Theia is thought to have formed the Moon. Over time, the Earth cooled, causing the formation of a solid crust, and allowing liquid water on the surface.