Pacific Ocean

57:8.3The real ge­o­logic his­tory of Uran­tia be­gins with the cool­ing of the earth’s crust suf­fi­ciently to cause the for­ma­tion of the first ocean. Wa­ter-va­por con­den­sa­tion on the cool­ing sur­face of the earth, once be­gun, con­tin­ued un­til it was vir­tu­ally com­plete. By the end of this pe­riod the ocean was world-wide, cov­er­ing the en­tire planet to an av­er­age depth of over one mile. The tides were then in play much as they are now ob­served, but this prim­i­tive ocean was not salty; it was prac­ti­cally a fresh-wa­ter cov­er­ing for the world. In those days, most of the chlo­rine was com­bined with var­i­ous met­als, but there was enough, in union with hy­dro­gen, to ren­der this wa­ter faintly acid.

57:8.4At the open­ing of this far­away era, Uran­tia should be en­vis­aged as a wa­ter-bound planet. Later on, deeper and hence denser lava flows came out upon the bot­tom of the pres­ent Pa­cific Ocean, and this part of the wa­ter-cov­ered sur­face be­came con­sid­er­ably de­pressed. The first con­ti­nen­tal land mass emerged from the world ocean in com­pen­satory ad­just­ment of the equi­lib­rium of the grad­u­ally thick­en­ing earth’s crust.

57:8.5950,000,000 years ago Uran­tia pre­sents the pic­ture of one great con­ti­nent of land and one large body of wa­ter, the Pa­cific Ocean. Vol­ca­noes are still wide­spread and earth­quakes are both fre­quent and se­vere. Me­te­ors con­tinue to bom­bard the earth, but they are di­min­ish­ing in both fre­quency and size. The at­mo­sphere is clear­ing up, but the amount of car­bon diox­ide con­tin­ues large. The earth’s crust is grad­u­ally sta­bi­liz­ing.

57:8.20Since the con­den­sa­tion of the earth’s hy­dro­sphere, first into the world ocean and sub­se­quently into the Pa­cific Ocean, this lat­ter body of wa­ter should be vi­su­al­ized as then cov­er­ing nine tenths of the earth’s sur­face. Me­te­ors falling into the sea ac­cu­mu­lated on the ocean bot­tom, and me­te­ors are, gen­er­ally speak­ing, com­posed of heavy ma­te­ri­als. Those falling on the land were largely ox­i­dized, sub­se­quently worn down by ero­sion, and washed into the ocean basins. Thus the ocean bot­tom grew in­creas­ingly heavy, and added to this was the weight of a body of wa­ter at some places ten miles deep.

60:1.12The ma­rine life of this pe­riod was mea­ger but im­proved rapidly with the new in­va­sion of the sea, which again pro­duced ex­ten­sive coast lines of shal­low wa­ters. Since there was more shal­low wa­ter around Eu­rope and Asia, the rich­est fos­sil beds are to be found about these con­ti­nents. To­day, if you would study the life of this age, ex­am­ine the Hi­malayan, Siberian, and Med­i­ter­ra­nean re­gions, as well as In­dia and the is­lands of the south­ern Pa­cific basin. A promi­nent fea­ture of the ma­rine life was the pres­ence of hosts of the beau­ti­ful am­monites, whose fos­sil re­mains are found all over the world.

79:1.6In­creas­ing arid­ity in cen­tral Asia fur­ther op­er­ated to re­duce pop­u­la­tion and to ren­der these peo­ple less war­like; and when the di­min­ish­ing rain­fall to the north forced the no­madic An­don­ites south­ward, there was a tremen­dous ex­o­dus of And­ites from Tur­kes­tan. This is the ter­mi­nal move­ment of the so-called Aryans into the Lev­ant and In­dia. It cul­mi­nated that long dis­per­sal of the mixed de­scen­dants of Adam dur­ing which ev­ery Asi­atic and most of the is­land peo­ples of the Pa­cific were to some ex­tent im­proved by these su­pe­rior races.