Posted on Thursday 30 July 2009
idea of the sun and planets, with their attendant satellites, not asturned out like manufactured articles, ready made, at measuredintervals, in a vast and deliberate celestial Orrery, but as due to theslow and gradual working of natural laws, in accordance with which eachhas assumed by force of circumstances its existing place, weight, orbit,and motion.
The grand conception of a gradual becoming, instead of a sudden making,which Kant and Laplace thus applied to the component bodies of theuniverse at large, was further applied by Lyell and his school to theouter crust of this one particular petty planet of ours. While theastronomers went in for the evolution of suns, stars, and worlds, Lyelland his geological brethren went in for the evolution of the earth’ssurface. As theirs was stellar, so his was mundane. If the world beganby being a red-hot mass of planetary matter in a high state of internalexcitement, boiling and dancing with the heat of its emotions, itgradually cooled down with age and experience, for growing old isgrowing cold, as every one of us in time, alas, discovers. As it passedfrom its fiery and volcanic youth to its staider and soberer middle age,a solid crust began to form in filmy fashion upon its cooling surface.The aqueous vapour that had floated at first as steam around its heatedmass condensed with time into a wide ocean over the now hardened shell.Gradually this ocean shifted its bulk into two or three main bodies thatsank into hollows of the viscid crust, the precursors of Atlantic,Pacific, and the Indian Seas. Wrinklings of the crust, produced by thecooling and consequent contraction, gave rise at first to baby mountainranges, and afterwards to the earliest rough draughts of the still veryvague and sketchy continents. The world grew daily more complex and morediverse; it progressed, in accordance with the Spencerian law, from thehomogeneous to the heterogeneous, and so forth, as aforesaid, withdelightful regularity.
At last, by long and graduated changes, seas and lands, peninsulas andislands, lakes and rivers, hills and mountains, were wrought out byinternal or external energies on the crust thus generally fashioned.Evaporation from the oceans gave rise to clouds and rain and hailstorms;the water that fell upon the mountain tops cut out the valleys and riverbasins; rills gathered into brooks, brooks into streams, streams intoprimaeval Niles, and Amazons, and Mississippis. Volcanic forces upliftedhere an Alpine chain, or depressed there a deep-sea hollow. Sedimentwashed from the hills and plains, or formed from countless skeletons ofmarine creatures, gathered on the sinking bed of the ocean as soft ooze,or crumbling sand, or thick mud, or gravel and conglomerate. Nowupheaved into an elevated table-land, now slowly carved again by rainand rill into valley and watershed, and now worn down once more intothe mere degraded stump of a plateau, the crust underwent innumerablechanges, but almost all of them exactly the same in kind, and mostly indegree, as those we still see at work imperceptibly in the world aroundus. Rain washing down the soil; weather crumbling the solid rock; wavesdashing at the foot of the cliffs; rivers forming deltas at their barred