The one point the catastrophists and the uniformitarians agreed upon, when this Society was founded, was to ignore it.  And you will find, if you look back into our records, that our revered fathers in geology plumed themselves a good deal upon the practical sense and wisdom of this proceeding.  As a temporary measure, I do not presume to challenge its wisdom; but in all organised bodies temporary changes are apt to produce permanent effects; and as time has slipped by, altering all the conditions which may have made such mortification of the scientific flesh desirable, I think the effect of the stream of cold water which has steadily flowed over geological speculation within these walls has been of doubtful beneficence.

The sort of geological speculation to which I am now referring (geological aetiology, in short) was created, as a science, by that famous philosopher Immanuel Kant, when, in 1775, he wrote his “General Natural History and Theory of the Celestial Bodies; or an Attempt to account for the Constitutional and the Mechanical Origin of the Universe upon Newtonian principles."[11]

[Footnote 11:  Grant (History of Physical Astronomy, p. 574) makes but the briefest reference to Kant.]

In this very remarkable but seemingly little-known treatise,[12] Kant expounds a complete cosmogony, in the shape of a theory of the causes which have led to the development of the universe from diffused atoms of matter endowed with simple attractive and repulsive forces.

[Footnote 12:  “Allgemeine Naturgeschichte und Theorie des Himmels; oder Versuch von der Verfassung und dem mechanischen Ursprunge des ganzen Weltgebaeudes nach Newton’schen Grundsatzen abgehandelt.”—­KANT’S Saemmtliche Werke, Bd. i. p. 207.]

“Give me matter,” says Kant, “and I will build the world;” and he proceeds to deduce from the simple data from which he starts, a doctrine in all essential respects similar to the well-known “Nebular Hypothesis” of Laplace.[13] He accounts for the relation of the masses and the densities of the planets to their distances from the sun, for the eccentricities of their orbits, for their rotations, for their satellites, for the general agreement in the direction of rotation among the celestial bodies, for Saturn’s ring, and for the zodiacal light.  He finds in each system of worlds, indications that the attractive force of the central mass will eventually destroy its organisation, by concentrating upon itself the matter of the whole system; but, as the result of this concentration, he argues for the development of an amount of heat which will dissipate the mass once more into a molecular chaos such as that in which it began.

[Footnote 13:  Systeme du Monde, tome ii. chap. 6.]