Call the World spider: and at fancy's touch
Thought becomes image and I see it such.
With viscous masonry of films and threads
Tough as the nets in Indian Forests found
It blends the Waller's and the Weaver's trades
And soon the tent-like Hangings touch the ground
A dusky chamber that excludes the day
But cease the prelude and resume the lay


FOOTNOTES:

[1111:1] Literally rendered is Flower Fadeless, or never-fading, from the Greek a not and marainō to wither.

[1111:2] Mate, Counterpart.


D

Note to Line 34 of the Joan of Arc Book II. 1796, pp. 41, 42.

Line 34. Sir Isaac Newton at the end of the last edition of his Optics supposes that a very subtile and elastic fluid, which he calls aether, is diffused thro' the pores of gross bodies, as well as thro' the open spaces that are void of gross matter: he supposes it to pierce all bodies, and to touch their least particles, acting on them with a force proportional to their number or to the matter of the body on which it acts. He supposes likewise, that it is rarer in the pores of bodies than in open spaces, and even rarer in small pores and dense bodies, than in large pores and rare bodies; and also that its density increases in receding from gross matter; so for instance as to be greater at the 1/100 of an inch from the surface of any body, than at its surface; and so on. To the action of this aether he ascribes the attractions of gravitation and cohœsion, the attraction and repulsion of electrical bodies, the mutual influences of bodies and light upon each other, the effects and communication of heat, and the performance of animal sensation and motion. David Hartley, from whom this account of aether is chiefly borrowed, makes it the instrument of propagating those vibrations or configurative motions which are ideas. It appears to me, no hypothesis ever involved so many contradictions; for how can the same fluid be both dense and rare in the same body at one time? Yet in the Earth as gravitating to the Moon, it must be very rare; and in the Earth as gravitating to the Sun, it must be very dense. For as Andrew Baxter well observes, it doth not appear sufficient to account how the fluid may act with a force proportional to the body to which another is impelled, to assert that it is rarer in great bodies than in small ones; it must be further asserted that this fluid is rarer or denser in the same body, whether small or great, according as the body to which that is impelled is itself small or great. But whatever may be the solidity of this objection, the following seems unanswerable: