| http://www.w3.org/ns/prov#value | - The relative distance between planets remaining ever the same, and being in no wise affected by the displacement of the whole system; and the distance between the latter and the stars and other suns being so incommensurable as to produce but little if any perceptible change for centuries and milleniums to come; -- no astronomer will perceive it telescopically, until Jupiter and some other planets,
|
