ing in twelve hours only one-fifth of the visible hemisphere, while crossing in the same time 144° on the zodiac—twelve degrees per hour, or our Moon's diameter in two minutes and a half—was left behind by the stars; and fixing what I may call the ocular attention on her, she seemed to stand still while they slowly passed her; thus making their revolution perceptible to sense as it never is on Earth, for lack of a similar standard. Caulna, rising in the west and moving eastwards, crossed the visible sky in five hours, and passed through the stars at the rate of 48° per hour, so that she seemed to sail past them like a golden cloudlet or celestial vessel driven by a slow wind. It happened this night that she passed over the star Fomalhaut—an occultation which I watched with great interest through an excellent field-glass, but which lasted only for about half a minute. About an hour before midnight the two moons passed each other in the Eastern sky; both gibbous at the moment, like our Moon in her last quarter. The difference in size and motion was then most striking; Caulna seeming to rush past her companion, and the latter looking like a stationary star in the slowly moving sky.
