became impossible with the naked eye to distinguish the individual points from the smaller stars; and shortly after this the nearest began to present discs of appreciable size but somewhat irregular shape. I had now no doubt that I was about to pass through one of those meteoric rings which our most advanced astronomers believe to exist in immense numbers throughout space, and to the Earth's contact with or approach to which they ascribe the showers of falling, stars visible in August and November. Ere long, one after another of these bodies passed rapidly before my sight, at distances varying probably from five yards to five thousand miles. Where to test the distance was impossible, anything like accurate measurement was equally out of the question; but my opinion is, that the diameters of the nearest ranged from ten inches to two hundred feet. One only passed so near that its absolute size could be judged by the marks upon its face. This was a rock-like mass, presenting at many places on the surface distinct traces of metallic veins or blotches, rudely ovoid in form, but with a number of broken surfaces, one or two of which reflected the light much more brilliantly than others. The weight of this one meteoroid was too insignificant as compared with that of the Astronaut seriously to disturb my course. Fortunately for me, I passed so nearly through the centre of the aggregation that its attraction as a whole was nearly inoperative. So far as I could judge, the meteors in that part of the ring through which I passed were pretty evenly distributed; and as from the appearance of the first which passed my window to the disappearance of the last four hours elapsed,
