New Lands, by Charles Fort, , at sacred-texts.com
Our data indicate that the planets are circulating adjacencies.
Almost do we now conceive of a difficulty of the future as being not how to reach the planets, but how to dodge them. Especially do we warn aviators away from that rhinoceros of the skies, Mercury. I have a note somewhere upon one of the wickedest-looking horns in existence, sticking out far from Mercury. I think it was Mr. Whitmell who made this observation. I'd like to hear Andrew Barclay's opinion upon that. I'd like to hear Capt. Noble's.
If sometimes does the planet Mars almost graze this earth, as is not told by the great telescopes, which are only millionaires’ memorials, or, at least, which reveal but little more than did the little spy glasses used by Burnham and Williams and Beer and Mädler—but if periodically the planet Mars comes very close to this earth, and, if Mars, an island with perhaps no more surface-area than has England, but likely enough inhabited, like England—
June 19, 1875—opposition of Mars.
Flashes that were seen in the sky upon the 25th of June, 1875, by Charles Gape, of Scole, Norfolk (Eng. Mec., 21-488). The Editor of Symons’ Met. Mag. (see vol. 10-116) was interested, and sent Mr. Gape some questions, receiving answers that nothing had appeared in the local newspapers upon the subject, and that nothing
could be learned of a display of fireworks, at the time. To Mr. Gape the appearances seemed to be meteoric.
The year 1877—climacteric opposition of Mars.
There were some discoveries.
We have at times wondered how astronomers spend their nights. Of course, according to many of his writings upon the subject, Richard Proctor had an excellent knowledge of whist. But in the year 1877, two astronomers looked up at the sky, and one of them discovered the moons of Mars, and the other called attention to lines on Mars—and, if for centuries, the moons of Mars could so remain unknown to all inhabitants of this earth except, as it were, Dean Swift—why, it is no wonder that we so respectfully heed some of the Dean's other intuitions, and think that there may be Liliputians, or Brobdingnagians, and other forms not conventionally supposed to be. As to our own fields of data, I have a striking number of notes upon signal-like appearances upon the moon, in the year 1877, but have notes upon only one occurrence that, in our interests, may relate to Mars. The occurrence is like that of July 31, 1813, and June 19, 1875.
Sept. 5, 1877—opposition of Mars.
Sept. 7, 1877—lights appeared in the sky of Bloomington, Indiana. They were supposed to be meteoric. They appeared and disappeared, at intervals of three or four seconds; darkness for several minutes; then a final flash of light. See Sci. Amer., 37-193.
That all luminous objects that are seen in the sky when the planet Venus is nearest may not be Venus; may not be fire-balloons:
In the Dundee Advertiser, Dec. 22, 1882, it is said that, between 10 and 11 A.M., December 21, at Broughty Ferry, Scotland, a correspondent had seen an unknown luminous body near and a little above the sun. In the Advertiser, December 25, is published a letter from someone who says that this object had been seen at Dundee, also; that quite certainly it was the planet Venus and "no other." In Knowledge, 2-489, this story is told by a writer who says that undoubtedly the object was Venus. But, in Knowledge, 3-13, the astronomer J. E. Gore writes that the object could
not have been Venus, which upon this date was 1 h. 33 m., R. A., west of the sun. The observation is reviewed in L’Astronomie, 1883-109. Here it is said that the position of Mercury accorded better. Reasonably this object could not have been Mercury: several objections are comprehended in the statement that superior conjunction of Mercury had occurred upon December 16.
Upon Feb. 3, 1884, M. Staevert, of the Brussels Observatory, saw, upon the disc of Venus, an extremely brilliant point (Ciel et Terre, 5-127). Nine days later, Niesten saw just such a point of light as this, but at a distance from the planet. If no one had ever heard that such things cannot be, one might think that these two observations were upon something that had been seen leaving Venus and had then been seen farther along. Upon the 3rd of July, 1884, a luminous object was seen moving slowly in the sky of Norwood, N. Y. It had features that suggest the structural: a globe the size of the moon, surrounded by a ring; two dark lines crossing the nucleus (Science Monthly, 2-136). Upon the 26th of July, a luminous globe, size of the moon, was seen at Cologne; it seemed to be moving upward from this earth, then was stationary "some minutes," and then continued upward until it disappeared (Nature, 30-360). And in the English Mechanic, 40-130, it is not said that a luminous vessel that had sailed out from Venus, in February, visiting this earth, where it was seen in several places, was seen upon its return to the planet, but it is said that an observer in Rochester, N. Y., had, upon August 17, seen a brilliant point upon Venus.