by my chronometer I should be exactly in the plane of the midnight meridian, or 6500 miles east of my starting-point in space, provided that I put the eastward apergic current in action exactly at 12 P.m. by the chronometer. At 1 A.m. also I should have generated a westward impulse of 1000 miles an hour. This, once created, would continue to exist though the force that created it were cut off, and would exactly counterbalance the opposite rotation impulse derived from the Earth; so that thenceforward I should be entirely free from the influence of the latter, though still sharing that motion of the Earth through space at the rate of nearly nineteen miles per second, which would carry me towards the line joining at the moment of opposition her centre with that of Mars.
All went as I had calculated. I contrived to arrest the Astronaut's motion at the required elevation just about the moment of sunset on the region of the Earth immediately underneath. At 12 P.m., or 24h by the chronometer, I directed a current of the requisite strength into the eastward conductor, which I had previously pointed to the Earth's surface, but a little short of the extreme terrestrial horizon, as I calculated it. At 1 A.m. I found myself, judging by the stars, exactly where I wished to be, and nearly stationary as regarded the Earth. I instantly arrested the eastward current, detaching that conductor from the apergion; and, directing the whole force of the current into the downward conductor, I had the pleasure of seeing that, after a very little adjustment of the helm, the stars remained stationary in the mirror of the metacompass, showing that I had escaped from the influence of the Earth's rotation. It was of course impossible to measure the distance traversed during the invisibility of the Earth, but I reckoned that I had made above 500 miles between 1h. and 2h. A.M., and that at 4h. I was not less than 4800 miles from the surface. With this inference the indication of my barycrite substantially agreed. The latter instrument consisted of a spring whose deflection by a given weight upon the equator had been very carefully tested. Gravity diminishing as the square of the distance from the centre, it was obvious that at about 8000 miles—or 4000 above the Earth's surface—this spring would be deflected only one quarter as much by a given weight as on Earth: at 16,000 miles from the surface, or 20,000 from the centre, one-twenty-fifth as much, and so on. I had graduated the scale accordingly, and it indicated at present a distance somewhat less than 9000 miles from the centre. Having adjusted the helm and set the alarum to wake me in six hours, I lay down upon my bed.
The anxiety and peril of my position had disturbed me very little whilst I was actively engaged either in steering and manipulating my machinery, or in looking upon the marvellous and novel spectacles presented to my eyes; but it now oppressed me in my sleep, and caused me frequently to wake from dreams of a hideous character. Two or three times, on such awaking, I went to examine the metacompass, and on one occasion found it necessary slightly to readjust the helm; the stars by which I steered having moved some second or two to the right of their proper position.
On rising, I completed the circuit which filled my vessel with brilliant light emitted from an electric lamp at the upper part of the stern, and reflected by the polished metallic walls. I then proceeded to get my breakfast, for which, as I had tasted nothing since some hours before the start, I had a hearty appetite. I had anticipated some trouble from the diminished action of gravity, doubting whether the boiling-point at this immense height above the Earth might not be affected; but I found that this depends upon the pressure of the atmosphere alone, and that this pressure was in nowise affected by the absence of gravity. My atmosphere being somewhat denser than that of the Earth, the boiling-point was not 100°, but 101° Cent. The temperature of the interior of the vessel, taken at a point equidistant from the stove and from the walls, was about 5° C.; unpleasantly cool, but still, with the help of a greatcoat, not inconveniently so. I found it absolutely impossible to measure by means of the thermometers I had placed outside the windows the cold of space; but that it falls far short of the extreme supposed by some writers, I confidently believe. It is, however, cold enough to freeze mercury, and to reduce every other substance employed as a test of atmospheric or laboratory temperatures to a solidity which admits of no further contraction. I had filled one outside thermometer with spirit, but this was broken before I looked at it; and in another, whose bulb unfortunately was blackened, and which was filled with carbonic acid gas, an apparent vacuum had been created. Was it that the gas had been frozen, and had sunk into the lower part of the bulb, where it would, of course, be invisible? When I had completed my meal and smoked the very small cigar which alone a prudent consideration for the state of the atmosphere would allow me, the chronometer showed 10 A.m. It was not surprising that by this time weight had become almost non-existent. My twelve stone had dwindled to the weight of a small fowl, and hooking my little finger into the loop of a string hung from a peg fixed near the top of the stern wall, I found myself able thus to support my weight without any sense of fatigue for a quarter of an hour or more; in fact, I felt during that time absolutely no sense of muscular weariness. This state of things entailed only one inconvenience. Nothing had any stability; so that the slightest push or jerk would upset everything that was not fixed. However, I had so far anticipated this that nothing of any material consequence was unfixed, and except that a touch with my spoon upset the egg-cup and egg on which I was about to breakfast, and that this, falling against a breakfast cup full of coffee, overturned that, I was not incommoded. I managed to save the greater part of the beverage, since, the atmospheric pressure being the same though the weight was so changed, lead, and still more china or liquid, fell in the Astronaut as slowly as feathers in the immediate vicinity of the Earth. Still it was a novel experience to find myself able to lean in any direction, and rest in almost any posture, with but the slightest support for the body's centre of gravity; and further to find on experiment that it was possible to remain for a couple of hours with my heels above my head, in the favourite position of a Yankee's lower limbs, without any perceptible congestion of blood or confusion of brain.
I was occupied all day with abstract calculations; and knowing that for some time I could see nothing of the Earth—her dark side being opposite me and wholly obscuring the Sun, while I was as yet far from having entered within the sphere where any novel celestial phenomena might be expected—I only gave an occasional glance at the discometer and metacompass, suppressing of course the electric glare within my vessel, till I awoke from a short siesta about 19h. (7 P.m.) The Earth at this time occupied on the sphere of view a space—defined at first only by the absence of stars—about thirty times greater than the disc of the Moon as seen through a tube; but, being dark, scarcely seemed larger to the eye than the full Moon when on the horizon. But a new method of defining its disc was presently afforded me. I was, in fact, when looking through the lower window, in the same position as regards the Earth as would be an inhabitant of the lunar hemisphere turned towards her, having no external atmosphere interposed between us, but being at about two-thirds of the lunar distance. And as, during an eclipse, the Lunarian would see round the Earth a halo created by the refraction of the Sun's rays in the terrestrial atmosphere—a halo bright enough on most occasions so to illuminate the Moon as to render her visible to us—so to my eyes the Earth was surrounded by a halo somewhat resembling the solar corona as seen in eclipses, if not nearly so brilliant, but, unlike the solar corona, coloured, with a preponderance of red so decided as fully to account for the peculiar hue of the eclipsed Moon. To paint this, unless means of painting light—the one great deficiency which is still the opprobrium of human art—were discovered, would task to the uttermost the powers of the ablest artist, and at best he could give but a very imperfect notion of it. To describe it so that its beauty, brilliancy, and wondrous nature shall be in the slightest degree appreciated by my readers would require a command of words such as no poet since Homer—nay, not Homer himself—possessed. What was strange, and can perhaps be rendered intelligible, was the variation, or, to use a phrase more suggestive and more natural, if not more accurate, the extreme mobility of the hues of this earthly corona. There were none of the efflorescences, if one may so term them, which are so generally visible at four cardinal points of its solar prototype. The outer portion of the band faded very rapidly into the darkness of space; but the edge, though absolutely undefined, was perfectly even. But on the generally rainbow-tinted ground suffused with red—which perhaps might best be described by calling it a rainbow seen on a background of brilliant crimson—there were here and there blotches of black or of lighter or darker grey, caused apparently by vast expanses of cloud, more or less dense. Round the edges of each of these were little irregular rainbow-coloured halos of their own interrupting and variegating the continuous bands of the corona;