,--which was still well above the sea--and immediately round the
terrestrial horizon, on which rested a ring of sunlit azure sky,
broken here and there by clouds. In every other direction I seemed to
be looking not merely upon a black or almost black sky, but into close
surrounding darkness. Amid this darkness, however, were visible
innumerable points of light, more or less brilliant--the stars--which
no longer seemed to be spangled over the surface of a distant vault,
but rather scattered immediately about me, nearer or farther to the
instinctive apprehension of the eye as they were brighter or fainter.
Scintillation there was none, except in the immediate vicinity of the
eastern horizon, where I still saw them through a dense atmosphere. In
short, before thirty minutes had elapsed since the start, I was
satisfied that I had passed entirely out of the atmosphere, and had
entered into the vacancy of space--if such a thing as vacant space
there be.

At this point I had to cut off the greater part of the apergy and
check my speed, for reasons that will be presently apparent. I had
started in daylight in order that during the first hundred miles of my
ascent I might have a clear view of the Earth's surface. Not only did
I wish to enjoy the spectacle, but as I had to direct my course by
terrestrial landmarks, it was necessary that I should be able to see
these so as to determine the rate and direction of the Astronaut's
motion, and discern the first symptoms of any possible danger. But
obviously, since my course lay generally in the plane of the ecliptic,
and for the present at least nearly in the line joining the centres of
the Earth and Sun, it was desirable that my real journey into space
should commence in the plane of the midnight meridian; that is, from
above the part of the Earth's surface immediately opposite the Sun. I
had to reach this line, and having reached it, to remain for some time
above it. To do both, I must attain it, if possible, at the same
moment at which I secured a westward impulse just sufficient to
counterbalance the eastward impulse derived from the rotation of the
Earth;--that is, in the latitude from which I started, a thousand
miles an hour. I had calculated that while directing through the main
bar a current of apergy sufficient to keep the Astronaut at a fixed
elevation, I could easily spare for the eastward conductor sufficient
force to create in the space of one hour the impulse required, b