Omega: The Last days of the WorldFlammarion, Camille
Philosophy
Omega: The Last days of the World
Flammarion, Camille
End of the world -- Fiction; Science fiction
When the threatening star arrived at a distance from the sun equal to
that of Mars, the popular fear was no longer a vague apprehension; it
took definite form, based, as it was, upon the exact knowledge of the
comet’s rate of approach. Thirty-four thousand meters per second meant
2040 kilometers per minute, or 122,400 kilometers per hour!
[Illustration]
As the distance of the orbit of Mars from that of the earth is only
76,000,000 of kilometers, at the rate of 122,400 kilometers an hour,
this distance would be covered in 621 hours, or about twenty-six days.
But, as the comet approached the sun, its velocity would increase, since
at the distance of the earth its velocity would be 41,660 meters per
second. In virtue of this increase of speed, the distance between the
two orbits would be traversed by a comet in 558 hours, or in
twenty-three days, six hours.
But the earth at the moment of meeting with the comet, would not be
exactly at that point of its orbit intersected by a line from the comet
to the sun, because the former was not advancing directly toward the
latter; the collision, therefore, would not take place for nearly a week
later, namely: at about midnight on Friday, the 13th of July. It is
unnecessary to add that under such circumstances the usual arrangements
for the celebration of the national fête of July 14th had been
forgotten. National fête! No one thought of it. Was not that date far
more likely to mark the universal doom of men and things? As to that,
the celebration by the French of the anniversary of that famous day had
lasted—with some exceptions, it is true—for more than five centuries:
even among the Romans anniversaries had never been observed for so long
a period, and it was generally agreed that the 14th of July had outlived
its usefulness.
It was now Monday, the 8th of July. For five days the sky had been
perfectly clear, and every night the fan-like comet hovered in the sky
depths, its head, or nucleus, distinctly visible and dotted with
luminous points which might well be solid bodies several kilometers in
diameter, and which, according to the calculations, would be the first
to strike the earth, the tail being in a direction away from the sun and
in the present instance behind and obliquely situated with reference to
the direction of motion. The new star blazed in the constellation of
Pisces. According to observations taken on the preceding evening, July
8th, its exact position was: right ascension, 23h., 10m., 32s.;
declination north, 7°, 36´, 4˝. The tail lay entirely across the
constellation of Pegasus. The comet rose at 9h., 49m. and was visible
all night long.
Public-domain text, read in full here on John Shaqi.
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