From the Earth to the Moon, Direct in Ninety-Seven Hours and Twenty Minutes: and a Trip Round It — John Shaqi
From the Earth to the Moon, Direct in Ninety-Seven Hours and Twenty Minutes: and a Trip Round ItVerne, Jules
Science
From the Earth to the Moon, Direct in Ninety-Seven Hours and Twenty Minutes: and a Trip Round It
Verne, Jules
Manned space flight -- Fiction; Moon -- Fiction; Science fiction; Space flight to the moon -- Fiction; Space ships -- Fiction
As soon as the ignoramuses came to understand as much as the Director of
the Observatory himself knew, they began to worry themselves regarding
her revolution round the earth, whereupon twenty scientific reviews
immediately came to the rescue. They pointed out to them then that the
firmament, with its infinitude of stars, may be considered as one vast
dial-plate, upon which the moon travels, indicating the true time to all
the inhabitants of the earth; that it is during this movement that the
Queen of Night exhibits her different phases; that the moon is _full_
when she is in _opposition_ with the sun, that is when the three bodies
are on the same straight line, the earth occupying the centre; that she
is _new_ when she is in _conjunction_ with the sun, that is, when she
is between it and the earth; and lastly, that she is in her _first_ or
_last_ quarter, when she makes with the sun and the earth an angle of
which she herself occupies the apex.
Regarding the altitude which the moon attains above the horizon, the
letter of the Cambridge Observatory had said all that was to be said
in that respect. Every one knew that this altitude varies according to
the latitude of the observer. But the only zones of the globe in which
the moon passes the zenith, that is, the point directly over the head
of the spectator, are of necessity comprised between the twenty-eighth
parallels and the equator. Hence the importance of the advice to try
the experiment upon some point of that part of the globe, in order that
the projectile might be discharged perpendicularly, and so the soonest
escape the action of gravitation. This was an essential condition to the
success of the enterprise, and continued actively to engage the public
attention.
Regarding the path described by the moon in her revolution round the
earth, the Cambridge Observatory had demonstrated that this path is a
re-entering curve, not a perfect circle, but an ellipse, of which the
earth occupies one of the _foci_. It was also well understood that it is
farthest removed from the earth during its _apogee,_ and approaches most
nearly to it at its _perigee._
Such then was the extent of knowledge possessed by every American on the
subject, and of which no one could decently profess ignorance. Still,
while these true principles were being rapidly disseminated many errors
and illusory fears proved less easy to eradicate.
For instance, some worthy persons maintained that the moon was an ancient
comet which, in describing its elongated orbit round the sun, happened to
pass near the earth, and became confined within her circle of attraction.
These drawing-room astronomers professed so to explain the charred aspect
of the moon—a disaster which they attributed to the intensity of the
solar heat; only, on being reminded that comets have an atmosphere, and
that the moon has little or none, they were fairly at a loss for a reply.
Public-domain text, read in full here on John Shaqi.
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