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
"'4. At what precise moment will the moon present herself in the most
favourable position to be reached by the projectile?
"'5. What point in the heavens ought the cannon to be aimed at which is
intended to discharge the projectile?
"'6. What place will the moon occupy in the heavens at the moment of the
projectile's departure?'
"Regarding the _first_ question, 'Is it possible to transmit a projectile
up to the moon?'
"_Answer_.—Yes; provided it possess an initial velocity of 1200 yards
per second; calculations prove that to be sufficient. In proportion as
we recede from the earth the action of gravitation diminishes in the
inverse ratio of the square of the distance; that is to say, _at three
times a given distance the action is nine times less._ Consequently, the
weight of a shot will decrease, and will become reduced to zero at the
instant that the attraction of the moon exactly counterpoises that of
the earth; that is to say, at 47/52 of its passage. At that instant the
projectile will have no weight whatever; and, if it passes that point,
it will fall into the moon by the sole effect of the lunar attraction.
The _theoretical possibility_ of the experiment is therefore absolutely
demonstrated; its success must depend upon the power of the engine
employed.
"As to the _second question_, 'What is the exact distance which separates
the earth from its satellite?'
"_Answer._—The moon does not describe a circle round the earth, but
rather an _ellipse_, of which our earth occupies one of the _foci;_ the
consequence, therefore, is, that at certain times it approaches nearer
to, and at others it recedes farther from, the earth; in astronomical
language, it is at one time in _apogee_, at another in _perigee._ Now the
difference between its greatest and its least distance is too considerable
to be left out of consideration. In point of fact, in its apogee the moon
is 247,552 miles, and in its perigee, 218,657 miles only distant; a fact
which makes a difference of 28,895 miles, or more than one ninth of the
entire distance. The perigee distance, therefore, is that which ought to
serve as the basis of all calculations.
"To the _third_ question:—
"_Answer._—If the shot should preserve continuously its initial velocity
of 12,000 yards per second, it would require little more than nine
hours to reach its destination; but, inasmuch as that initial velocity
will be continually decreasing, it results that, taking everything into
consideration, it will occupy 300,000 seconds, that is 83hrs. 20m. in
reaching the point where the attraction of the earth and moon will be
_in equilibrio._ From this point it will fall into the moon in 50,000
seconds, or 13hrs. 53m. 20sec. It will be desirable, therefore, to
discharge it 97hrs. 13m. 20sec. before the arrival of the moon at the
point aimed at.
"Regarding question _four_, 'At what precise moment will the moon present
herself in the most favourable position, &c.?'
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