The Story of the HeavensBall, Robert S. (Robert Stawell)
History
The Story of the Heavens
Ball, Robert S. (Robert Stawell)
Astronomy
The imaginary sketch in Fig. 36 denotes a section of the earth with a
high mountain thereon.[12] If a cannon were stationed on the top of the
mountain at C, and if the cannonball were fired off in the direction C E
with a moderate charge of powder, the ball would move down along the
first curved path. If it be fired a second time with a heavier charge,
the path will be along the second curved line, and the ball would again
fall to the ground. But let us try next time with a charge still further
increased, and, indeed, with a far stronger cannon than any piece of
ordnance ever yet made. The velocity of the projectile must now be
assumed to be some miles per second, but we can conceive that the speed
shall be so adjusted that the ball shall move along the path C D, always
at the same height above the earth, though still curving, as every
projectile must curve, from the horizontal line in which it moved at the
first moment. Arrived at D, the ball will still be at the same height
above the surface, and its velocity must be unabated. It will therefore
continue in its path and move round another quadrant of the circle
without getting nearer to the surface. In this manner the projectile
will travel completely round the whole globe, coming back again to C and
then taking another start in the same path. If we could abolish the
mountain and the cannon at the top, we should have a body revolving for
ever around the earth in consequence of the attraction of gravitation.
Make now a bold stretch of the imagination. Conceive a terrific cannon
capable of receiving a round bullet not less than 2,000 miles in
diameter. Discharge this enormous bullet with a velocity of about 3,000
feet per second, which is two or three times as great as the velocity
actually attainable in modern artillery. Let this notable bullet be
fired horizontally from some station nearly a quarter of a million miles
above the surface of the earth. That fearful missile would sweep right
round the earth in a nearly circular orbit, and return to where it
started in about four weeks. It would then commence another revolution,
four weeks more would find it again at the starting point, and this
motion would go on for ages.
Do not suppose that we are entirely romancing. We cannot indeed show the
cannon, but we can point to a great projectile. We see it every month;
it is the beautiful moon herself. No one asserts that the moon was ever
shot from such a cannon; but it must be admitted that she moves as if
she had been. In a later chapter we shall enquire into the history of
the moon, and show how she came to revolve in this wonderful manner.
As with the moon around the earth, so with the earth around the sun. The
illustration shows that a circular or nearly circular motion harmonises
with the conception of the law of universal gravitation.
Public-domain text, read in full here on John Shaqi.
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