The story of the universe. Volume 1 (of 4) : $b The starry skies
History
The story of the universe. Volume 1 (of 4) : $b The starry skies
Astronomy; Earth (Planet); Natural history
Now, whatever opinion we form as to the exact character of the
system of bodies pointed to by the researches of Leverrier and
Baxendell—whether we suppose that system to form a zone around
the sun, or that (as I believe) the system is merely due to the
aggregation of meteoric perihelia in the sun’s neighborhood—we may
be quite certain of this, that during a total solar eclipse the
system could not fail to become visible. Hence there is a double
objection to the view put forward by Mr. Lockyer and others. In the
first place, it fails to account for the appearance presented by
the corona; in the second place, it fails to render an account of
the implied non-appearance of the system which, according to the
researches of Leverrier and Baxendell, circles around the sun.
[Illustration: Fig. 34.—Scale of Planets
_Jupiter and Saturn are shown in their true axial positions, Uranus
and Neptune in the axial positions inferred from the motions of their
satellites_]
We know that the sun is the sole source whence light and heat are
plentifully supplied to the worlds which circle around him. The
question immediately suggests itself—Whence does the sun derive
those amazing stores of force from whence he is continually supplying
his dependent worlds? We know that, were the sun a mass of burning
matter, he would be consumed in a few thousand years. We know that,
were he simply a heated body, radiating light and heat continually
into space, he would in like manner have exhausted all his energies
in a few thousand years—a mere day in the history of his system.
Whence, then, comes the enormous supply of force which he has
afforded for millions on millions of years, and which also our reason
tells us he will continue to afford while the worlds which circle
around him have need of it—in other words, for countless ages to come?
Now, there are two ways in which the solar energies might be
maintained. The mere contraction of the solar substance, Helmholtz
tells us, would suffice to supply such enormous quantities of heat
that, if the heat actually given out by the sun were due to this
cause alone, there would not, in many thousands of years, be any
perceptible diminution of the sun’s diameter. But, secondly, the
continual downfall of meteors upon the sun would cause an emission
of heat in quantities vast enough for the wants of all the worlds
circling round him; while his increase of mass from this cause would
not be rendered perceptible in thousands of years, either by any
change in his apparent size or by changes in the motions of his
family of worlds.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account