Science in Short ChaptersWilliams, W. Mattieu (William Mattieu)
Science
Science in Short Chapters
Williams, W. Mattieu (William Mattieu)
Science
It appears to me that this unsophisticated conception of radiant
mechanical repulsive force, and its necessary mechanical reaction
on the radiant body, meets all the facts at present revealed by the
experiments of Mr. Crookes and others.
The attraction which occurs when the disc of the radiometer is
surrounded with a considerable quantity of atmospheric matter is
probably due to inequality of atmospheric pressure. The absorbing
face of the disc becomes heated above the temperature of the opposite
face, the film of air in contact with the warmer face rises, leaving
a relatively vacuous space in front. This produces a rush of air from
back to front which carries the radiometer vane with it. When the
exhaustion of the radiometer is carried so far that the residual air
is only just sufficiently dense to neutralize the direct repulsion of
radiation, the neutral point is reached. When exhaustion is carried
beyond this, repulsion predominates.
Taking Mr. Crookes’s estimate of the mechanical energy of solar
radiation at 32 grains per square foot, 2 cwts. per acre, 57 tons per
square mile, etc., and accepting these as they are offered, _i.e._,
merely as provisional and approximate estimates, we are led to a
cosmical inference of the highest importance, one that must materially
modify our interpretations of some of the grandest phenomena of the
universe. Although the estimated sunlight pressure upon the earth, the
three thousand millions of tons, is too small a fraction of the earth’s
total weight to effect an easily measurable increase of the length of
our year, the case is quite otherwise with the asteroids and the zones
of meteoric matter revolving around the sun.
The mechanical repulsion of radiation is a superficial action, and
must, therefore, vary with the amount of surface exposed, while that of
gravitation varies with the mass. Thus the ratio of radiant repulsion
to the attraction of gravitation goes on increasing with the subdivison
of masses, and becomes an important fraction in the case of the smaller
bodies of the solar system. A zone of meteorites traveling around
the sun would be broken up, sifted, and sorted into different orbits,
according to their diameters, if this superficial repulsion operated
against gravitation without any compensating agency. Gravitation would
be opposed in various degrees, neutralized, and, in the case of cosmic
dust, even reversed. Comets presenting so large a surface in proportion
to their mass would either be driven away altogether or forced to move
in orbits utterly disobedient to present calculations. This would occur
if the inter-planetary spaces were as nearly vacuous as the torsion
instrument with which Mr. Crookes made his measurements.
Public-domain text, read in full here on John Shaqi.
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