Side-Lights on Astronomy and Kindred Fields of Popular ScienceNewcomb, Simon
Science
Side-Lights on Astronomy and Kindred Fields of Popular Science
Newcomb, Simon
Astronomy; Compass; Flying-machines; Hyperspace; Learning and scholarship; Rain-making
The most inexplicable feature of all is the rapid formation of a nebula
around this star. In the first photographs of the latter, the
appearance presented is simply that of an ordinary star. But, in the
course of three or four months, the delicate photographs taken at the
Lick Observatory showed that a nebulous light surrounded the star, and
was continually growing larger and larger. At first sight, there would
seem to be nothing extraordinary in this fact. Great masses of
intensely hot vapor, shining by their own light, would naturally be
thrown out from the star. Or, if the star had originally been
surrounded by a very rare nebulous fog or vapor, the latter would be
seen by the brilliant light emitted by the star. On this was based an
explanation offered by Kapteyn, which at first seemed very plausible.
It was that the sudden wave of light thrown out by the star when it
burst forth caused the illumination of the surrounding vapor, which,
though really at rest, would seem to expand with the velocity of light,
as the illumination reached more and more distant regions of the
nebula. This result may be made the subject of exact calculation. The
velocity of light is such as would make a circuit of the earth more
than seven times in a second. It would, therefore, go out from the star
at the rate of a million of miles in between five and six seconds. In
the lapse of one of our days, the light would have filled a sphere
around the star having a diameter more than one hundred and fifty times
the distance of the sun from the earth, and more than five times the
dimensions of the whole solar system. Continuing its course and
enlarging its sphere day after day, the sight presented to us would
have been that of a gradually expanding nebulous mass--a globe of faint
light continually increasing in size with the velocity of light.
The first sentiment the reader will feel on this subject is doubtless
one of surprise that the distance of the star should be so great as
this explanation would imply. Six months after the explosion, the globe
of light, as actually photographed, was of a size which would have been
visible to the naked eye only as a very minute object in the sky. Is it
possible that this minute object could have been thousands of times the
dimensions of our solar system?
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