Astronomy of To-day: A Popular Introduction in Non-Technical LanguageDolmage, Cecil Goodrich Julius
Science
Astronomy of To-day: A Popular Introduction in Non-Technical Language
Dolmage, Cecil Goodrich Julius
Astronomy
unsettle its newly acquired orbit, and send it out again into the
celestial spaces.
With regard to the matter of which comets are composed, the spectroscope
shows the presence in them of hydrocarbon compounds (a notable
characteristic of these bodies), and at times, also, of sodium and iron.
Some of the light which we get from comets is, however, merely reflected
sunlight.
The fact that the tails of comets are always directed away from the sun,
has given rise to the idea that this is caused by some repelling action
emanating from the sun itself, which is continually driving off the
smallest particles. Two leading theories have been formulated to account
for the tails themselves upon the above assumption. One of these, first
suggested by Olbers in 1812, and now associated with the name of the
Russian astronomer, the late Professor Brédikhine, who carefully worked
it out, presumes an electrical action emanating from the sun; the other,
that of Arrhenius, supposes a pressure exerted by the solar light in its
radiation outwards into space. It is possible, indeed, that repelling
forces of both these kinds may be at work together. Minute particles are
probably being continually produced by friction and collisions among the
more solid parts in the heads of comets. Supposing that such particles
are driven off altogether, one may therefore assume that the so-called
captured comets are disintegrating at a comparatively rapid rate. Kepler
long ago maintained that "comets die," and this actually appears to be
the case. The ordinary periodic ones, such, for instance, as Encke's
Comet, are very faint, and becoming fainter at each return. Certain of
these comets have, indeed, failed altogether to reappear. It is notable
that the members of Jupiter's comet family are not very conspicuous
objects. They have small tails, and even in some cases have none at all.
The family, too, does not contain many members, and yet one cannot but
suppose that Jupiter, on account of his great mass, has had many
opportunities for making captures adown the ages.
Of the two theories to which allusion has above been made, that of
Brédikhine has been worked out so carefully, and with such a show of
plausibility, that it here calls for a detailed description. It appears
besides to explain the phenomena of comets' tails so much more
satisfactorily than that of Arrhenius, that astronomers are inclined to
accept it the more readily of the two. According to Brédikhine's theory
the electrical repulsive force, which he assumes for the purposes of his
argument, will drive the minutest particles of the comet in a direction
away from the sun much more readily than the gravitative action of that
body will pull them towards it. This may be compared to the ease with
which fine dust may be blown upwards, although the earth's gravitation
is acting upon it all the time.
Public-domain text, read in full here on John Shaqi.
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