The Story of the Solar SystemChambers, George F. (George Frederick)
Science
The Story of the Solar System
Chambers, George F. (George Frederick)
Solar system
The variations of the spots which we now recognise naturally recall
those obscurations of the Sun which are recorded in history; but it is
necessary to accept many of these with caution. A great number of these
phenomena which attracted the attention of people in early times are
only eclipses badly observed and still more badly described. In other
instances the obscuration has been produced by very protracted dry fogs.
It is probably to this last-named cause that we must ascribe the
obscuration which, according to Kepler and Gemma Frisius, took place in
1547.
It was in some such way as this that, according to Virgil (Georg. i,
630), who has echoed a tradition which he found in history, the Sun was
obscured at the death of Cæsar:—
Ille etiam extincto miseratus Cæsare Romam
Quum caput obscura nitidum ferrugine texit,
Impiaque æternam timuerunt sæcula noctem.
In the year 553 A.D., and again in the year 626 A.D. the Sun remained
obscured for several months; but these facts (if facts they are) besides
being ill-observed, and clothed, no doubt, in extremely exaggerated
language, are brought to our notice as having occurred at epochs which
are quite independent of one another, whilst the variations in the
markings on the Sun, which we have just been talking about, present an
almost mathematical regularity of sequence.
We must now institute some inquiries as to the causes of the periodicity
of the spots. A periodicity so well established would naturally invite
astronomers to seek the causes which produced it. The presence of spots
only in the Zodiacal regions led Galileo to suspect the existence of
some relation between the spots and the position of the planets; but
there is in this a mere surmise, which, when it was made, had nothing to
justify it, and it is still impossible for us to say anything for
certain on the point. The determining cause of the periodicity may exist
in the interior of the Sun, and may depend on circumstances which will
for ever remain unknown to us. Or it may be something external: it may
be due after all to the influence of the planets. It remains for us,
therefore, to search and see if any such influence can be traced.
Public-domain text, read in full here on John Shaqi.
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