The Story of the Solar SystemChambers, George F. (George Frederick)
Science
The Story of the Solar System
Chambers, George F. (George Frederick)
Solar system
When several spots appear simultaneously, they describe in the same
period of time similar paths which are sensibly parallel to one another
although they may be in very different latitudes. The conclusion from
this is inevitable, that spots are not bodies independent of the Sun, as
satellites would be, but that they are connected with the Sun’s surface,
and are affected by its movement of rotation. If we make every day for a
few days in succession a drawing of the Sun’s disc with any spots that
are visible duly marked thereon, we shall see that their apparent
progress is rapid near the centre of the Sun, but slow near either limb.
These differences, however, are apparent and not real, for their
movement appears to us to take place along a plane surface, whilst in
reality it takes place along a circle parallel to the solar equator. The
spots in approaching the Sun’s W. limb, if they happen to seem somewhat
circular in form when near the centre, first become oval, and then seem
to contract almost into mere lines. These changes are simple effects of
perspective, and are to be explained in the same manner as the apparent
decrease in the size of many of the spots is often explicable. But this
condition of things proves, however, that the spots belong to the actual
surface of the Sun, for, on a contrary supposition, we should have to
regard them as circular bodies greatly flattened like lozenges, and this
would be contrary to all we know of the forms affected by the heavenly
bodies. Of course besides the apparent changes of form just alluded to
as the effect of perspective, it is abundantly certain that solar spots
often undergo very real changes of form, not only from day to day, but
in the course of a few hours. Several spots will often become
amalgamated into one, and it was ephemeral changes of this character
which hindered generally the early observers from determining with
precision the duration of the Sun’s rotation.
Public-domain text, read in full here on John Shaqi.
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