The starry skies : $b or, First lessons on the sun, moon and stars — John Shaqi
The starry skies : $b or, First lessons on the sun, moon and starsGiberne, Agnes
General
The starry skies : $b or, First lessons on the sun, moon and stars
Giberne, Agnes
Astronomy -- Juvenile literature
Dark spots on the Sun are very often to be seen; sometimes only through
a telescope, but now and then one is large enough to be seen with no
such help--by the eye alone.
It was by means of these spots that the Sun was first found to spin
upon its axis, just as our Earth does.
A black spot would be noticed upon one side of the Sun’s face. It would
be seen slowly to cross over, and to disappear on the other side.
Nearly a fortnight would be needed for the journey across, and for
another fortnight, or nearly so, the spot would be hidden behind the
Sun. After which it would turn up again, on the same side as at first,
and in the very same place. Then once more it would travel across and
disappear, and in another fortnight it would come round over to its
starting-point.
If only a single spot had behaved in this way it might have meant
little. But when numbers of spots did the very same thing, time after
time, it became clear that the great body of the sun was whirling
round, carrying the spots with it.
The Sun, like the Earth, has a north pole, and a south pole, and an
equator.
We give the name “north pole” to one end of the axis or line on which
he spins, and the name “south pole” to the other end of that axis. And
we give the name “equator” to a line exactly round the middle of the
Sun, half-way between his two poles.
Most of the spots which we see are somewhere near the Sun’s equator,
not very near to his north pole or to his south pole.
They come and go and change their shapes, and get bigger or
smaller--sometimes slowly, sometimes very fast. A spot may appear and
grow and vanish again in one day, or it may stay on for days and weeks,
and even months, hardly altering at all, only journeying round and
round the Sun.
These things show us that the great Sun spins round upon his axis: and
that for each spin he takes about twenty-five or twenty-six days.
But the whirling round of the Sun means no Day and Night by turns to
him, for the whole of the Sun is always light--bright with his own
radiance.
Once upon a time it used to be thought that the Sun spots were perhaps
_raised_ things--dark objects standing high, like mountains. And I will
tell you why this idea was given up.
Take an empty cup, and hold it before your eyes, with the open part
turned full towards you. The cup must be held as if lying on its
side--not with the mouth upwards, as it would stand on a table. You can
see, thus, the full circle of the opening, and the whole empty inside.
Next, move it a little way to the right from before your face, turning
it slightly away, and you will then see no longer the whole inside, but
only a part: and the round opening will have an oval look.
Turn it still further, and you will see a very narrow oval opening, and
hardly any of the inside.
Now this is just how the spots seem to behave as they cross the Sun.
Public-domain text, read in full here on John Shaqi.
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