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
Once in a while the tiny body of Mercury is seen to creep, as a little
black dot, across the face of the Sun: though this is only visible in a
telescope. Then we have a “Transit of Mercury.” In the last chapter you
were told what is meant by a Transit.
If Mercury were as near to us as our Moon is, he would hide the Sun
from us in his transit just as the Moon does in an eclipse--only more
fully, because Mercury is bigger than our Moon.
In a Transit, as in an Eclipse, there is no real drawing together of
Sun and Planet. Be very clear in your mind about this. Mercury glides
_between_ our Earth and the Sun, but he is just as far as usual from
the Earth on one side and from the Sun on the other side.
If you are gazing at a church-tower a great many miles away, and a bird
near at hand flies between, hiding for a moment that tower from you,
the bird may be said to “eclipse” the tower. But he does not go nearer
to the church. He only moves into the straight line between you and the
tower.
And if, instead of this, a bird some distance off flies between--then
you have a “transit.” The more distant bird cannot hide the
church-tower, but you see his little body pass across it, as a dark
spot.
A transit of Mercury is not common. For though Mercury often passes
between the Earth and the Sun he is not often _exactly_ between. His
oval pathway is not quite on the same level as the Earth’s pathway. So
he is usually a little too high or a little too low for us to see him
against the Sun.
Leaving Mercury behind we come next to the pathway of the planet VENUS.
Mercury was a good deal smaller than our Earth; but Venus is almost
the same size. Instead of being, like Mercury, only some thirty-six
millions of miles away from the Sun, Venus is about sixty-five millions
of miles off. She journeys round him at a rate of some twenty-two
miles each second, and her year lasts about seven months and a half of
Earth-time. In make she is not quite so solid and heavy as our Earth.
Venus in her journey round the Sun, as our Moon travels round the
Earth, is now believed to turn on her axis so very slowly that the same
side is always towards the Sun, and the other side is always turned
away. If this really is so, one half of Venus has an endless day, and
the other half an endless night.
The same state of things may possibly be also true of Mercury.
Both these worlds are believed to have air around them, and Venus
seems to be enwrapped in thick clouds. This helps to explain the great
brilliancy of Venus. Nothing lights up so well in sunshine as masses
of cloud, though of course we on Earth more generally see the dark
_undersides_ of clouds.
So far as we know, Venus is a lonely world. She seems to have no
little moon-friend to journey with her in the sky.
Public-domain text, read in full here on John Shaqi.
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