Astronomy in a nutshell : $b The chief facts and principles explained in popular language for the general reader and for schoolsServiss, Garrett Putman
Science
Astronomy in a nutshell : $b The chief facts and principles explained in popular language for the general reader and for schools
Serviss, Garrett Putman
Astronomy -- Juvenile literature
(The same thing occurs with the moon, though to a less degree owing to
the smaller eccentricity of the moon's orbit, which, however, is
sufficient to enable us to see at one time a short distance round one
side of the moon and at another time a short distance round the opposite
side.) This phenomenon is known as libration. Mercury apparently
possesses an atmosphere, but we know nothing certain concerning its
density.
* * * * *
The next planet, in the order of distance from the sun, is Venus, whose
average distance is 67,200,000 miles. The orbit of Venus is remarkable
for its small eccentricity, so that the difference between its greatest
and least distances from the sun is less than a million miles. The
period, or year, of Venus is 225 of our days. Owing to her situation
closer to the sun, she gets nearly twice as much light and heat as the
earth gets. In size Venus is remarkably like the earth, her diameter
being 7713 miles, which differs by only 205 miles from the mean diameter
of the earth. Her axis is nearly perpendicular to the plane of her
orbit. Her globe is a more perfect sphere than that of the earth, being
very little flattened at the poles or swollen at the equator. Although
Venus, like Mercury, has no satellite, her mean density has been
calculated by other means, and is found to be 0.89 that of the earth.
From this, in connection with her measured diameter, it is easy to
deduce her mass, and the force of gravity on her surface. The latter
comes out at about 0.85 that of the earth, _i. e._ a body weighing 100
pounds on the earth would weigh 85 pounds if removed to Venus. She
possesses an atmosphere denser and more extensive than would
theoretically have been expected—indicating, perhaps, a difference of
constitution. Her atmosphere has been estimated to be twice as dense as
ours, a great advantage, it may be remarked, from the point of view of
aëronautics. But this dense and abundant atmosphere renders Venus a very
difficult object for the telescope on account of the brilliance of its
reflection. In consequence, we know but little of the surface of the
planet.
Public-domain text, read in full here on John Shaqi.
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