Astronomy of To-day: A Popular Introduction in Non-Technical LanguageDolmage, Cecil Goodrich Julius
Science
Astronomy of To-day: A Popular Introduction in Non-Technical Language
Dolmage, Cecil Goodrich Julius
Astronomy
The marked difference in the brightness between the two planets has
already been alluded to. The surface of Venus is, indeed, about five
times as bright as that of Mercury. The actual brightness of Mercury is
about equivalent to that of our moon, and astronomers are, therefore,
inclined to think that it may resemble her in having a very rugged
surface and practically no atmosphere. This probable lack of atmosphere
is further corroborated by two circumstances. One of these is that when
Mercury is just about to transit the face of the sun, no ring of
diffused light is seen to encircle its disc as would be the case if it
possessed an atmosphere. Such a lack of atmosphere is, indeed, only to
be expected from what is known as the _Kinetic Theory of Gases_.
According to this theory, which is based upon the behaviour of various
kinds of gas, it is found that these elements tend to escape into space
from the surface of bodies whose force of gravitation is weak. Hydrogen
gas, for example, tends to fly away from our earth, as any one may see
for himself when a balloon rises into the air. The gravitation of the
earth seems, however, powerful enough to hold down other gases, as, for
instance, those of which the air is chiefly composed, namely, oxygen and
nitrogen. In due accordance with the Kinetic theory, we find the moon
and Mercury, which are much about the same size, destitute of
atmospheres. Mars, too, whose diameter is only about double that of the
moon, has very little atmosphere. We find, on the other hand, that
Venus, which is about the same size as our earth, clearly possesses an
atmosphere, as just before the planet is in transit across the sun, the
outline of its dark body is seen to be surrounded by a bright ring of
light.
The results of telescopic observation show that more markings are
visible on Mercury than on Venus. The intense brilliancy of Venus is,
indeed, about the same as that of our white clouds when the sun is
shining directly upon them. It has, therefore, been supposed that the
planet is thickly enveloped in cloud, and that we do not ever see any
part of its surface, except perchance the summit of some lofty mountain
projecting through the fleecy mass.
With regard to the great brilliancy of Venus, it may be mentioned that
she has frequently been seen in England, with the naked eye in full
sunshine, when at the time of her greatest brightness. The writer has
seen her thus at noonday. Needless to say, the sky at the moment was
intensely blue and clear.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account