Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent AstronomersOlmsted, Denison
Science
Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent Astronomers
Olmsted, Denison
Astronomy
Were it not for the power the atmosphere has of dispersing the solar
light, and scattering it in various directions, no objects would be
visible to us out of direct sunshine; every shadow of a passing cloud
would involve us in midnight darkness; the stars would be visible all
day; and every apartment into which the sun had not direct admission
would be involved in the obscurity of night. This scattering action of
the atmosphere on the solar light is greatly increased by the
irregularity of temperature caused by the sun, which throws the
atmosphere into a constant state of undulation; and by thus bringing
together masses of air of different temperatures, produces partial
reflections and refractions at their common boundaries, by which means
much light is turned aside from a direct course, and diverted to the
purposes of general illumination.[6] In the upper regions of the
atmosphere, as on the tops of very high mountains, where the air is too
much rarefied to reflect much light, the sky assumes a black appearance,
and stars become visible in the day time.
Although the atmosphere is usually so transparent, that it is invisible
to us, yet we as truly move and live in a fluid as fishes that swim in
the sea. Considered in comparison with the whole earth, the atmosphere
is to be regarded as a thin layer investing the surface, like a film of
water covering the surface of an orange. Its actual height, however, is
over a hundred miles, though we cannot assign its precise boundaries.
Being perfectly elastic, the lower portions, bearing as they do, the
weight of all the mass above them, are greatly compressed, while the
upper portions having little to oppose the natural tendency of air to
expand, diffuse themselves widely. The consequence is, that the
atmosphere undergoes a rapid diminution of density, as we ascend from
the earth, and soon becomes exceedingly rare. At so moderate a height as
seven miles, it is four times rarer than at the surface, and continues
to grow rare in the same proportion, namely, being four times less for
every seven miles of ascent. It is only, therefore, within a few miles
of the earth, that the atmosphere is sufficiently dense to sustain
clouds and vapors, which seldom rise so high as eight miles, and are
usually much nearer to the earth than this. So rare does the air become
on the top of Mount Chimborazo, in South America, that it is incompetent
to support most of the birds that fly near the level of the sea. The
condor, a bird which has remarkably long wings, and a light body, is the
only bird seen towering above this lofty summit. The transparency of the
atmosphere,--a quality so essential to fine views of the starry
heavens,--is much increased by containing a large proportion of water,
provided it is perfectly dissolved, or in a state of invisible vapor. A
country at once hot and humid, like some portions of the torrid zone,
presents a much brighter and more beautiful view of the moon and stars,
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