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
Had the axis of the earth been perpendicular to the plane of the
ecliptic, then the sun would always have appeared to move in the
equator, the days would every where have been equal to the nights, and
there could have been no change of seasons. On the other hand, had the
inclination of the ecliptic to the equator been much greater than it is,
the vicissitudes of the seasons would have been proportionally greater,
than at present. Suppose, for instance, the equator had been at right
angles to the ecliptic, in which case, the poles of the earth would have
been situated in the ecliptic itself; then, in different parts of the
earth, the appearances would have been as follows: To a spectator on the
_equator_, (where all the circles of diurnal revolution are
perpendicular to the horizon,) the sun, as he left the vernal equinox,
would every day perform his diurnal revolution in a smaller and smaller
circle, until he reached the north pole, when he would halt for a
moment, and then wheel about and return to the equator, in a reverse
order. The progress of the sun through the southern signs, to the south
pole, would be similar to that already described. Such would be the
appearances to an inhabitant of the equatorial regions. To a spectator
living in an _oblique_ sphere, in our own latitude, for example, the
sun, while north of the equator, would advance continually northward,
making his diurnal circuit in parallels further and further distant from
the equator, until he reached the circle of perpetual apparition; after
which, he would climb, by a spiral course, to the north star, and then
as rapidly return to the equator. By a similar progress southward, the
sun would at length pass the circle of perpetual occultation, and for
some time (which would be longer or shorter, according to the latitude
of the place of observation) there would be continual night. To a
spectator on the _pole_ of the earth and under the pole of the heaven,
during the long day of six months, the sun would wind its way to a point
directly over head, pouring down upon the earth beneath not merely the
heat of the torrid zone, but the heat of a torrid noon, accumulating
without intermission.
The great vicissitudes of heat and cold, which would attend these
several movements of the sun, would be wholly incompatible with the
existence of either the animal or the vegetable kingdom, and all
terrestrial Nature would be doomed to perpetual sterility and
desolation. The happy provision which the Creator has made against such
extreme vicissitudes, by confining the changes of the seasons within
such narrow bounds, conspires with many other express arrangements in
the economy of Nature, to secure the safety and comfort of the human
race.
Public-domain text, read in full here on John Shaqi.
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