The Prehistoric World; Or, Vanished RacesAllen, Emory Adams
History
The Prehistoric World; Or, Vanished Races
Allen, Emory Adams
Archaeology; Indians; Prehistoric peoples
In common language we would state that the shape of the path of
the earth around the sun was sometimes much more elongated and
elliptical than at others. The line drawn through the longest
part of an ellipse is called the major axis. Now the sun does not
occupy the center of this line, but is placed to one side of it;
or, in other words, occupies one focus of the ellipse. It will
thus be seen that the earth, at one time during its yearly
journey, is considerably nearer to the sun than at others. The
point where it approaches nearest the sun is called _Perihelion,_
and the point where it reaches the greatest distance from the sun
is called its _Aphelion._ It will be readily seen that the more
elliptical its orbit becomes the greater will be the difference
between the perihelion and aphelion distance of the sun. At
present the earth is about three millions of miles nearer the sun
in perihelion than in aphelion. But we must remember the orbit of
the earth is now nearly circular. There have been times in the
past when the difference was about thirteen millions of miles. We
must not forget to add, that the change in the shape of the
earth’s orbit is not a regular increase and decrease between
well-known extremes. It is caused by the attraction of the other
planets. It has been calculated at intervals of ten thousand
years for the last million years. In this way it has been found
that “the intervals between connective turning points are very
unequal in length, and the actual maximum and minimum values of
the eccentricity are themselves variable. In this way it comes
about that some periods of high eccentricity have lasted much
longer than others, and that the orbit has been more elliptical
at some epochs of high eccentricity than at others.”14 We have
just seen that the earth is nearer the sun at one time of the
year than at another. At present the earth passes its perihelion
point in the Winter of the Northern Hemisphere, and its aphelion
point in the Summer. We will for the present suppose that it
always reaches the points at the same season of the year. Let us
see if the diminished distance from the sun in Winter has any
thing to do with the climate.
Public-domain text, read in full here on John Shaqi.
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