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वेदों की प्राचीनता एवं काल-निर्णय / ओरायन (लोकमान्य बाल गंगाधर तिलक - खगोलीय वैदिक शोध)

वेदों की प्राचीनता एवं काल-निर्णय / ओरायन (लोकमान्य बाल गंगाधर तिलक - खगोलीय वैदिक शोध)

The Orion and The Arctic Home in the Vedas by Lokmanya Tilak

लोकमान्य बाल गंगाधर तिलक द्वारा

DevanagariHindipublished548 पृष्ठ

पृष्ठ 61, कुल 548 में से

संदर्भ में पढ़ें
पृष्ठ 61

30 THE ARCTIC HOME IN THE VEDAS.
There is another consideration which we must take into
account in estimating the severity of winter or the mildness of
summer in any hemisphere. If the summer be defined to be the
period of time required by the earth to travel from one equinoctial
point Q' to another equinoctial point Q, this interval cannot always
be constant for we have seen that the winter and summer points
(P and A), and with them the equinoctial points (Q and Q') are
not stationary, but revolve along the orbit once in 21,000 years.
Had the orbit been a circle, the lines qq' and pa will have always
divided it in equal parts. But the orbit being an ellipse these
two sections are unequal. For instance, suppose that the winter
occurs when the earth is at P, then the duration of the summer
will be represented by Q'AQ, but when the winter occurs at A
the summer time will be represented by QPQ', a segment of the
ellipse necessarily smaller than Q'AQ. This inequality is due to
the ellipticity of the orbit, and the more elongated or elliptic the
orbit is, the greater will be the difference between the durations
of summer and winter in a hemisphere. Now the ellipticity of
the orbit is measured by the difference between the mean and
the greatest distance of the earth from the sun, and is called in
astronomy the eccentricity of the earth's orbit. This eccentricity
of the earth's orbit is not a constant quantity, but varies, though
slowly, in course of time, making the orbit more and more
elliptical, until it reaches a maximum value, when it again begins
to reduce until the original value is reached. The duration of
summer and winter in a hemisphere, therefore, varies as the
value of the eccentricity of the earth's orbit at that time; and it
has been stated above that the difference between the duration of
summer and winter also depends on the position of the equinoctial
line, or of the points in the earth's orbit at which the winter and
the summer in a hemisphere occur. As the joint result of