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
पृष्ठ 83, कुल 548 में से
संदर्भ में पढ़ें52 • THE ARCTIC HOME IN THE VEDAS.
and the stars will now appear to move in circles inclined to
his horizon, as shown in the figure by the black lines AA', BH'
and CC'. Some of the stars, viz., those that are situated in the
part of the celestial dome represented by H'PB, will be visible
throughout the night, as their circles of revolution will be above
the horizon H'C'D'H. But all the stars, whose Polar distance
is greater than PB or PH', will, in their daily revolution, be partly
above and partly below the horizon. For instance, the stars at
C and D will describe circles, some portions of which will be
below the horizon H'H. In other words, the appearance of the
visible celestial hemisphere to a person, whose zenith is at
Z, will be different from the appearance presented by the
heavens to an observer at the North Pole. The stars will not
now revolve in horizontal planes, but obliquely. A great number
of them would be circumpolar and visible during the whole
night, but the remaining will rise and set as with us in the
tropics, moving in oblique circles. When Z is very near P, only
a few stars will rise and set in this way, and the difference will
not be a marked one ; but as Z is removed further south, the
change will become more and more apparent.
Similar modifications will be introduced in the duration of
day and night, when the observer's position is shifted to the
south of the terrestrial North Pole. This will be clear by a
reference to the figure on the next page. Let P be the celestial
North Pole, and Q'Q the celestial equator. Then since the
sun moves in the ecliptic E'E, which is inclined at an angle
of about 23½° (23° 28' ) to the equator, the circles T'E and E'T
will correspond with the terrestrial circles of latitude, called the
Tropics, and the circle AC with the Arctic Circle on the terres-
trial globe. Now as the sun moves in the ecliptic E'E, in his
annual course he will always be twice over-head for an observer