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Know_files/FINGERPRINTS OF THE GODS.pdf - D Ank Unlimited

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Chapter 11<br />

Intimations of Antiquity<br />

Graham Hancock – <strong>FINGERPRINTS</strong> <strong>OF</strong> <strong>THE</strong> <strong>GODS</strong><br />

In his voluminous work Tiahuanacu: the Cradle of American Man, the late<br />

Professor Arthur Posnansky (a formidable German-Bolivian scholar whose<br />

investigations at the ruins lasted for almost fifty years) explains the<br />

archaeo-astronomical calculations which led to his controversial re-dating<br />

of Tiahuanaco. These, he says, were based ‘solely and exclusively on the<br />

difference in the obliquity of the ecliptic of the period in which the<br />

Kalasasaya was built and that which it is today’. 1<br />

What exactly is ‘the obliquity of the ecliptic’, and why does it make<br />

Tiahuanaco 17,000 years old?<br />

According to the dictionary definition it is ‘the angle between the plane<br />

of the earth’s orbit and that of the celestial equator, equal to<br />

approximately 23° 27’ at present’. 2<br />

To clarify this obscure astronomical notion, it helps to picture the earth<br />

as a ship, sailing on the vast ocean of the heavens. Like all such vessels<br />

(be they planets or schooners), it rolls slightly with the swell that flows<br />

beneath it. Picture yourself on board that ship as it rolls, standing on the<br />

deck, gazing out to sea. You rise up on the crest of a wave and your<br />

visible horizon increases; you fall back into a trough and it decreases.<br />

The process is regular, mathematical, like the tick-tock of a great<br />

metronome: a constant, almost imperceptible, nodding, perpetually<br />

changing the angle between yourself and the horizon.<br />

Now picture the earth again. Floating in space, as every schoolchild<br />

knows, the axis of daily rotation of our beautiful blue planet lies slightly<br />

tilted away from the vertical in its orbit around the sun. From this it<br />

follows that the terrestrial equator, and hence the ‘celestial equator’<br />

(which is merely an imaginary extension of the earth’s equator into the<br />

celestial sphere) must also lie at an angle to the orbital plane. That angle,<br />

at any one time, is the obliquity of the ecliptic. But because the earth is a<br />

ship that rolls, its obliquity changes in a cyclical manner over very long<br />

periods. During each cycle of 41,000 years the obliquity varies, with the<br />

precision and predictability of a Swiss chronograph, between 22.1° and<br />

1 Tiahuanacu, II, p. 89.<br />

2 Collins English Dictionary, London, 1982, p. 1015. In addition, Dr John Mason of the<br />

British Astronomical Association defined obliquity of the ecliptic in a telephone interview<br />

on 7 October 1993: ‘The earth spins about an axis which goes through its centre and its<br />

north and south poles. This axis is inclined to the plane of the earth's orbit around the<br />

sun. This tilt is called the obliquity of the ecliptic. The current value for the obliquity of<br />

the ecliptic is 23.44 degrees.’<br />

83

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