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Stonehenge and Other British Stone Monuments Astronomically Considered

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Author Topic: Stonehenge and Other British Stone Monuments Astronomically Considered  (Read 1747 times)
Ericka Bowman
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Posts: 127

« Reply #60 on: January 12, 2009, 01:07:58 am »

line joining the stones is therefore about 4 feet to the S.E. of the axis of the present circles, which, it may be

p. 90

stated, passes 3 feet to the N.W. of the N.W. edge of the Friar's Heel (see Fig. 24).

There are besides these two large untrimmed sarsen stones, one standing some distance outside the vallum, one recumbent lying on the vallum; both nearly, but not quite, in the sunrise line as viewed from the centre of the sarsen circle. These are termed the "Friar's Heel" and "Slaughter Stone" respectively.

I will deal with (1) first, and begin by another quotation from Mr. Cunnington, who displayed great acumen in dealing with the smaller stones not sarsens.

“The most important consideration connected with the smaller stones, and one which in its archæological bearing has been too much overlooked, is the fact of their having been brought from a great distance. I expressed an opinion on this subject in a lecture delivered at Devizes more than eighteen years ago, and I have been increasingly impressed with it since. I believe that these stones would not have been brought from such a distance to a spot where an abundance of building Stones equally suitable ill every respect already existed, unless some special or religious value had been attached to them. This goes far to prove that Stonehenge was originally a temple, and neither a monument raised to the memory of the dead, nor an astronomical calendar or almanac.

"It has been suggested that they were Danams, or the offerings of successive votaries. Would there in such case have been such uniformity of design, or would they have been all alike of foreign materials? I would make one remark about the small impost of a trilithon of syenite, now lying prostrate within the circle. One

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writer has followed another in taking it for granted that there must have been a second, corresponding with it, on the opposite side. Of this there is neither proof nor record, not a trace of one having been seen by any person who has written on the subject. This small impost, not being of sarsen, but syenite, must have belonged to the original old circle; it may even have suggested to the builders of the present Stonehenge the idea of the large imposts, and trilithons with their tenons and mortices."

In Prof. Gowland's examination of the contents of the holes necessarily dug in his operations, it was found over and over again, indeed almost universally, that the quantity of blue stone chippings was much greater than that front the sarsen stones. While the sarsen stones had only been worked or tooled on their surface; the blue stones had been hewed and trimmed in extraordinary fashion; indeed it is stated by Prof. Judd that they had been reduced to half their original dimensions in this process, the chippings almost equalling the volume of the stones themselves.

It seems, then, that when the sarsen stones were set up, the sarsen and blue stones were treated very differently. This being so, the following quotation from Prof. Judd's "Note" is interesting (Archaeologia, p. 81):—

“I may repeat my conviction that if the prevalent beliefs and traditions concerning Stonehenge were true, and the "Bluestone" circles were transported from some distant locality, either as trophies of war or as the sacred treasures of a wandering tribe, it is quite inconceivable that they should have been hewed and

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chipped, as we now know them to have been, and reduced in some cases to half their dimensions, after having been carried with enormous difficulty over land and water, and over hills and valleys. On the other hand, in the glacial drift, which once probably thinly covered the district, the glacial deposits dying out very gradually as we proceed southwards, we have a source from which such stones might probably have been derived. It is quite a well-known peculiarity of the glacial drift to exhibit considerable assemblages of stones of a particular character at certain spots, each of these assemblages having probably been derived from the same source.

"I would therefore suggest as probable that when the early inhabitants of this island commenced the **** of Stonehenge, Salisbury Plain was sprinkled over thickly with the great white masses of the sarsen stones ('grey wethers'), and much more sparingly with darker coloured boulders (the so-called 'blue-stones'), the last relics of the glacial drift, which have been nearly denuded away. From these two kinds of materials the stones suitable for the contemplated temple were selected. It is even possible that the abundance and association of these two kinds of materials so strikingly contrasted in colour and appearance, at a particular spot, may not only have decided the site, but to some extent have suggested the architectural features of the noble structure of Stonehenge."

If we grant everything that Prof. Judd states, the question remains—why did the same men in the same place at the same time treat the sarsen and blue stones so differently?

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I shall show subsequently that there is a definite answer to the question on one assumption.

I next come to (2). The important point about these stones is that with the amplitude 26°, at Stonehenge, a line from the centre of the circle over the N.W. stone would mark the sunset place in the first week in May, and a line over the S.E. stone would similarly deal with the November sunrise. We are thus brought, in presence of the May-November year.

Another point about these stones is that they are not at the same distance from the centre of the sarsen stone circle, which itself is concentric with the temenos mound; this is why they lie at different distances from the mound. Further, a line drawn from the point of the Friar's heel over the now recumbent Slaughter Stone with the amplitude determined by Mr. Penrose and myself for the summer solstice sunrise in 1680 B.C. cuts the line joining the stones at the middle point, suggesting that the four untrimmed sarsen stones provided alignments both for the May and June years at about that date.

Nor is this all; the so-called tumuli within the vallum (Fig. 10) may have been observation mounds, for the lines passing from the northern tumulus over the N.W. stone and from the southern tumulus over the S.E. one are parallel to the avenue, and therefore represent the solstitial orientation.

So much, then, for the stones. We see that, dealing only with the untrimmed sarsens that remain, the places of the May sunset and June and November sunrises were marked from the same central point.

Statements have been made that there was the stump

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of another stone near the vallum to the S.W., in the line of the Friar's Heel and Slaughter Stone, produced backwards, at the same distance from the old centre as the N.W. and S.E. stones. This stone was not found in an exploration by Sir Edmund Antrobus, Mr.

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