Stonehenge and Other British Stone Monuments Astronomically ConsideredLockyer, Norman, Sir
History
Stonehenge and Other British Stone Monuments Astronomically Considered
Lockyer, Norman, Sir
Druids and Druidism; Great Britain -- Antiquities; Stonehenge (England); Sun worship; Temples
There is also another circle of smaller upright stones, respecting which
the only point requiring notice now is that none of them would have
interrupted the line of the axis of the avenue. The circular temple was
also surrounded by the earthen bank, shown in Fig. 15, of about 300
feet in diameter, interrupted towards the north-east by receiving into
itself the banks forming the avenue before mentioned, which is about 50
feet across. Within this avenue, no doubt an old _via sacra_, and
looking north-east from the centre of the temple, at about 250 feet
distance and considerably to the right hand of the axis, stands an
isolated stone, which from a mediæval legend has been named the Friar’s
Heel.
[Illustration: FIG. 15.--General plan; the outer circle, naos and avenue
of Stonehenge.
_F.H._ = Friar’s Heel.]
The axis passes very nearly centrally through an intercolumniation (so
to call it) between two uprights of the external circle and between the
uprights of the westernmost trilithon as it originally stood. Of this
trilithon the southernmost upright with the lintel stone fell in 1620,
but the companion survived as the leaning stone which formed a
conspicuous and picturesque object for many years, but happily now
restored to its original more dignified and safer condition of
vertically. The inclination of this stone, however, took place in the
direction of the axis of the avenue, and as the distance between it and
its original companion is known both by the analogy of the two perfect
trilithons and by the measure of the mortice holes on the lintel they
formerly supported, we obtain by bisection the distance, 11 inches, from
its edge, of a point in the continuation of the central axis of the
avenue and temple.
The banks which form the avenue have suffered much degradation. It
appears from Sir Richard Colt Hoare’s account that at the beginning of
the last century they were distinguishable for a much greater distance
than at present, but they are still discernible, especially on the
northern side, for more than 1300 feet from the centre of the temple,
and particularly the line of the bottom of the ditch from which the
earth was taken to form the bank, and which runs parallel to it.
CHAPTER VII
ASTRONOMICAL OBSERVATIONS AT STONEHENGE IN 1901[11]
An investigation was undertaken by Mr. Penrose and myself in the spring
of 1901, as a sequel to analogous work in Egypt and Greece, with a view
to determine whether the orientation theory could throw any light upon
the date of the foundation of Stonehenge, concerning which authorities
vary in their estimates by some thousands of years. Ours was not the
first attempt to obtain the date of Stonehenge by means of astronomical
considerations. In Mr. Godfrey Higgins’ work[12] he refers to a method
of attack connected with precession. This furnished him with the date
4000 B.C.
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