CHAPTER XVI

THE DARTMOOR AVENUES (_continued_)

My inquiries began at Merrivale because there is a circle associated

with the avenues a little to the south of the west end of the longest;

and again nearly, or quite, south of this there is a fine menhir,

possibly used to give a north-south line. There is another menhir given

on the Ordnance map, azimuth N. 70° 30′ E., which, with hills 3° high,

points out roughly the place of sunrise from the circle in May (April

29). Although this stone has been squared and initialed, I think I am

justified in claiming it as an ancient monument. There is still another,

azimuth N. 83° E., giving a line from the circle almost parallel to the

avenue. I hope some local archæologist will examine it, for if ancient

it will tell us whether the N. avenue or the circle was built first, a

point of which it is difficult to overrate the importance, as it will

show the strict relationship between the astronomy of the avenues and

that of the circle, and we can now, I think, deal with the astronomical

use of circles after the results obtained at Stonehenge, Stenness and

the Hurlers as an accepted fact. With the above approximate values the

date comes out 1750 B.C., the declination of the Pleiades being N. 6°

35′.

I now pass on from Merrivale as an example of those avenues the

direction of which lies somewhere in the E.-W. direction. Others which I

have not seen, given by Rowe, are at Assacombe, Drizzlecombe and

Trowlesworthy; to these Mr. Worth adds Harter or Har Tor (or Black Tor).

The avenues which lie nearly N. and S. are more numerous. Rowe gives the

following:--Fernworthy, Challacombe, Trowlesworthy, Stalldon Moor,

Battendon, Hook Lake, and Tristis Rock. Of these I have visited the

first two, as well as one on Shovel Down not named by Rowe, and the next

two I have studied on the 6-inch Ordnance map.

_Fernworthy_ (lat. 50° 38′).--Here are two avenues, one with azimuth N.

15° 45′ E., hills 1° 15′. There is a sighting stone at the N. end. We

appear to be dealing with Arcturus as clock-star 1610 B.C. This is about

the date of the erection of the N. avenue at Merrivale.

The second avenue has its sighting stone built into a wall at the south

end. Looking south along the avenue, the conditions are azimuth S. 8°

42′ W., hills 3° 30′.

Both these avenues are aligned on points within, but _not_ at the centre

of, the circle.

_Challacombe_ (lat. 50° 36′).--This is a case of a triple avenue,

probably the remains of eight rows, in a depression between two hills,

Challacombe Down and Warrington. There is no circle. The azimuth is 23°

37′ N.W. or S.E., according to direction. The northern end has been

destroyed by an old stream work; there is no blocking stone to the south

on either of the remaining avenues, but one large menhir terminates one

row of stones. The others may have been removed. So it is probable that

the alignment was to the north. If so, we are dealing with the setting

of Arcturus, warning the summer solstice sunrise in 1860 B.C. To the S.

the hills are 4° 48′, to the N. 4° 50′.

To this result some importance must be attached, first, because it

brings us into presence of the cult of the solstitial year, secondly,

because it shows us that the system most in vogue in Brittany was

introduced in relation to that year. In Brittany, as I have before

shown, the complicated alignments, there are 11 parallel rows at Le

Ménac (p. 99) (there _were_ 8 parallel rows at Challacombe), were set up

to watch the May and August sunrises, and the solstitial alignments came

afterwards. The Brittany May alignments, therefore, were probably used

long before 1860 B.C., the date we have found for Challacombe, where not

the sunrise but the setting star which gave warning of it was observed.

[Illustration: FIG. 45.--The remains of the eight rows of the

Challacombe Avenue. Looking North of East. Terminal Menhir on the

extreme right.]

It is worth while to point out that at Challacombe, as elsewhere, the

priest-astronomers so located their monuments that the nearly

circumpolar stars which were so useful to them should rise over an

horizon of some angular height. In this way the direction-lines would be

available for a longer period of time, for near the north point the

change of azimuth with change in the declination of the star observed is

very rapid.

_Shovel Down_, near Batworthy (lat. 50° 39′ 20″).--A group of five rows

of stones, four double, one single, with two sets of azimuths.

One set gives az. 22° 25°, and 28°. They seem to be associated. I will

call them A, B, and C. A is directed to the circle on Godleigh Common.

Its ends are free. B is a single line of stones to the E. of the triple

circle, about which more presently. It is not marked on the Ordnance

map; its ends are also free. C has its south end blocked, I think in

later times, by a kistvaen. The astronomical direction may be,

therefore, either N.W. or S.E. We find a probable use in the N.W.

quadrant, as at Challacombe, Arcturus setting at daybreak as a warner of

the summer solstice.

The height of hills is 46′; we have then:--

Az. N. Dec. Star. Date.

N. 22° W. 36° 19′ 40″ Arcturus 1210 B.C.

N. 25° W. 35° 23′ 20″ „ 1040 „

N. 28° W. 34° 19′ 30″ „ 850 „

Adjacent to A, B, C, is another avenue, which I will call D. Unlike the

others, its northern end points 2° E. of N. Its southern end is blocked

by a remarkable triple circle, the end of the avenue close to it being

defined by two tall terminal stones. We are justified, then, in thinking

that its orientation was towards the north; the height of the horizon I

measured as 45′. It may have been an attempt to mark the N. point of

the horizon.

The triple circle to which I have referred is not an ordinary circle. I

believe it to be a later added, much embellished, cairn. According to

Ormerod, the diameters are 26, 20, and 3 feet, and there are three small

stones at the centre.

All the above avenues are on the slope of the hill to the north. On the

south slope we find the longest of all, as shown on the Ordnance map

survey of 1885. There is a “long stone” in its centre, and at the

southern end was formerly a cromlech, the “three boys.” Part of this

avenue, and two of the three “boys,” have been taken to build a wall.

The long stone remains, because it is a boundary stone!

The azimuth is 2° 30′ W. of north or E. of south. Looking N. from the

long stone, the height of the horizon is 2° 30′. I think this avenue was

an attempt to mark the S. point.

_Trowlesworthy_ (lat. 50° 27′ 30″).--The remains here are most

interesting. This is the only monument on Dartmoor in which I have so

far traced any attempt to locate the sun’s place at rising either for

the May or solstitial year. But I will deal with the N.-S. avenue first,

as it is this feature which associates it with Fernworthy and

Challacombe.

As at Merrivale, the avenue has a decided “kink” or change of direction.

The facts as gathered from the 6-inch map are as follows:--

Az. Hills. Dec. N. Star. Date.

S. part of Avenue N. 7° E. 2° 52′ 41° 29′ 10″ Arcturus 2130 B.C.

N. „ „ N. 12° E. 2° 52′ 41° 6′ 20″ „ 2080 B.C.

[Illustration: FIG. 46.--The sight-lines at Trowlesworthy, showing high

northern azimuths. From the Ordnance map.]

This date is very nearly that of the use of the S. circle at the

Hurlers, and it is early for Dartmoor; but it is quite possible that

local observations on an associated avenue a little to the west of the

circle which terminates the N.-S. avenue will justify it. This is not

far from parallel to that at Merrivale, but its northern azimuth is

greater, so that if it turns out to have been aligned on the Pleiades

its date will be some time before that of Merrivale, that is, before

1580 B.C. I can say nothing more about it till I have visited it.

The new features to which I have referred are two tumuli which in all

probability represent more recent additions to the original scheme of

observation, as we have found at Stenness, and show that Trowlesworthy

was for long one of the chief centres of worship on Dartmoor. Their

azimuths are S. 64° E. and S. 49° W., dealing, therefore, with the May

year sunrises in November and February and the solstitial sunset in

December. It is probable that, as at the Hurlers, tumuli were used

instead of stones not earlier than 1900 B.C.

_Stalldon Moor_ (lat. 50° 27′ 45″) I have already incidentally referred

to. The azimuth of the stone row as it leaves the circle, _not_ from its

centre as I read the 6-inch map, is N. 3° E.; as the azimuth gradually

increases for a time, we may be dealing with Arcturus, but local

observation is necessary.

The differences between the Cornish and Dartmoor monuments give much

food for thought, and it is to be hoped that they will be carefully

studied by future students of orientation, as so many questions are

suggested. I will refer to some of them.

(1) Are the avenues, chiefly consisting of two rows of stones, a

reflection of the sphinx avenues of Egypt? and, if so, how can the

intensification of them on Dartmoor be explained?

(2) Was there a double worship going on in the avenues and the circles

at the same time? If not, why were the former not aligned on the

circles? On a dead level, of course, if the avenues were aligned on the

centre of the circle towards the rising or setting of the sun or a star,

the procession in the _via sacra_ would block the view of those in the

circle. We have the avenue at Stonehenge undoubtedly aligned on the

centre of the circle, but there the naos was on an eminence, so that the

procession in the avenue was always below the level of the horizon, and

so did not block the view.

(3) Do all the cairns and cists in the avenues represent later

additions, so late, indeed, that they may have been added after the

avenues had ceased to be used for ceremonial purposes? The cairn at

nearly the central point of the S. avenue at Merrivale was certainly not

there as a part of the structure when the avenue was first used as a

_via sacra_ for observing the rising of the Pleiades. I have always held

that these ancient temples, and even their attendant long and chambered

barrows, were for the living and not for the dead, and this view has

been strengthened by what I have observed on Dartmoor.

There was good reason for burials after the sacred nature of the spot

had been established, and they may have taken place at any time since;

the most probable time being after 1000 B.C. up to a date as recent as

archæologists may consider probable.

Mr. Worth, whose long labours on the Dartmoor avenues give such

importance to his opinions, objects to the astronomical use of those

avenues because there are so many of them; he informs me that he knows

of 50; I think this objection may be considered less valid if the

avenues show that they were dedicated to different uses, some practical

and others sacred, at different times of the year. For instance,

Challacombe is not a duplicate of Merrivale; one is solstitial, the

other deals with the May year; and a complete examination of them--I

have only worked on the fringe--may show other differences having the

same bearing.

In favour of the astronomical view it must be borne in mind that the

results obtained in Devon and Cornwall are remarkably similar, and the

dates are roughly the same. Among the whole host of heaven from which

objectors urge it is free for me to select any star I choose, at present

only six stars have been considered, two of which were certainly used,

as in Egypt, as clock-stars as they just dipped below the northern

horizon, and other two afterwards at Athens; and these six stars are

shown by nothing more recondite than an inspection of a precessional

globe to have been precisely the stars, the “morning stars,” wanted by

the priest-astronomers who wished to be prepared for the instant of

sunrise at the critical points of the May or solstitial year.

Stonehenge and Other British Stone Monuments Astronomically Considered · 第 4 / 18 章