I.
Monument.Position.Alignment.Az.Hills.Decl. N.Date B.C.
Lat. N.Long. W.
Tregaseal50°805°3920Circ. to Carn KenidjackN.12°8E.4°042°332330
The Hurlers5031042720S. circ. over cent. circ.N.1115E.32441382170
Cent. circ. over N. circ.N.1418E.3244192090
N. circ. over N.E. barrowN.1844E.3244061900
Merrivale5033154230Circ. to remains of cromlechN.150E.3140361990
Direction of smaller avenueN.2425E.5039551860
Fernworthy50383035410Direction of AvenueN.130E.1153971720
N.1420E.11538511670
Stanton Drew5122023420Cent. of Gt. Circ. to QuoitN.1759E.23338381620
Fernworthy50383035410Direction of AvenueN.1545E.11538341610
Merry Maidens5034053525Circ. to stone in the roadN.1145E.01238271590
Stanton Drew5122023420S.W. circ. to centre of Gt. Circ.N.1951E.14437301420
II.
Monument.Position.Alignment.Az.Hills.Decl. N.Date B.C.
Lat. N.Long. W.
Trowlesworthy50°27304°020Direction of primary avenueN.7°0E.2°5241°242130
Direction of final avenueN.120E.2524162080
Longstone (Tregaseal)5081053820Longstone to Chûn CromlechN.90E.14340392000
Lee Moor50263035940Direction of avenueN.220E.22838171500

In some cases, for one reason or another, this arrangement was not carried out, and Capella, in spite of the objection I have stated, was used in the following circles:—

CAPELLA AS A CLOCK-STAR.

Monument.Position.Alignment.Az.Hills.Decl. N.Date B.C.
Lat. N.Long. W.
I.
Boscawen-un50°5205°370Circ. to Stone CrossN.43°15E.2°729°362250
Merry Maidens5034053525Circ. over the “Pipers”N.3826E.02029582100
II.
The Nine Maidens50282045430Direction of Nine Maidens rowN.280E.0033471480
Stripple Stones50325143735Centre to N.E. bastionN.260E.02234381320

At the Merry Maidens, however, with nearly a sea horizon, when Arcturus ceased to be circumpolar and rose in Azimuth N. 11° 45′ E., it replaced Capella, and was used as a clock-star after 1600 B.C.

In this system of night observation we have the germ of the use in later times of an instrument called the “night-dial,” specimens of which, dating from the fourteenth century, can be seen in our museums. The introduction of graduated circles permitted the employment of circumpolar stars, and the “guards” of the Little Bear or the “pointers” of the Great Bear were thus used. There was a disc with a central aperture through which the pole star could be observed; the disc could be adjusted for every night in the year; an arm was then moved round so that the direction of the pointers (or the guards) with regard to the vertical could be measured; on a second concentric circle the time of night could be read off.

Fig. 62.—A “night-dial.”


[119] Dawn of Astronomy, 1894, p. 343.