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Recent astronomical observations at Kilmartin Glen, Argyll, Scotland

Published online by Cambridge University Press:  22 April 2026

Abstract

Information

Type
Rapid Communication
Copyright
Copyright © The Author(s), [2010]. Published by Cambridge University Press on behalf of Antiquity Publications Ltd.
Figure 0

Figure 1. The location of the Temple Wood stone circles and the Nether Largie stones in the Kilmartin Glen on the west coast of Argyll, Scotland.

Figure 1

Figure 2. Plan of the Temple Wood stone circles (after RCAHMS 1999, with permission).

Figure 2

Figure 3. The spirals on stone 10.

Figure 3

Figure 4. The Nether Largie stones S1, S2 and S3 viewed from the south. The south side of S1 is covered with cup-and ring marks, some of which are joined with grooves to other cupmarks. There are also a number of cupmarks on the southern side of S2, and on the inner western side of S3.

Figure 4

Figure 5. Summary of the solar and lunar sightlines observed between the southern Temple Wood stone circles and the Nether Largie stones. The solar-lunar sightlines are shown in red and blue.

Figure 5

Figure 6. The midwinter sun seen from the northern circle setting above the southern circle on the 17 December 2007. The double spirals on stone 10 could be marking where the sun set about 10 days before midwinter, and perhaps the concentric circles on stone 12 are depicting this event.

Figure 6

Figure 7. The midwinter sun rising in line with S4-S5, about 9:28am on the 17 December 2007, Azi. 141° 38' Alt. 2°47' Decl. -23° 21'. Some 4000 years ago, the winter solstice sun would have risen in line with the lower right sides of the two stones. This has been confirmed by a star trail photograph.

Figure 7

Figure 8. The solar and lunar alignments of the Nether Largie stones.

Figure 8

Figure 9. This time-exposed picture of the rising moon, declination -28° 14', was taken from about 12:13am GMT on the 5 of May 2007. As the video camera recording the moonrise was in line with the stones, the above picture was taken slightly to the north of their alignment, about ten minutes after the moon had risen. The dark form of S3 can be seen just to the left of S2.

Figure 9

Figure 10. Digital illustration showing the trajectory of the midsummer moon. From S2 the midsummer moon will generally rise in line with S3 when it has a declination of about -28° 30'. Over the next few nights, the moon's declination would continue to lower and it would rise slightly more to the right of S2-S3, and then set between S5-S4. As there are cupmarks on the southern side of S2, and S3 has some on its lower inner side, these could have been connected in some way with the rising and setting moon.

Figure 10

Figure 11. The setting major standstill moon with a declination of -29° 38' was observed from the northern stones S2-S3 about 8:00 pm GMT, on the 29 September 2006. Even though the moon was completely hidden by the trees before it came in line with the stones, careful examination of its setting angle suggests that it would have set between S5-S4.

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Table 1: The orientations from the southern circle

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Table 2: The orientations from the northern circle

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Table 3: The orientations from the Nether Largie stones

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Table 4: The orientations of Q.