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
Salisbury Spire 0° 0′ 0″
N. side of opening in N.E. trilithon of the external ring 237 27 40
Tree in middle of clump on Sidbury Hill 237 40 20
Highest point of Friar’s Heel 239 47 25
S. side of opening in N.E. trilithon 240 14 40
Middle „ „ „ 238 51 10
(2) _Absolute Azimuths._--All the azimuths were referred to that of
Salisbury Spire, the azimuth of which was determined by observations of
the Sun and Polaris.
(_a_) _Observation of Sun_, _June 23, 1901_, 3.30-3.40 P.M.
Mean of observed altitudes of Sun 41° 26′ 35″
Refraction -1′ 4″} 0 0 58
Parallax + 6 }
-----------
True altitude of Sun’s centre 41 25 37
Latitude = 51° 10′ 42″. Sun’s declination = 23° 26′ 43″. Using the
formula
sin ¹⁄₂(Δ + _c_ - _z_) sin ¹⁄₂(Δ + _z_ - _c_)
cos² ¹⁄₂ A = --------------------------------------------
sin _c_ . sin _z_
where A = azimuth from south, Δ = polar distance, _c_ = co-latitude,
and _z_ = zenith distance,
we get
Azimuth of Sun S. 75° 30′ 30″ W.
Mean circle reading on Sun 84 38 35
----------
Azimuth of Salisbury Spire S. 9 8 5 E.
(_b_) _Observations of Polaris._--June 23, 1901. Time of greatest
easterly elongation, calculated by formula cos _h_ = tan φ cot δ, is
G.M.T. 1.34 A.M.
Azimuth at greatest easterly elongation, calculated by the formula
sin A = cos δ sec φ
is 181° 57′ 0″ from south.
Observed maximum reading of circle 256° 33′ 0″
True azimuth of star 181 57 0
----------
Meridian (S.) reading of circle 74 36 0
Circle reading on Salisbury Spire 65 28 0
---------
Azimuth of Salisbury Spire S. 9 8 0 E.
The mean of the two determinations gives for the azimuth of Salisbury
Spire S. 9° 8′ 2″ E. This result agrees well with the value of the
azimuth communicated by the Ordnance Survey Office, namely, 9° 4′ 8″
from the centre of the circle, which being corrected by +4′ 12″ for the
position of station _a_, is increased to 9° 8′ 20″.
Hence, from the point of observation _a_, 9° 8′ 20″ has been adopted as
the azimuth of Salisbury Spire.
We thus get the following absolute values of the principal azimuths from
the point _a_:
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