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At
a lunar site
we should expect to find markers at either the foresight,
on the horizon, or near the backsight
which cater for the measurement of the perturbation
wobble, (+&- p), to a resolution
of
better than 2 arc
minutes of declination.
Without these installed a lunar
site would be inoperable.
Here on Glog Hill the two hill peaks on the northern end of the ridge are adorned with tumuli which bracket precisely the full range of cyclic perturbation at the Northern Major Lunar Standstill. The upper limb of the Moon, when rising near a standstill, will appear between these two tumuli allowing the astronomers to make an accurate estimation of the current condition of the lunar perturbation. Taking careful readings for several months prior to and after the standstill will furnish enough data to allow the current cycle of perturbation to be established and eliminated from the final calculations. which pin-point the day of the standstill. |