John Tyrrell Baylee, Method of Finding the Longitude (1823)
“ To find the Longitude:—Assume any meridian, R, as a first meridian, and find the time of the culmination of any fixed star, for any day of any year, with respect to the meridian R: the difference between the time so found and the time of the culmination of the same fixed star, for the same day of any year, with respect to any other meridian, S, will give the difference of longitude between the two meridians, R and S. The times of the respective culminations should, for greater accuracy, be found by observation, and not by calculation only. ”
