Longitude

Definition and stakes

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.
Source: Wikisource

by the United States government Chapters (2002)

Assumed longitude is the longitude at which an observer is assumed to be located for an observation or computation. Observed longitude is determined by one or more lines of position extending in a generally north-south direction. Difference of longitude is the smaller angle at the pole or the shorter arc of a parallel between the meridians of two places, expressed in angular measure. Fictitious longitude is the arc of the fictitious equator between the prime fictitious meridian and any given fictitious meridian.
Source: Wikisource

D.C.) International Meridian Conference (1884 : Washington International Conference Held at Washington for the Purpose of Fixing a Prime Meridian and a Universal Day…

With regard to the reckoning of longitude, I submit that longitude and time are so intimately related that they may be expressed by a common notation. Longitude is simply the angle formed by two planes passing through the earth's axis, while time is the period occupied by the earth in rotating through that angle. If we adopt the system of measuring time by the revolution of the earth from a recognized zero, one of these planes—that through the zero—may be considered fixed; the other—that through the meridian of the place—being movable, the longitudinal angle is variable.
Source: Gutenberg

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