NavList:
A Community Devoted to the Preservation and Practice of Celestial Navigation and Other Methods of Traditional Wayfinding
From: Lars Bergman
Date: 2026 May 1, 06:28 -0700
The navigator is making an a.m. chronometer check while passing 3 miles west of the southern point of Brava Island in the Cape Verdes. The latitude of that point is N 14°50' and that close to the equator the 3 miles of departure corresponds to 3' of longitude, using integer minutes of arc. With the Sun bearing SE-by-E he (or she?) takes a series of five timed sights and calculates the mean value of times and altitudes. The date given, December 8th 1840 seems to be the civil date as he uses a declination of S 22°46' and an equation of time of 7m42s. The altitude is corrected by 10', indicating a fairly large height of eye or possibly some index error is included. He arrives at a local apparent time of 8h46m59s (civil time). Adding the equation of time the LMT becomes 8h39m17s. He then calculates his longitude using the "old" chronometer correction and compare the result with the known longitude.
A more direct approach would be to add the known longitude of W 24°46' or 1h39m4s to LMT, thus getting GMT 10h18m21s and comparing it with the uncorrected chronometer reading of 10h13m38s, giving a chronometer correction of 4m43s slow.
The difference of 50s when compared to the "old" correction from 35 days ago indicates that the used daily rate should be adjusted by 1.4s per day.
Lars






