
NavList:
A Community Devoted to the Preservation and Practice of Celestial Navigation and Other Methods of Traditional Wayfinding
Re: lunars with and without altitudes
From: George Huxtable
Date: 2006 Nov 14, 17:49 -0000
From: George Huxtable
Date: 2006 Nov 14, 17:49 -0000
A thoughtful contribution fro Henry Halboth states- " ... you both ignore the fact that one of the observations in the Lunar set is also intended for the purpose of establishing the Local Apparent Time, for ultimate comparison with the GAT deduced from the GMT established by the distance cleared...." He is right to point out that determining a longitude involves comparing LAT (Local Apparent Time) with Greenwich time, and both those quantities are needed. Most of the discussion about lunars concentrates on the lunar-distance measurement itself, because it's so difficult to get sufficient accuracy. That is mostly because of the slow motion of the Moon with respect to the stars, only about half a degree in an hour, so that a measurement of lunar distance to 1 arc-minute determines GMT to no better than 2 minutes of time, and therefore longitude to 30 arc-minutes. In contrast, determining LAT involves measuring the altitudes of bodies which move across the sky at 15 degrees in an hour, so that measuring altitude under optimum conditions to an arc-minute can determine LAT to (roughly speaking) four seconds of time, which will have an effect on the resulting longitude of only 1 arc-minute. Because getting LAT to sufficient precision is so easy, then, it's rather taken for granted when lunars and longitude are being discussed. That doesn't mean that it can be neglected. Henry continued- "An error in the Altitude or Latitude employed for that purpose will affect whatever accuracy in Longitude or Chronometer Error may be expected from the observations as a whole. The Latitude induced error, of course, being dependent on the distance off the Prime Vertical of the body employed for the purpose of establishing the LAT." All that is perfectly true, but for the reasons given above, any such contribution to the overall error will usually be small, compared with the errors in the lunar-distance part of the process. and further- "In response to my previous comments, George has taken issue with my statement to the effect that computed altitudes were dependent upon knowledge of "position/time", but seems to go right on to prove my point by citing a prior knowledge of LAT to assist in the altitude computation." I don't recall having taken issue with such a statement at all. Indeed, I agree with Henry that a measurement of LAT is necessary. He had written- "... yes, I know it's possible to calculate the altitudes - however, does not that require a position/time of reasonable accuracy - some authorities stating these calculated altitudes should be within four arc minutes of the truth,..." and I hadn't disagreed with that, but answered "no" to his follow-up question- " ...and does not such accuracy require a position/time accuracy better than is ultimately determinable by the Lunar Distance. " The iteration method, as I explained it, requires a precise value of LAT, which is a time that doesn't depend on lunar distance for its measurement, combined with a guessed initial value for longitude. That guess is improved at each iteration, and that process does indeed rely on the measured lunar distance. That was my only point of disagreement with Henry's analysis. If altitudes of the two bodies involved in a lunar are measured, rather than calculated, it can often be convenient to use one of those observations as a time-sight also, to obtain LAT. This is handy, because it's a measure of LAT or very near the same moment as the lunar. Especially handy, in the early days when a ship might not have carried any timepiece at all; not even a hack-watch. Often, however, LAT is determined from a time-sight taken at some other moment in that day from the lunar, in which case the elapsed time between the two must be accounted for, including any known error in the rate of the timepiece, and an allowance must also be made for any change in longitude over that period., derived from dead-reckoning. You can see the circumstances in which this procedure must apply. If a Moon-star lunar distance is measured in the dark of night, with no horizon visible, then altitudes of the two bodies can't be observed, and must be found by calculation. And neither can a time-sight be taken; that has to await some light on the horizon, and the difference between the times of the two observations has to be allowed for. Henry has described those possibilities well in his last posting, which ends "but that is probably a subject for later discussion." I await his words of wisdom with some interest. George. contact George Huxtable at george@huxtable.u-net.com or at +44 1865 820222 (from UK, 01865 820222) or at 1 Sandy Lane, Southmoor, Abingdon, Oxon OX13 5HX, UK. --~--~---------~--~----~------------~-------~--~----~ To post to this group, send email to NavList@fer3.com To unsubscribe, send email to NavList-unsubscribe@fer3.com -~----------~----~----~----~------~----~------~--~---