NavList:
A Community Devoted to the Preservation and Practice of Celestial Navigation and Other Methods of Traditional Wayfinding
From: Henry Halboth
Date: 2010 Feb 18, 18:27 0800
George.
I usually do not buy books on the subject of Navigation. My library is already overflowing and internet sources are prolific, so there appears little reason to invest in what generally turns out to be a reinvent of some old theme, or at best a different slant on the same. The recent exchange of posts on the subject of John Letcher’s “Self Contained Navigation by HO 208” and the simple fact that I for many years used the original HO 208 in sight reduction, as well as the knowledge that John is a careful researcher, piqued my interest  so for the grandiose sum of $3.75 + a modest shipping charge (original 1977 jacket cost noted as $12.50) I have acquired a copy of this pub, used but in otherwise mint condition. John’s perspective on clearing a Lunar Distance is conventional to say the least; he does present a formula, without derivation, to clear the sextant distance, which is observed in the usual manner. He claims this formula to be a simplification which, including “neglected effects, such as oblateness of the earth, augmentation of the Moon’s semidiameter, parallax of the Sun, and the elliptical figures of the Sun and Moon due to refraction might combine in some cases to cause an error as large as 0.3 minute in the clearing…”. He gives an example of a clearing whereby his methodology gives a cleared distance of 590536 against the same clearing by Chauvenet’s method of 590533. I am here acting solely as the “messenger” and have not sought to prove or disprove his claim. The real apparent novelty of his methodology is that he presents a method, using HO 208, whereby the true Lunar Distance may be calculated at hourly intervals to allow for interpolation in finding the GMT once the sextant distance is cleared. Given the fact that in 1977 tables of Lunar Distances were probably not published on a then nonexistent Internet, as they are today, this convenience was certainly attractive – in the 1940s, when I first began doing Lunars, I found it necessary to calculate the true distances by spherical trig, as there were then no known (to me) distances published. John does devote a Chapter to “Time by Lunar Lines of Position”, which I assume to be the basis for many of the comments previously posted on this List. He here advances the theory that a Chronometer error will show in a disagreement between Sun or Stellar Sights and Moon Sights, i.e., “If the Chronometer is wrong, and you work the sights as if it were right, the moon lines will lie consistently to either the eastward or westward of the other lines, depending on whether the chronometer is fast of slow on GMT.” Thereafter, by a process of trial and error, a time may be found at which the lines come into coincidence and thus the CE determined at the time of sights. As a special circumstance of the method of Lunar Altitudes, John does deal with the matter of “Same or Opposite Azimuths” of the Moon and another body, stating here that the separation of LOPs here generated for any specific time by chronometer is an indicator of CE, depending again on eastward or westward displacement of the LOP based on the Moon sight. There are a number of caveats and case differentiations applicable to this methodology generally which are far too detailed for incorporation in this post – if interested, get the book, for $3.50 you can hardly go wrong. Again, please understand that I am only the “messenger” here and fully realize that any use of altitudes is fraught with error occasioned by the vagrancies of dip, refraction, and other variable horizon conditions too numerous to mention. Of particular interest is the preference to the reproduced HO 208 Tables, which states in part “Prior to reproduction, a total of 203 errata were corrected by the publisher. The corrections were noted during machine recomputation of the tables at the Ladd Observatory …”. Unfortunately, these corrections are not identified of quantified. I now have in hand four copies of HO 208, one of which must be assumed more correct than the others. Regards, Henry
