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Re: Halley's lunars, back in 1698-1700

From: Frank Reed (no email)
Date: Thu May 06 2004 - 19:26:50 EDT

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    George H, you've referred to Halley's observations as "lunars". I don't think
    that's necessarily a good idea. They're conjunction and occultation
    observations. These were widely used by astronomers starting around Halley's time, but
    I bet he was one of the very few to observe them at sea. The Nautical Almanacs
    in the late 18th century included a table of "Other Phenomena" for every
    month that listed conjunctions of stars with the Moon. Many of these stars were
    quite faint. For example, the almanac for August, 1805 lists a conjunction with
    theta Ophiuchi on the 6th at 01:59 Greenwich time. Later in the month, on the
    17th at 15:13 there's a conjunction with the star they called eta Pleiadum
    (eta Tauri today).

    The process of reducing observations of occultations and conjunctions was
    considered much more complicated than lunars proper, and so it was never
    considered a real "navigational" method of finding longitude but definitely useful in
    the hands of a skilled astronomer. Also, the horns of the Moon can be
    decidedly variable since the mountains and craters at the poles can hide or expose
    large areas. It would be an interesting modern experiment to see how accurately
    one can deduce Greenwich time by watching faint stars line up with the horns of
    the Moon through a low-power telescope (such as might be held stable on a
    vessel at sea). Personally, I doubt that this could be done better than about
    five minutes of time. With proper astronomical instruments and detailed
    calculations, of course, it can be very accurate.

    Speaking of those craters and mountains and their variable orientation, they
    make the limb of the Moon "bumpy". It seems to me that the relative
    unpredictability of the mountains on the Moon's limb would place the ultimate limit on
    lunars. From photos I've taken, I would estimate that the mountains and valleys
    along the limb make a zone about 0.05 minutes of arc thick. So the sextant's
    ability to measure angles down to 0.1 minutes is really very close to the
    ultimate limit of lunar distances you could ever measure. Can anyone put better
    numbers on this issue?

    Frank R
    [X] Mystic, Connecticut
    [ ] Chicago, Illinois


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