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Re: Sextant Scope Parallelism (was Re : SNO-T Sextant)

From: Frank Reed (no email)
Date: Thu Aug 12 2004 - 23:31:10 EDT

  • Next message: Frank Reed: "Re: Sextant Scope Parallelism (was Re: SNO-T Sextant)"

    Robert G, you wrote:
    "That’s where you got me. If the sextant is vertical you are measuring the
    correct angle. If the scope is pointing off center by a small amount then
    you see the sun a little displaced from the center of the scope. But isn’t
    the sun still in the center of the horizon mirror and therefore in the right
    place for the measurement.  If you insist on keeping the sun in the center
    of the scope I don’t think that you can get the sun to the bottom of the
    arc, it will wander off center as you get to the bottom.  Can you force it
    both to the center of the scope and the bottom of the arc at the same time
    if the scope is out of Parallelism?"

    The purpose of "swinging" the sextant is to ensure that you are holding it
    vertically. So let's set that aside. Let's suppose you have ensured that the
    sextant is exactly and precisely vertical by swinging or even by mounting the
    instrument on a pole. With that done, you can still rotate the sextant about its
    vertical axis so that the Sun and the spot on the horizon beneath will pan
    from left to right across the field of view of the telescope. If the telescope is
    not parallel to the sextant frame, the contact between horizon and Sun will
    change as you pan, typically only by a few tenths of a minute of arc. In
    practice, you would almost never notice this effect with a standard Sun sight,
    except at noon, because the Sun is moving so fast. The best way to test for this
    alignment issue is by bringing two star images together. Observed angles between
    stars do change (because of changing refraction as the stars travel across
    the sky), but the change occurs very slowly and would not be obervable for
    several minutes. So you bring two stars together in the field of view of your
    sextant. Usually you will do this somewhere near the center of the field of view.
    Now rock the sextant back and forth so that the superimposed star images shift
    from left to right. If they do not remain superimposed across the whole field
    of view, the telescope is not parallel to the frame. When shooting lunars,
    where a couple of tenths of a minute of arc can be a big deal, this alignment
    error can lead to surprising errors. Speaking from experience, getting the scope
    parallel goes a long way towards making the sights more accurate.

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


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