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    Position by azimuth of stars
    From: Bill Lionheart
    Date: 2024 Jan 22, 18:20 +0000

    I was playin with apps on my phone that give a compass graticule
    overlaid on an image from a front facing camera, sometimes, Lat and
    Long, a map etc as well. Neat, I thought, this is the new "monocular
    compass" (well you can also stick on a monocular but my camera has a
    telephoto lens anyway).   But some of the apps I tried only worked
    with the phone horizontal. I presume they misread the output from the
    magnetometer.
    
    That had me thinking. Suppose you point a camera upwards and have a
    good compass to orient it. That would give you the azimuth of
    astronomical bodies near your Geographical position. So some quick
    calculations (open to refinement). Suppose you observe with six
    degrees of arc of your Zenith and get the azimuth to an accuracy of 1
    degree (maybe OK with enough averaging and stabilization).
    
    The density of "visible" stars (for some value of visible, lets say a
    clear night away from light pollution) is around 0.1 to 0.2 stars per
    square degree I think. Well it actually varies a lot but suppose this
    hypothetical device is sitting there watching the sky all the time
    with nothing better to do and sometimes gets lucky with lots of stars
    near the Zenith.  So 6 degree FOV radius is about 360 square degrees,
    so we will have between 3 and 7 starts to work with typically. So we
    have position lines as though we took bearings on the GP of  the stars
    and work as though it was a hand bearing compass fix  on objects up to
    360 Nautical miles away. A one degree error is about 6 nautical mile
    as 360 nautical miles, but that is the extreme and much of the time
    there will be stars closer to the GP.  If we average over time
    (and have good accelerometers and DR) and combine more than 3 LOP, etc
    we can perhaps do as well  as a round of sextant sights, but with a
    less accurate horizontal needed easier to automate.
    
    
    So a few comments.
    
    This is not even back of the envelope. I just thought of it driving so
    I may well have made some mistakes.  I usually do. Even if I did for
    some star density, accuracy etc it  would work in theory. Feedback
    welcome.
    
    While it would be handy to have a giro stabilized camera looking up,
    we could also pattern match the visible stars and average as the field
    of view moves around, maybe a wider field of view. Presumably the
    wealth of astrophotography algorithms would help.  If I am right it
    needs an approximate vertical but not a horizontal to minutes of arc
    as is traditional.
    
    Typically on ocean crossings one fix per 24 hours is fine. This could
    give quite a few fixes in the night, and could be automated.
    
    Presumably either this has been tried and didn't work but maybe not
    with the current technology. One can buy an automated deep sky
    astrophotography set up for a few hundred pounds now (eg ZWO Seestar),
    and computation can often be a substitute for more expensive optics.
    You can also get automated camera gimbals cheaply, beloved of the
    social media vloggers.
    
    Looking forward to hearing your thoughts and corrections.
    
    Bill Lionheart
    
    
    
    

       
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