NavList:
A Community Devoted to the Preservation and Practice of Celestial Navigation and Other Methods of Traditional Wayfinding
Re: star-to-star distances
From: Alexandre Eremenko
Date: 2004 Sep 29, 17:12 -0500
From: Alexandre Eremenko
Date: 2004 Sep 29, 17:12 -0500
Dear Fred, Thank you very much. I am analysing your data. On Wed, 29 Sep 2004, Fred Hebard wrote: > to play a piano, but it takes some proficiency. Sounds encouraging. I studied piano too in my youth:-) > as I had trouble with a telescope. What trouble with a telescome? I think I am also having troubles with my scopes, and even considering buying a Cassens-Plath telescope (which fits SNO-T as well, they say). > I would buy > a Tamaya Spica. I would like to sample some of the Russian sextants > too, but.... Why Tamaya? You think it is superior to Cassens-Plath is some respects? I would be also interested to sample a Cassens-Plath; maybe sometime we will come together... BTW, does anyone in the list own an SNO-T? Or maybe an inverting scope of SNO-T? I have some VERY technical matters about this scope to discuss... > from electrolytic corrosion, which disfigures many an aluminum sextant. An interesting (and probably unique?) feature of the SNO-T I mentioned before is its NON-ELECTRIC illumination... > I still have trouble getting stars to overlap > precisely, although some measurements were much more accurate Exactly the same problems I have. Is there an alternative way of sextant calibration? I mean without using other expensive instruments like a theodolite? Yout table (which I still have to study carefully) shows that you had problems somewhat similar to my ones. Which sextant (and scope!) was used, if you remember? The columns in the table I received were not aligned well. After the date, what is this? GMT? And what is "N(Da-Do)"? (Third column from the right). > Note the widely > varying difference between Da-Do for objects between 25 and 33 degrees > apart. Yes!! Same effect I had. I even suspected something was wrong with the refraction theory... for this case. How did you calculate the "real" distances? > Object1 Object2 degrees date N(Da-Do) Mean(Da-Do:sec) Std(Da-Do:sec) > > Betelgeuse Rigel 18 04/02/2003 00:59:18 3 17 20 > Procyon Betelgeuse 25 01/13/2003 01:25:29 1 5 > Sirius Procyon 25 02/14/2003 04:57:12 3 -2 5 > Sirius Procyon 25 02/23/2003 22:24:40 4 30 20 > Sirius Betelgeu 27 01/12/2003 03:46:39 2 -52 0 > Betelgeuse Pollux 33 02/23/2003 22:33:08 3 -45 11 > Capella Betelgeuse 39 01/20/2003 23:21:31 3 2 10 > Vega Arcturus 59 07/16/2004 02:40:23 5 -13 59 > Sirius Capella 65 02/03/2003 02:09:00 13 -63 71 > Sirius Schedar 104 02/03/2003 04:09:56 4 -47 95 >