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Re: Ulugh Beg's sextant
From: Herbert Prinz
Date: 2006 Mar 26, 05:38 -0500
From: Herbert Prinz
Date: 2006 Mar 26, 05:38 -0500
Frank Reed wrote: >The accuracy was presumably a few minutes of arc, but I have >never checked the observations myself. Anyone? > E. B. Knobel investigated the accuracy of Ulugh Beg's star catalogue in the introduction to his edition of it. After grouping the stars into northern, zodiacal and southern ones, he shows a systematic bias in longitude of 18', 14' and 4' respectively. Then he subdivides each group into 18 sub-groups, each 20 deg of longitude wide. The corresponding errors in longitude fluctuate about a quarter of a degree around those means, occasionally a little more. Therefore, some longitudes are more than half a degree off the truth. The errors in latitude are of a similar magnitude. From what I see, they may be just marginally better than those of Ptolemy/Hipparchus. The catalogue contains over 100 stars that had not been observed but whose longitude or latitude was taken over from Ptolemy's catalogue by applying a (slightly wrong) adjustment for precession, or by referencing them to an other star. These are not included in the above statistics. The established latitude of the observatory was not bad. It was too low by 1 1/2' or 2', depending on which sources you choose. The star places are tabulated in degrees and minutes. C.H.F. Peters remarked that the latitudes are all integer multiples of 3', whereas the longitudes end in 1' mod 3 (i.e. have a remainder of 1' after dividing by 3). Knobel sees this (particularly the latitudes) as a "clear indication" that the instrument was graduated in steps of 3'. It's not so clear to me. It would be a clear indication if the latitudes would have been observed directly, say, on an armilla. But assuming that the meridian instrument was used, any odd latitude can result from the required reduction, whatever the graduation may have been. So there is a riddle here and I don't know whether it has been solved. Similar for the longitudes. They must be the result of some final constant adjustment, but what for? Precession, perhaps? And, again, how did they get rounded to a multiple of 3' in the first place? Herbert Prinz