The Leardo Map of the World, 1452 or 1453: In the Collections of the American Geographical Society — John Shaqi
The Leardo Map of the World, 1452 or 1453: In the Collections of the American Geographical SocietyWright, John Kirtland
History
The Leardo Map of the World, 1452 or 1453: In the Collections of the American Geographical Society
Wright, John Kirtland
Early maps; Leardo, Giovanni
[9]Grotefend, _op. cit._, p. 113, asserts that O was usually omitted to
avoid confusion with zero. Leardo, however, includes O. J and I are
counted as one letter. The golden number of 1453 is 10; Leardo’s A
corresponds with golden number 8.
[10]The following is a comparison of the times of the new moon on
certain dates as indicated by Leardo with the actual times as
determined for the meridian of Venice from Th. von Oppolzer, _Canon
der Finsternisse_ (constituting _Denkschr. Kaiserl. Akad. der Wiss.
in Wien, Math.-naturw. Classe_, Vol. 52, 1887).
Leardo’s Times Actual Times
1453 Dec. 1 ? hrs. 203? pts. Nov. 30 2.40 P. M.
1455 Apr. 16 21 hrs. ? Apr. 17 12.22 A. M.
1456 Apr. 6 7 hrs. 229 pts. Apr. 5 4.25 A. M.
1461 Jan. 11 21 hrs. ? Jan. 11 8.44 P. M.
1468 Feb. 23 14 hrs. 747 pts. Feb. 23 10.15 P. M.
The discrepancies are too great and too variable to enable us to
come to any very definite conclusions as to the place or manner of
origin of Leardo’s figures.
[11]The division of the hour into 1080 points (3×6×60, as Dom Bévenot
points out) is puzzling. More usually the hour was subdivided into
four points. See Grotefend, _op. cit._, p. 188.
[12]The dominical letter for 1453 was G.
[13]On the basis of certain of the figures given by Leardo for the
lengths of the days at about the times of the solstices, I have
estimated that this table was worked out for about lat. 42° 45′ N,
which is more nearly the latitude of Orvieto than that of Venice
(45° 30′). (This calculation was made with the _Smithsonian
Meteorological Tables_, 4th edit. (constituting _Smithsonian Misc.
Colls._, Vol. 69, No. 1), Washington, 1918: Table 87, “Duration of
Sunshine at Different Latitudes,” and Table 88, “Declination of the
Sun for the Year 1899.” The difference in the declination of the sun
for 1452 and 1899 is negligible.) Dom Bévenot writes: “I fancy day
lengths were reckoned roughly for degrees. Here in Weingarten about
1490 they used tables drawn up for lat. 45° N, though the place is
actually 47° 40′.”
[14]I am indebted to Dom Bévenot for the following comment:
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