A General History and Collection of Voyages and Travels - Volume 18: Historical Sketch of the Progress of Discovery, Navigation, and; Commerce, from the Earliest Records to the Beginning of the Nineteenth; Century, By William StevensonKerr, Robert
History
A General History and Collection of Voyages and Travels - Volume 18: Historical Sketch of the Progress of Discovery, Navigation, and; Commerce, from the Earliest Records to the Beginning of the Nineteenth; Century, By William Stevenson
Kerr, Robert
Voyages and travels
If we knew exactly the length of the stadium of the ancients, or, to speak
more accurately, what stadium is referred to in the accounts which have
been transmitted to us of the result of the operations of Eratosthenes,
(for the ancients employed different stadia,) we should be able precisely
to ascertain the circumference which this philosopher ascribed to the
earth, and also, whether a nearer approximation to the truth was made by
any subsequent or prior ancient philosopher. The circumference of the earth
was conjectured, or ascertained, by Aristotle, Cleomedes, Posidonius, and
Ptolemy respectively, to be 400, 300, 240, and 180 thousand stadia. It is
immediately apparent that these various measures have some relation to each
other, and probably express the same extent; measured in different stadia;
and this probability is greatly increased by comparing the real distances
of several places with the ancient itinerary distances.
The observation of Eratosthenes respecting the obliquity of the ecliptic
(though undoubtedly not so immediately or essentially connected with our
subject as his observation of the circumference of the earth) is too
important to be passed over entirely without notice. He found the distance
between the tropics less than 53° 6', and greater than 52° 96', which gives
a mean of 23° 51' for the obliquity of the ecliptic. The observations of
Hipparchus (who flourished at Alexandria about 140 years before Christ, and
whom we shall have occasion to mention more particularly afterwards)
coincided with those of Eratosthenes. Plutarch, however, who died A.D. 119,
informs us, that, in his time, the gnomons at Syene were no longer
shadowless on the day of the summer solstice. As the interval between
Eratosthenes and Plutarch was only about 512 years, Bishop Morsley has very
naturally expressed his doubts of the accuracy of Plutarch's assertion. He
says, that the change in the obliquity of the ecliptic in this interval was
only 2' 36". "A gnomon, therefore, at Syene, of the length of twelve
inches, if it cast no shadow on the day of the solstice in the time of
Eratosthenes, should have cast a shadow in the time of Plutarch of the
length only of 9/1000th, or not quite 1/100th part of an inch. The shadow
of a perpendicular column of the height of 100 feet would have been 9/10ths
of an inch." As, however, the ancients do not appear to have constructed
gnomons of such a size, and as gnomons of inferior size would have given a
shadow scarcely perceptible, it is probable that Plutarch is mistaken in
his assertion; or, at any rate, that the very small variation which did
take place between his time and that of Eratosthenes (if it were observed
at all) was ascertained by means of the well itself, which would point it
out much more distinctly and accurately than any gnomon the ancients can be
supposed to have used.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account