The National Geographic Magazine, Vol. II., No. 2, May, 1890 — John Shaqi
The National Geographic Magazine, Vol. II., No. 2, May, 1890Various
Science
The National Geographic Magazine, Vol. II., No. 2, May, 1890
Various
Geography -- Periodicals
In conclusion I desire to state that I am well aware this paper cannot
be regarded as a finality, but as a contribution to the geographical
history of North America it will not be without its value, while the
fact that I have myself spent parts of three summers in scientific
exploration of the coast visited by Bering and first charted by him,
has greatly helped me in my discussion of minor details of his work.
[Illustration: BERING'S CHART OF HIS FIRST VOYAGE. FROM D'ANVILLES
ATLAS. 1737. The first published map of his Explorations.]
INSTRUMENTS AND METHODS.
In considering the work done by the expedition it is very necessary to
bear in mind the character of the instrumental outfit, if any, which
they might have possessed, and the state of the science of navigation
at the time.
When Bering and his two cartographers left St. Petersburg in February,
1725, the astronomical instrument in use by navigators was the Davis
quadrant or "backstaff," in which the sun's altitude was measured by
sighting without a telescope or tube on the shadow cast by the sun from
one projection of the instrument upon another, the observer's back of
course, being turned to the luminary. The only alternative to this was
the still older astrolabe with which the observer had to look along the
two lines of his angle at the same time, and which also depended upon
sights or spurs attached to a frame. The reflecting quadrant of Hadley
was not invented until 1731 and telescopes were not used on the
instruments of navigation until somewhat later. There were no
chronometers or reliable watches or clocks for use in dividing
intervals of time. Even after the Hadley quadrant came into use, time
was noted by a pendulum vibrating seconds, which could not be used on
ship-board.
A futile attempt had been made by means of tables of variation of the
compass to determine the longitude by comparison with observed
variation in the field. Results by this method approached the truth
accidentally, if at all. Lunar observations were the only means of
getting an approximation to the longitude except the occultations of
Jupiter's satellites, both methods being impracticable on board ship,
with the instruments then employed.
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.
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account