But all the tables of declination are of no use without an instrument
with which to measure accurately the angle between the sun and the
horizon, and such an instrument was slow in coming. The first apparatus
used was called a “cross staff.” It was made of two rods, one about
thirty-six inches and the other about twenty-six inches long. The
shorter staff was arranged so that its centre slid along the other
while it remained rigidly at right angles to the longer staff. To work
out one’s latitude with this instrument the observer waited until
noon was almost upon him. He then took his cross staff and, placing
one end of the longer crossbar to his eye and holding the instrument
so that the shorter bar stood in a vertical plane, moved the shorter
bar back and forth until he could sight over the upper end at the sun
and, at the same time, beneath the lower end at the horizon. As the
sun continued to mount to its highest point he pulled the cross staff
slowly toward him, measuring a greater and a greater angle. When the
sun had reached its highest point and the angle between it and the
horizon began to lessen, his “sight” was completed, and carefully
holding the crossbar where it marked the greatest angle he laid it on
a table on which a circle was inscribed. The end that had been at his
eye he placed at the centre of the circle, and the segment marked by
the lines from the centre past the two ends of the crossbar showed the
number of degrees in the angle he had measured between the horizon and
the sun.
But any one who has attempted to sight a gun accurately while
standing on an irregularly moving platform will have some idea of
the difficulty these old sailors had in sighting accurately at the
horizon and the sun at identically the same time from the deck of a
bobbing ship. The glare of the sun, the motion of the ship, and the
inaccuracy of the instrument itself could not be expected to give more
than approximate results, especially as the several corrections on the
angle now known to be necessary (the refraction of the sun’s rays as
they enter our atmosphere is one) were either not recognized or were
inaccurately known.
[Illustration: USING AN ASTROLABE
_This instrument was meant to improve on the cross staff. One
man held it, when it was supposed to hang with the horizon line
horizontal. Another man sighted at the sun or the stars, and a third
read and recorded the angle. Needless to say the instrument was very
inaccurate._
]
Public-domain text, read in full here on John Shaqi.
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