American Horological Journal, Vol. I, No. 1, July 1869: Devoted to Pratical Horology
Science
American Horological Journal, Vol. I, No. 1, July 1869: Devoted to Pratical Horology
Clocks and watches -- Periodicals
At the present time the position of the equinoctial points shows a
recession of the whole, 30° 1´ 40´´.2. At this rate of motion the
constellations called the Signs of the Zodiac are some distance from
the divisions of the ecliptic that bear their names. At the rate
of 50´´.1 the whole revolution of the equinoctial points will be
accomplished in 25,868 years; but this is again modified because the
precession must vary in different centuries for the following reasons:
the sun’s motion is direct, the precession retrograde; therefore, the
sun arrives at the equator sooner than he does at the same star of
observation. Now, the tropical year is 365d. 5h. 48´ 49´´.7; and as the
precession is exactly 50´´.1, we must suppose it takes some time for
the sun to move through that arc. By direct observation it is found
that the time required for such translation is 20´ 19´´.6. By adding
this amount to the tropical year we have the sidereal year of 365d.
6h. 9´ 9´´.6 in mean solar days. This amount of precession has been
on the increase since the days of its first recorder, Hipparchus, as
the augmentation amounts to no less than 0.´´455. By adding that to the
known precession we find that the civil year is shorter now by 4´´.21
than in his time; but, as a great division of time, the year can be
changed by this cause not more than 43.´´
The action of the moon on the accumulation of matter at the earth’s
equator is a source of disturbance that in very accurate observations
for time should be eliminated. Thus the moon, with the conjoint action
of the sun, depending on relative position, causes the pole of the
equator to describe a small ellipse in the heavens with axes of 18´´.5
for the major, and 13´´.674 for the minor; the longer axis being
directed to the pole of the ecliptic. This inequality has a period
of 19 years,--it being equal to the revolution of the nodes of the
lunar orbit. The combination of these disturbances changes, by a small
quantity, the position of the polar axis of the earth in regard to the
stars, but not in regard to its own surface. With so many disturbing
causes, we must add that of Jupiter, whose attraction is diminishing
the obliquity of the ecliptic by 0´´.457 according to M. Bessel.
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