International Conference Held at Washington for the Purpose of Fixing a Prime Meridian and a Universal Day. October, 1884.: Protocols of the ProceedingsInternational Meridian Conference (1884 : Washington, D.C.)
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International Conference Held at Washington for the Purpose of Fixing a Prime Meridian and a Universal Day. October, 1884.: Protocols of the Proceedings
International Meridian Conference (1884 : Washington, D.C.)
Prime Meridian -- Congresses; Time -- Systems and standards -- Congresses
Professor J. C. ADAMS, Delegate of Great Britain, stated that he
merely desired to refer to one subject touched on by the Delegate of
France, Mr. JANSSEN, whose opinion he thought could hardly be
supported, and that was that the question of longitude was purely one
of geography. He desired to controvert that, and to hold that the
question of longitude was purely one of astronomical observation. The
difference of longitude between two places could not be determined by
geodetic observations, because to do this you must take hypothesis as
to the figure of the earth, and the figure of the earth is not a
simple figure. You may take as hypothesis that the figure of the earth
is spheroidal, and that the ratio of the axes is exactly defined. Now,
in the first place, we are not agreed as to the exact ratio of the
axes, nor are we agreed as to the exact figure of the earth. If an
attempt is made to measure the difference of longitude between two
points on the earth's surface, especially when they are a considerable
distance from each other, it is necessary to depend upon astronomical
observations. In attempting to deduce the difference of longitude from
geodetic measures, you must assume that the true figure and dimensions
of the earth are known, which is far from being the case. The theory
that the prime meridian is a matter purely of a geographical nature is
liable to the fatal objection that the determination of the difference
of longitude between one place and the other is really the
determination of the difference of time of the passage of a star
across the meridian of the two places concerned. That is very
definite. You observe the transit of the star at one place, and you
observe the transit of the star at the other place, and by means of
telegraphic communications you are able to determine their difference
of longitude independent of the figure of the earth. He said, in
conclusion, that he thought the honorable Delegate of France was
mistaken upon the main point which he had just referred to, if,
indeed, he had rightly understood him.
M. JANSSEN, Delegate of France, replied as follows:
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