was in a condition to do it connected with its principal observatory
not only the geodetic or topographical work which was done at home--a
very natural thing--but also general geographical or hydrographical
work which was executed abroad, a practice which contained the germ of
all the difficulties with which we are troubled to-day. Thus, as maps
accumulated, the need of uniformity, especially in those that referred
to general geography, was felt more and more.

This explains why this question of a single meridian as a starting
point has been so often raised of late.

Among the assemblies which have occupied themselves with this
question, the one which principally calls for our attention is that
which was held at Rome last year; indeed, for many of our colleagues
the conclusions adopted by the Congress of Rome settle the whole
matter. These conclusions must, therefore, receive our special
attention.

In reading the reports of the discussions of that Congress, I was
struck with the fact that in an assembly of so many learned men and
eminent theorists it was the practical side of the question that was
chiefly considered, and which finally determined the character of the
resolutions adopted.

Thus, instead of laying down the great principle that the meridian to
be offered to the world as the starting-point for all terrestrial
longitudes should, have above all things, an essentially geographical
and impersonal character, the question was simply asked, which one of
the meridians in use among the different observatories has (if I may
be allowed to use the expression) the largest number of clients? In a