The Book of Trinity College Dublin 1591-1891Trinity College (Dublin, Ireland)
History
The Book of Trinity College Dublin 1591-1891
Trinity College (Dublin, Ireland)
Trinity College (Dublin, Ireland)
It was thus only a few years before Sir W. R. Hamilton’s death
that Dunsink Observatory possessed a really fine objective; but
it was only an objective, it was not a telescope. The engrossing
labours of Sir W. R. Hamilton’s mathematical work, his advancing
years, and his declining health, did not permit him to undertake
the arduous labour of its erection. Sir James South found in this
a sad grievance. I have heard him denounce this inaction with that
vigorous language which he was accustomed to use. He had even
offered to contribute liberally to the expenses of mounting, if the
College authorities would put it in hands. It was not, however,
until Sir W. R. Hamilton’s successor was appointed (1865) that the
work was done. South lived just long enough to know that the great
instrument was at last being erected. A view of the instrument,
named the South Equatorial, after the donor, is shown in the
adjoining illustration.
The successor of Sir William Rowan Hamilton as Andrews Professor
of Astronomy was Dr. Francis Brünnow. He was a German by birth,
who had distinguished himself by various astronomical researches,
and by an excellent work on Practical Astronomy. He had previously
occupied the Chair of Astronomy at the University of Michigan.
When Brünnow came to Dunsink, his first care was the mounting
of the great South Equatorial. A building was erected on the
lawn, surmounted by a dome, and fitted with revolving machinery
by Messrs. Grubb, who also constructed the tube and stand. A
micrometer, from the Berlin firm of Messrs. Pistor & Martin, was
added, and thus the South object-glass, forty years after it was
made, came into actual use.
Dr. Brünnow devoted himself chiefly to the investigation of the
Parallax of Stars. In this he was, indeed, following the traditions
of the Observatory as laid down by Brinkley. Brünnow published two
parts of his researches on this difficult subject. These papers are
now regarded as a classical authority in this branch of astronomy.
The pains which he took to eliminate error, and the consummate
manner in which he has discussed his results, show him to have been
both a skilful observer and an ingenious computer.
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