soon favourably received, and
from which connection he obtained very profitable employment as a
valuer."
1837
"My connection with Cambridge Observatory was not yet finished. I had
determined that I would not leave a figure to be computed by my
successor. In October I had (at my private expense) set Mr Glaisher to
work on reducing the observations of Sun, Moon, and Planets made in
1833, 1834, 1835; and subsequently had the calculations examined by Mr
Hartnup. This employed me at times through 1837. I state here, once
for all, that every calculation or other work in reference to the
Cambridge Observatory, in this and subsequent years, was done at my
private expense. The work of the Northumberland Telescope was going on
through the year: from Nov. 24th to 29th I was at Cambridge on these
works.
"An object-glass of 6-3/4 inches aperture (a most unusual size at this
time, when it was difficult to find a 4-inch or 5-inch glass) had been
presented to the Greenwich Observatory by my friend Mr Sheepshanks,
and on Mar. 29th I received from the Admiralty authority for mounting
it equatoreally in the empty South Dome, which had been intended for a
copy of the Palermo Circle.--In the month of July the Admiralty wished
for my political assistance in a Greenwich election, but I refused to
give any.--On Jan. 3rd I gave notice to the Admiralty that I had
finished the computations of Groombridge's Catalogue, and was ready to
print. The printing was authorized and proceeded (the introduction was
finished on Nov. 22nd), but the book was not quite ready till the
beginning of 1838.--In connection with the Cavendish experiment: on
June 10th I wrote to Spring Rice (Chancellor of the Exchequer) for
_L500_, which was soon granted: and from this time there is a great
deal of correspondence (mainly with Mr Baily) upon the details of the
experiment and the theory of the calculation.--On July 24th I saw the
descent of the parachute by which Mr Cocking was killed. I attended
the coroner's inquest and gave evidence a few days later.
"The Planetary Reductions from 1750 to 1830 had been going on: the
computers (Glaisher, Hartnup, and Thomas) worked in the Octagon Room,
and considerable advance was made.--In consequence of the agitation of
the proposal by Mr Lubbock to form empirical tables of the Moon, for
which I proposed to substitute complete reduction of the observations
of the Moon from 1750, the British
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