Sydney Observatory Papers No.31
SYDNEY OBSERVATORY : 1858 to 1958 Part 3
By HARLEY WOOD
WILLIAM SCOTT
Meanwhile steps were being taken to appoint an astronomer. Denison
wrote to the Secretary of State (1855, October 15) and to the
Astronomer Royal (G. B. Airy) who was asked to “secure the services of a competent
person”. On October 26 he wrote, “I have forwarded to England a large meridian
circle which appears to require some alteration and correction before
can be made useful in the Observatory”.
Airy was asked to supervise this as well as the purchase of the sets
of the meteorological instruments. The appointment was accepted by
the Reverend William Scott, M.A., to whom Airy offered it. Scott was
born at Hartland, North Devon, in 1825, graduated as Third Wrangler
in 1848 and continued to reside in Cambridge as Fellow and afterwards
Mathematical Lecturer of Sidney Sussex College. Airy, in recommending
the appointment to the Secretary of State, said : “Mr. Scott will be prepared to commence the
duties of the office (including in that term the making himself
generally familiar with the technicalities of an Observatory, the
examination of the Sydney instruments, etc.) under my general
superintendence, tomorrow, April 16, and I request that his
nomination may be dated from that day”.
Scott “spent as large a portion as
possible of the intervening time”
before sailing early in July” at the
Greenwich Observatory, where he received every assistance from the
Astronomer Royal in completing his knowledge of practical Astronomy,
and in making himself familiar with the most recent improvements in
the construction and use of astronomical instruments”. His salary was £500 per annum.
Passages were arranged for “Scott, his
wife, three children and one female servant” on the ship “Sultana” at a
cost“ in whole of £.200,
including beer, and wine and spirits for Mr. and Mrs. Scott”. He arrived in Sydney on 1856, October
31.
Five days later Denison wrote to Parker, the Colonial Secretary,
“I went with the Astronomer over the
ground yesterday, and he agreed with me that the best site for the
Observatory would be on Flagstaff Hill at Fort Phillip. Would you
write to the Secretary of Lands and Works requesting him to direct
the Colonial Architect to put himself in communication with the
Astronomer, for the purpose of forming a plan and estimate of the
Observatory, and the dwelling-house for the Astronomer, the sooner
you get to work at this the better”.
Scott, in writing of this choice, said “it was considered of great public utility
that the Time Ball attached to the Observatory should be visible over
as great a portion of the Harbour as possible; it was also thought
desirable for other reasons that the Observatory should be in or very
near to the town. Such being the case, no better site could be found
than that on which it now stands and no other foundation could be
obtained than the sandstone rock on which the whole of Sydney is
built.”.
A plan was immediately prepared by the Colonial Architect said
Scott, “as to its scientific
requirements by the Governor General and the Astronomer”. Tenders for the erection of the “Observatory and Astronomer’s Residence”
were invited by the N.S.W. Government Gazette of 1857, February 17,
and on March 18, the successful tenders, Charles Biningermann and
Ebenezer Dewar, signed the contract to do the work for £4,330.
The original plan did not include a dome but when it was found that
sufficient money was available one was included on the the western
end of the building. [pg.9]
From 1858, February, Scott dated most of his letters from Sydney
Observatory. from the beginning, they were from 11 Macquarie Street
South. On April 11th he moved into residence and by June, 1858, the
building “was sufficiently advanced to
admit of meridian observations for time” The first recorded meridian observation is
of a transit of the Sun on 1858, July 5. The time ball was at first
at mean noon (beginning on 1858, June 5) but by the time of
Scott’s in December, 1858, it was being
dropped at 1 p.m. as it has been ever no doubt to enable to observe
the transit of the Sun.
The Observatory was built in Sydney sandstone designed in the
style of the Florentine Renaissance. From west to cast were the dome
for the equatorial telescope, the transit room, the time ball tower
and the Astronomer’s residence. So that
the time ball could be seen over most of the Harbour the tower was
made 58 feet high and consequently covered much of the eastern sky as
seen from the dome. Scott said that during his absence from the
Colony (Scott was away from from 1857, May 13, to about 1857,
September 21) it was made higher than he had originally agreed.
Meanwhile Scott, having approved of the the site of the
Observatory and set in train the arrangements for building it,
started to work in other directions. He unpacked and made ready the
twelve sets of meteorological instruments which, had from England,
collected together the instruments which had formerly to Parramatta
Observatory and began to prepare them for use in their home. He also
made extensive journeys into country areas to establish
meteorological stations. Of these Brisbane and Rockhampton were soon
transferred to the newly formed state of Queensland and Gabo Island
in Victoria.
His entailed a good deal of work and much of Scott’s correspondence at this was concerned with
coaching the observers to get satisfactory results. Most of them had
no scientific training and several changes of observers had to be
made within a few years. Communications ere poor and Scott, writing
to Airy, said that “of 10 (mercurial
barometers) which were distributed only one (was) broken which was
carried over a mountainous country in a bullock dray that was
overturned four times on the road.”
The observers selected by Scott were paid a fee of £20 per
annum but the experienced finally led to a changed arrangement. On
1860, October 8, he wrote to the Colonial Secretary asking that eight
of the sets of instruments should be transferred to telegraph
stations and recommending ” that it be
made a part of the telegraph clerk’s
duty to take regular observations and transmit a monthly return to
the Observatory ”.The arrangement,
which played an important part in developing Australian
meteorological services, was made in 1861 with the Superintendent of
Telegraphs. One of its advantages was that the observer would have at
hand a convenient means of communication. At the same time Scott a
plan for the inclination of storm warnings.
At the Observatory Scott initiated correspondence with astronomers
in other parts of the world in order to establish a library, seek
suggestions about his programme of work and make enquiries
preliminary to obtaining an equatorial telescope for his dome. The
old transit instrument from Parramatta was known to be very poor and
serious meridian work was postponed until the arrival of the Jones
meridian circle which had been used at Parramatta Observatory from
1835 and had been sent to England to be repaired by Messrs. Troughton
& Sims under the direction of the Astronomer Royal. [pg.9]
About this time occurred two astronomical phenomena which aroused
public interest. These were the total solar eclipse of 1857, March
26, and the appearance of Donati’s
Comet in 1858. They underlined the necessity for providing the
Observatory with satisfactory equipment for observational work.
Soon after the Observatory was occupied Scott wrote to the
Colonial Secretary proposition “the
appointment of a Board of Visitors for the Observatory”. The Executive Council appointed, “under the title of the Observatory
Board”, a body consisting of the
Governor General, the Colonial Secretary, the Surveyor General, the
Professor of Mathematics of the University of Sydney and the
Commanders of such of Her Majesty’s
Ships of War as may be in the Harbour”
The Board so constituted received reports of the Observatory and took
interest in its affairs until 1876 when it appears to have lapsed. At
the first meeting on 1858, December 2, support was given to
Scott’s plans for obtaining an
equatorial telescope and appointing an assistant. Scott outlined the
requirements for the telescope for which a sum of £1,000 was
voted. He wrote to Airy who had offered to arrange the purchase of
the instruments which was of 7¼ inches aperture and 124 inches
focal length and was made by Merz and Son of Munich. It arrived in
Sydney about the end of April, 1861 and, appropriately, was first
used on June 8 to observe the great comet of 1861 which was
discovered by John Tebbutt of Windsor on May 13. The position of
computer was advertised and Scott recommended the appointment of H.
C. Russell who had recently taken the B.A. Degree at the University
of Sydney and was to give distinguished service to the 0bservatory
for many years.
Until the return of the meridian circle from England the work of
the Observatory was confined to observations for time with the old
Parramatta transit instrument and the collation and publication of
the meteorological returns of the twelve stations.
The meridian circle arrived in December, 1858, and regular
observations were commenced in June, 1859. “He observed stars near the zenith at Sydney
or near the celestial pole which were not in the programme of the
Cape Observatory. The work was pursued with energy and a really good
tally of transit observations, the results of which were published in
annual volumes, was recorded from 1859 to 1862. However he was not
entirely pleased with his transit instrument and decided that on the
arrival, of the new equatorial telescope it would be more useful to
devote himself to that, paving especial attention to the “re-examination of the double stars of the
Southern Hemisphere observed at the Cape of Good Hope by Sir J.
Herschel.” The work with the meridian
circle also included “observations of
Moon culminations or the determination of longitude and observations
for the determination of latitude”.
In May, 1861, he made, with Ellery of Melbourne a telegraphic
determination of the difference in longitude between Sydney and
Melbourne. In connection with his meridian work he at first wished to
establish a meridian mark some distance away on the North Shore and
selected a site on property belonging to Alexander Berry but, having
had some experience with a temporary mark, he decided to erect to the
south, about 45 feet away, a pillar with a mark which could be
allowed through a lens of long focus built into the wall.
Daily observations of the temperature of the sea water were
commenced in 1860 as were also observations of the rise and fall of
the tide with the co-operation of the Harbour Master.
Scott made some observations of positions of comets and a series
of results for the comet 1860 III and comet 1861 II (Tebbutt), is
reported in the volumes he published for those years. The latter case
is interesting in that the orbits calculated by Scott, Tebbutt and
others suggest that the Earth passed through the tail of [pg.10] the
comet about June 29. He also [pg.10] the comet about June 29. He also
made observations of a solar eclipse on 1861, January 11, the transit
of Mercury on 1861, November 11 (12) and Encke’s comet in February, 1862. Observations of
occultations of stars and measurement of some of J. Herschel’s double stars were also begun with the new
equatorial.
Scott and the Observatory Board wished to promote a “popular taste for astronomy” and Scott invited persons with suitable
qualifications to attend for instruction in the subject. He managed
to get a small class together but no persisted to the stage of
undertaking, useful amateur work for which he was willing to provide
facilities and by which indeed he had hoped to augment the output of
the Observatory.
By early 1861 Scott had become discouraged in his work. He
referred, in 1861 report, to the strain put upon him and finally, on
1862, May 9, he penned his letter of resignation. He said “four years of close application to my duties
have so far affected my sight as to convince me that 1 could not much
longer continue to perform those duties in a manner satisfactory to
myself. I have therefore thought to restrict my appointment as soon
as I should be able to do so without at my duty altogether ruining
myself by so doing”.
The work to which Scott went was with the Church, first as master
of school. From 1865 to 1878 lie was Warden of St. Paul’s College within the University of Sydney,
after which he entered into parish work in the Goulburn diocese. He
retained his interest in science and remained an active member of the
Philosophical Society of N.S.W. and the Royal Society of N.S.W., of
which he was Honorary Secretary from 1867 to 1874 and Treasurer for
several years. He died on the 29th March, 1917.
Scott recommended that John Tebbutt, whose astronomical work was
now well known, should be appointed in his place and the Colonial
Secretary would appointed but that Tebbutt indicated his
unwillingness. Scott then, in response to a request from the Colonial
Secretary, suggested that the choice should be left to Sir J.
Herschel and the Astronomer Royal. Until Scott’s successor arrived the essential work of
the Observatory was carried on by Russell who prepared for
publication the observations made in Scott’s time and designed and set up a self
recording anemometer.
Last Update : 14th November 2012
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