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William Parsons, Lord Rosse
1800–1867
William Parsons, third earl of Rosse, is among the giants of nineteenth-century science
and one of the most remarkable Irishmen of his day. Born in York on 17th June 1800, into a
leading Irish family, he was a son of Lawrence Parsons, the second early of Rosse. He was
educated at Trinity College, where he became a student in 1818. In 1821 he went on to Magdalen
College in Oxford. That year he was also
elected to Parliament as the member for King's County (now Laois). He held the seat until 1834, but resigned in
order to pursue his scientific interests.
After he inherited his title he was a representative Irish peer at
Westminster from 1845.
He
was already deeply interested in astronomy and had made experiments with
telescopes at his father's estate at Parsonstown (now
Birr). The key element in a reflective
telescope, such as Parsons had in mind, was its mirror.
William
Herschel had already been working with reflecting telescopes, but he had never
published any information about how he cast and polished his specula. Parsons had to make his own experiments. He described his work in 1828 in the Edinburgh
Journal of Science. His speculum
metal combined copper and tin in proportions to make a brilliant alloy. Because this metal was very brittle, his first
mirrors were made up of a number of thin plates of the metal soldered on the
back of a strong light framework of a brass composed to have the same expansion
rate. He needed sixteen plates for a
three-foot mirror.
In
1839 the three-foot mirror was finished and mounted, but it presented
difficulties due to its expansion, so Parsons decided to cast a solid
three-foot mirror. He achieved this,
overcoming yet more technical difficulties, in 1840. In 1842 he began work on an even larger
six-foot mirror, which was finished in 1845.
This
was to be mounted in an instrument which came to be called the Leviathan, and
was the largest telescope of the nineteenth century. If was fifty-four feet long and the tube was
so wide that a man could walk upright through it.
The
mirror of Leviathan was seventy-two inches wide. The instrument took seventeen years to bring
to completion. Using local craftsmen -
the sons of tenants on his estate whom he trained as technicians and chemists -
he had first to build a steam engine to drive the tools needed to polish the
mirror. Five years were then spent on
the composition of the metal alloy for the mirror. At last he managed to compose an alloy of tin
and copper of exceptional brilliance.
His first mirror was three feet wide, but this was followed by a
six-foot one which weighed four tons.
This was mounted in the fifty-eight-foot wooden tube. He let a ball and socket into the solid rock,
and on this base laid out a platform of oak trunks over which were laid
twenty-seven cast iron plates. On this
machinery the telescope could swing from left to right by a chain drive. It was protected from the winds by two
walls. It looked for all the world like
part of the Gothic castle in which the earl himself lived, surrounded by drawbridges,
ladders, and the moving tower in the centre of it all.
Strange
as it appeared, this was not amateurish work.
The sheen which Parsons and his team achieved was created by polishing
off a layer 1/10,000 of a millimetre thick from the pre-polished mirror, evenly
from the centre to the edge. This
remarkable feat of precision made the mirror almost free of distortion, and was
rightly considered an optical marvel.
The
Leviathan established Birr as a leading astronomical site for decades, for this
was the largest telescope in existence until 1878. Rosse and fellow
astronomers invited to use the telescope made many extraordinary
discoveries. Parsons himself brought to
light the spiral form of nebulae, those strange cloudlike formations in the
distant reaches of the universe. The
telescope was powerful enough to reveal many previously unknown features of
these mysterious objects. A special
study was undertaken of the nebulae of Orion, and the large drawings which
resulted from the observations gave a remarkably clear idea of these objects.
Though
it was eventually stripped down, the telescope itself survives, and its
speculum is kept in London at the South Kensington Science Museum. Rosse's wife was a
noted photographic pioneer; his son, the fourth earl (1840-1929) was a noted
astronomer, while his third son, Charles Parsons (born in 1854), was the
inventor of the steam turbine engine in 1884, which revolutionized shipping and
was later applied to airplane jet engines.
Rosse was president of the Royal Society from
1849 to 1854, and chancellor of Dublin University in 1864.
Though
wealthy and indulgent of his scientific interests, Lord Rosse
was also a good landlord, especially so during the grim famine years at Parsonstown. He died
at Monkstown on the seacoast south of Dublin on 30th
October 1867.
His
great telescope continued to probe the deepest mysteries of the universe from
the small town in the Irish midlands.
The discovery of the size and nature of the universe has been one of
man's great intellectual adventures, probing as it does into the very first
seconds of life itself. Lord Rosse made his country a part of this great adventure.