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Irish astronomer and telescope builder (1800–1867)
The eldest son of the second earl of Rosse, William Parsons was born at York in England. He was educated at Trinity College, Dublin, and Oxford University, where he graduated in 1822. He was a member of parliament from 1822 until 1834, when he resigned to devote himself to science.
Rosse's main aim was to build a telescope at least as large as those of William Herschel. As Herschel had left no details of how to grind large mirrors, Rosse had to rediscover all this for himself. It was not until 1839 that he had made a 3-inch (8-cm) mirror; this was followed by mirrors of 15 inches (38 cm), 24 inches (61 cm), and 36 inches (91 cm) until, in 1842, he felt confident enough to start work on his 72-inch (183-cm) masterpiece. He was only successful on the fifth casting. It weighed 8960 pounds (4064 kg), cost £12,000, and became known as the ‘Leviathan of Corkstown’. Its tube was over 50 feet (15 m) long and because of winds it had to be protected by two masonry piers 50 feet high and 23 feet (7 m) apart in which it was supported by an elaborate system of platforms, chains, and pulleys.
The giant reflector suffered, despite the cost and time, from two major defects. The climate of central Ireland is such that very few nights of viewing are possible during the year. Also, viewing (when possible), was restricted by the piers to a few degrees of the north–south meridian. Despite this Rosse made a couple of discoveries. He was the first to identify a spiral nebula and went on to discover 15 of them. He also named and studied the Crab nebula, which has been so important to contemporary astronomy. The telescope was finally dismantled in 1908. More than the individual discoveries made by Rosse, the Leviathan was important in the warnings it gave telescope builders. Good big mirrors were needed but they were by no means sufficient; in addition a good site and an adequate mounting were necessary.
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| William Parsons, 3rd Earl of Rosse | |
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William Parsons, 3rd Earl of Rosse
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| Born | June 17, 1800 York |
| Died | October 31, 1867 (aged 67) |
| Fields | Astronomy |
| Known for | telescope |
William Parsons, 3rd Earl of Rosse KP (17 June 1800 – 31 October 1867) built several telescopes including the world's largest telescope in 1845 and it remained the world's largest for the rest of the century. Using this telescope he saw and cataloged a large number of galaxies. His 72-inch (6 feet/1.8 m) Leviathan was the first to see the spiral structure of what was later known as the Whirlpool Galaxy, then called M51.[1]
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He was born in York in Yorkshire, England.[2] He was educated at Trinity College, Dublin, and Magdalen College, Oxford, graduating with first-class honors in mathematics in 1822. He inherited an earldom and a large estate in King's County (now County Offaly) in Ireland when his father died in 1841.
Rosse married Mary Field, daughter of John Wilmer Field, on 14 April 1836. They had four children:
In addition to his astronomical pursuits, Rosse served as an Member of Parliament (MP) for King's County from 1821 to 1834, an Irish representative peer after 1845, president of the Royal Society (1848–1854), and chancellor of Trinity College, Dublin (1862–1867).
In the 1840s, he built the Leviathan of Parsonstown, a 72-inch (183-cm) telescope at Birr Castle, Parsonstown, County Offaly. He had to invent many of the techniques he used in constructing this telescope, both because its size was without precedent and because earlier telescope builders had guarded their secrets or had simply failed to publish their methods. Rosse's telescope was considered a marvelous technical and architectural achievement, and images of it were circulated widely within the British commonwealth. Building of the telescope began in 1845 and in 1847 it was put into service. The 72-inch (1.8 m) telescope replaced a 36-inch (910 mm) that he had built previously.
Lord Rosse carried out pioneering astronomical studies and discovered the spiral nature of some nebulas, today known to be spiral galaxies. The first spiral galaxy he detected was M51, and his drawings of it closely resemble modern photographs (today it is known as the Whirlpool Galaxy).
Rosse named the Crab Nebula, based on an earlier drawing made with his older 36-inch (91 cm) telescope in which it resembled a crab. A few years later, when the 72-inch (183 cm) telescope was in service, he produced an improved drawing of considerably different appearance, but the original name stuck.
A main component of Rosse's nebular research was attempting to resolve the nebular hypothesis, which posited that planets and stars were formed by gravity acting on gaseous nebulae. Rosse himself did not believe that nebulas were truly gaseous, but rather that they were made of such an amount of fine stars that most telescopes could not resolve them individually (that is, he considered nebulas to be stellar in nature). Rosse and his technicians claimed to resolve the Orion nebula into its individual stars, which would have both political and cosmological implications, as at the time there was considerable debate over whether or not the universe was "evolved" (in a pre-Darwinian sense), a concept Rosse disagreed with strongly. Rosse's primary opponent in this was John Herschel, who used his own instruments to claim that the Orion nebula was a "true" nebula, and discounted Rosse's instruments as flawed (an insult Rosse returned about Herschel's own). In the end, neither man (nor telescope) could establish sufficient scientific authority in its results to solve the question by themselves (the convincing evidence for the gaseous nature of the nebula would come later from spectroscopic evidence, though it would not resolve the philosophical issues).
One of Rosse's telescope admirers was Thomas Langlois Lefroy, a fellow Irish MP, who said, "The planet Jupiter, which through an ordinary glass is no larger than a good star, is seen twice as large as the moon appears to the naked eye/.../But the genius displayed in all the contrivances for wielding this mighty monster even surpasses the design and execution of it. The telescope weighs sixteen tons, and yet Lord Rosse raised it single-handed off its resting place, and two men with ease raised it to any height."[3]
Lord Rosse's son published his father's findings, including the discovery of 226 NGC objects in Observations of Nebulae and Clusters of Stars Made With the Six-foot and Three-foot Reflectors at Birr Castle From the Year 1848 up to the Year 1878, Scientific Transactions of the Royal Dublin Society Vol. II, 1878.[4]
Lord Rosse built a variety of optical reflecting telescopes.[1] Rosse's telescopes used cast speculum metal parabolically ground and polished.
| Parliament of the United Kingdom | ||
|---|---|---|
| Preceded by Thomas Bernard John Clere Parsons |
Member of Parliament for King's County with Thomas Bernard 1821–1833 Nicholas Fitzsimon 1833–1835 1821 – 1835 |
Succeeded by John Craven Westenra Nicholas Fitzsimon |
| Political offices | ||
| Preceded by The Earl of Limerick |
Representative peer for Ireland 1845–1867 |
Succeeded by The Lord Dunboyne |
| Honorary titles | ||
| New title | Lord Lieutenant of King's County 1831–1867 |
Succeeded by Thomas Bernard |
| Peerage of Ireland | ||
| Preceded by Lawrence Parsons |
Earl of Rosse 1841–1867 |
Succeeded by Lawrence Parsons |
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