William Parsons, 3rd Earl of Rosse

William Parsons, 3rd Earl of Rosse

Infobox Scientist
name = William Parsons, 3rd Earl of Rosse
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caption = William Parsons, 3rd Earl of Rosse
birth_date = June 17, 1800
birth_place = York
death_date = October 31, 1867
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field = Astronomy
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known_for = telescope
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William Parsons, 3rd Earl of Rosse KP (June 17, 1800 – October 31, 1867) built the world's largest telescope in 1845 and it remained the world's largest for the rest of the century. Using his big telescope he saw and cataloged a large number of galaxies.

Biography

He was born in York in Yorkshire [ [http://www.thepeerage.com/p1279.htm#i12787 thePeerage.com - Person Page 1279 ] ] . 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 County Offaly in Ireland when his father died in 1841. 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 convert|72|in|m|sing=on telescope replaced a convert|36|in|mm|sing=on one 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 (91cm) telescope in which it resembled a crab. A few years later, when the 72-inch (183cm) 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).

In addition to his astronomical pursuits, Rosse served as a member of Parliament 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). 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." [Lefroy, T. 1871, Memoir of Chief Justice Lefroy, Hodges, Foster & Co., Dublin.]

Rosse married Mary Field, daughter of John Wilmer Field, on 14 April 1836. They had four children:

* Lawrence Parsons, 4th Earl of Rosse (b. 17 November 1840, d. 30 August 1908)
* Reverend Randal Parsons (b. 26 April 1848, d. 15 November 1936)
* Hon. Richard Clere Parsons (b. 21 February 1851, d. 26 January 1923), apparently made a name for himself building railways in South America.
* Sir Charles Algernon Parsons (b. 13 June 1854, d. 11 February 1931), is known for his commercial development of the steam turbine.

References

External links

* [http://www.klima-luft.de/steinicke/ngcic/persons/rosse3.htm A list of galaxies credited to Parsons for seeing first]
* [http://articles.adsabs.harvard.edu/full/seri/MNRAS/0029//0000124.000.html William Parsons' biography written in 1868 as an obituary, published in "Monthly Notices of the Royal Astronomical Society"]
* [http://www.birrcastle.com/telescopeHistory.asp Website of Birr Castle, where the telescope was located, has some historical info]
* [http://www.thepeerage.com/p1279.htm#i12787 thePeerage.com entry]


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