William Parsons, 3rd Earl of Rosse (17 June 1800 – 31 October 1867), was an Irish engineer and astronomer. He built several giant telescopes.
His 72-inch telescope, built in 1845 and colloquially known as the "Leviathan of Parsonstown", was the world's largest telescope, in terms of aperture size, until the early 20th century. From April 1807 until February 1841, he was styled as Baron Oxmantown.
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Life
He was born in York, England, the son of Sir Lawrence Parsons, later 2nd Earl of Rosse, and Alice Lloyd. He was educated at Trinity College Dublin and Magdalen College, Oxford, graduating with first-class honours in mathematics in 1822. He inherited an earldom and a large estate in King's County (now County Offaly) in Ireland when his father, Lawrence, 2nd Earl of Rosse, died in February 1841.
Lord Rosse married Mary Field, daughter of John Wilmer Field, on 14 April 1836. They had thirteen offspring, of which four sons survived to adulthood:
Lawrence, 4th Earl of Rosse (known as Baron Oxmantown until 1867; 17 November 1840 – 30 August 1908).
The Rev. Randal Parsons (26 April 1848 – 15 November 1936).
The Hon. Richard Clere Parsons (21 February 1851 – 26 January 1923), apparently known for developing railways in South America.
The Hon. Sir Charles Algernon Parsons (13 June 1854 – 11 February 1931), known for inventing the steam turbine.
In addition to his astronomical interests, Rosse served as a Member of Parliament (MP) for King's County from 1821 to 1834, president of the British Association in 1843–1844, an Irish representative peer after 1845, president of the Royal Society (1848–1854), and chancellor of the University of Dublin (Trinity College Dublin) (1862–1867). He was appointed Colonel of the disembodied King's County Royal Rifle Militia (a regiment formerly commanded by his father) from 19 June 1834 and was joined by his younger brother the Hon Lawrence Parsons as Lieutenant-Colonel from 24 December 1847. When the regiment was next embodied, in 1852, the position of colonel had become an honorary post.
Scientific studies
During the 1840s, he had the Leviathan of Parsonstown built, a 72-inch (6 feet/1.83 m) telescope at Birr Castle, Parsonstown, County Offaly. The 72-inch (1.8 m) telescope replaced a 36-inch (910 mm) telescope that he had built previously.
He had to invent many of the techniques he used for constructing the Leviathan, both because its size was without precedent and because earlier telescope builders had guarded their secrets or had not published their methods. Details of the metal, casting, grinding and polishing of the 3-ton 'speculum' were presented in 1844 at the Belfast Natural History Society. Rosse's telescope was considered a marvellous technical and architectural achievement, and images of it were circulated widely within the British Commonwealth. Building of the Leviathan began in 1842 and it was first used in 1845; regular use waited another two years, due to the Great Irish Famine. It was the world's largest telescope, in terms of aperture size, until the early 20th century. Using this telescope Rosse saw and catalogued a large number of nebulae (including a number that would later be recognised as galaxies).
Lord Rosse performed astronomical studies and discovered the spiral nature of some nebulae, today known to be spiral galaxies. Rosse's telescope Leviathan was the first to reveal the spiral structure of M51, a galaxy nicknamed later as the "Whirlpool Galaxy", and his drawings of it closely resemble modern photographs.
The Crab Nebula received its name based on a drawing made by Rosse in the early 1840s 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 (or one of his assistants) produced an improved drawing of a considerably different appearance, but the original name continued to be used.
A main component of Rosse's nebular research was his attempt 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, arguing 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). In 1845 Rosse and his technicians claimed to have resolved the Orion Nebula into its individual stars using the Leviathan, a claim which had considerable cosmological and even philosophical implications, as at the time there was considerable debate over whether or not the universe was "evolved" (in a pre-Darwinian sense), a concept which the nebular hypothesis supported and with which Rosse disagreed 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 (i.e. gaseous, not stellar), and discounted Rosse's instruments as flawed (a criticism Rosse returned about Herschel's own). Eventually, neither man (nor telescope) could establish sufficiently scientific results to resolve the question (the convincing evidence for the gaseous nature of the nebula would be developed later from William Huggins's spectroscopic evidence, though it would not immediately resolve the philosophical issues).
Lord Rosse's telescopes
Lord Rosse had a variety of optical reflecting telescopes built. Rosse's telescopes used cast speculum metal ground parabolically and polished.
15-inch (38 cm)
24-inch (61 cm)
36-inch (91 cm) (aka Rosse 3-foot telescope)
72-inch (180 cm) (aka Rosse 6-foot telescope or "Leviathan of Parsonstown"), started in 1842 and completed in 1845.