Leviathan of Parsonstown

Historic Irish reflecting telescope

Leviathan of Parsonstown
Victorian picture of the "Leviathan of Parsonstown"
Alternative names	Great Rosse
Named after	Leviathan
Location(s)	Birr Castle, Birr, County Offaly, Leinster, Ireland
Coordinates	53°05′48″N 7°55′03″W / 53.0967722°N 7.9175782°W / 53.0967722; -7.9175782
Observing time	60 nights per year
Built	1842–1846 (1842–1846)
First light	15 February 1845
Telescope style	astronomical observatory Newtonian telescope
Diameter	72 inches (183 cm)
Focal length	16 m (52 ft 6 in)
Mounting	altazimuth mount
Website	birrcastle.com/telescope-astronomy/
Location of Leviathan of Parsonstown
Related media on Commons
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Leviathan of Parsonstown, or Rosse six-foot telescope, is a historic reflecting telescope of 72 inches (1.83 m) aperture, which was the largest telescope in the world from 1845 until the construction of the 100-inch (2.5 m) Hooker Telescope in California in 1917. The Rosse six-foot telescope was built by William Parsons, 3rd Earl of Rosse on his estate, Birr Castle, at Parsonstown (now Birr) in Ireland.

Design and construction

Parsons improved the techniques of casting, grinding and polishing large telescope mirrors from speculum metal, and constructed steam-powered grinding machines for parabolic mirrors. His 3 foot (91 cm) mirror of 1839 was cast in smaller pieces and then fitted together before grinding and polishing; its 1840 successor was cast in a single piece. In 1842, Parsons cast his first 6 foot (1.83 m) mirror, but it took another five casts before he had two ground and polished mirrors. Speculum mirrors tarnished rapidly; with two mirrors, one could be used in the telescope while the other was being re-polished. The telescope tube and supporting structure were completed in 1845.

The mirror was 5 inches (13 cm) thick and weighed almost 3 tons. This required a mirror cell to support and to prevent the mirror deforming under its own weight. The length of the tube and mirror box is about 54 feet (16.5 m); including the mirror it weighed about 12 tons. The tube is supported at the mirror end by a "universal joint", a hinge with two axes, which allows the tube to be inclined through a large range of altitude and also to be turned through a limited range of azimuth. The azimuth range is limited to about one hour by the supporting walls that flank the tube on its eastern and western sides. The walls are 23 feet (7.0 m) apart, 40 feet (12 m) high, and 71 feet (21.6 m) long. A chain and counterweight keeps the telescope in balance, another chain with a winch controls the altitude. A rack and pinion beam underneath the tube controls the azimuth. This beam is connected to the eastern supporting wall, where it can move on a circular iron arc to allow the telescope to change altitude.

The tube is of the Newtonian design with the eyepiece on its western side. At low altitude, the observer accesses the eyepiece from a wooden gallery that spans the distance between the walls and can slide up and down guides to follow the telescope in altitude. A cage on the gallery moves sideways to reach the eyepiece at different azimuth. At high elevation, curved galleries on top of the western wall are used, which can be moved across the wall to follow the telescope in azimuth.

Operation

The purpose of the telescope was to re-visit the nebulae in the catalogues of Charles Messier and John Herschel. These catalogues list star clusters as well as nebulae, and the question was whether the latter were merely unresolved star clusters or genuinely nebulous regions of space. It resolved into stars unclear areas which might be the first galaxies to be identified as such. Parsons discovered that several nebulae had a spiral structure, suggesting "dynamical laws". The most notable spiral nebula observed by Parsons was Messier 51, which he resolved into stars.

After William Parsons (the 3rd Earl of Rosse) died in 1867, the 4th Earl (Laurence Parsons) continued to operate the six-foot telescope. From 1874 to 1878, J. L. E. Dreyer worked with the telescope and began the compilation of his New General Catalogue of Nebulae and Clusters of Stars.

Although the 4th Earl built a smaller 3 ft equatorial in 1876, the six-foot telescope remained in use until about 1890. After his death in 1908, the telescope was partly dismantled, and in 1914, one of the mirrors with its mirror box was transferred to the Science Museum in London. The walls remained. The tube, second mirror box, and universal joint survived.

Restoration

Following a TV programme, lecture, and book by Patrick Moore, there was renewed interest in the six-foot telescope in the 1970s. Gradually, the telescope became a visitor attraction. But it was not until the 1990s that plans to actually rebuild the telescope came to fruition. In 1994 the retired structural engineer and amateur astronomer Michael Tubridy was called in to research and re-design the Rosse six-foot telescope. The original plans were lost, and so it took detective work to review the remains of the telescope, incidental comments in observing logs, and contemporary photographs taken by Mary Rosse, wife of the 3rd Earl. Reconstruction work lasted from early 1996 to early 1997. It had been planned to include a working mirror, but due to budget constraints this had to be left for a separate project.

The new mirror was installed in 1999. Unlike the speculum original, and unlike modern aluminium- or silver-coated glass mirrors, this is made of aluminium, as a compromise between authenticity and utility in astronomical observation.

Modern companion radio telescope

In 2017, LOFAR radio-telescope station IE613, one of some 50 similar stations in Europe, was constructed in the grounds of the castle. This is the westernmost station in the LOFAR network. LOFAR makes observations in the 10 MHz to 240 MHz frequency range with two types of antennas: Low Band Antenna (LBA) and High Band Antenna (HBA), optimized for 10-80 MHz and 120-240 MHz respectively. The Birr Castle station consists of 96 LBA's and 96 HBA's and a total of 96 digital Receiver Units (RCU's).

The Birr Castle station on its own is the Irish Low Frequency Array (I-LOFAR) I-Lofar telescope. In 2018, I-LOFAR observed for the first time a billion-year-old red-dwarf, flare star, namely CN Leo (Wolf 359), 7.9 light years away.

Pictures

One of the two original mirrors
The reconstructed telescope
Drawing of M51, later known as the Whirlpool Galaxy by 3rd Earl of Rosse in 1845 based on observations using the Leviathan

References

Greenslade Jr., Thomas B. "The Earl of Rosse's Leviathan Telescope". Kenyon College. Archived from the original on 29 October 2013.
^ Michael Tubridy (1998). "Reconstruction of the Rosse Six Foot Telescope". Journal of the Antique Telescope Society. 14: 18–24. Bibcode:1998JATSo..14...18T.
^ William Parsons (Lord Rosse) (1850). "XXV. Observations on the Nebulæ". Philosophical Transactions of the Royal Society of London. 140: 499–514. doi:10.1098/rstl.1850.0026. S2CID 115269149.
^ Observing and Cataloguing Nebulae and Star Clusters: From Herschel to Dreyer's New General Catalogue, by Wolfgang Steinicke, year 2010, 650 pages. The book discusses Parsons' Leviathan telescope in section 6.4 (including page 115).
"Telescope Restoration Archived 27 September 2008 at the Wayback Machine". Birr Castle. Retrieved 22 November 2009.
"The Build - I-LOFAR". Archived from the original on 30 June 2018. Retrieved 27 March 2018.
"Antenna Description". ASTRON. Retrieved 12 May 2015.
"LOFAR Stations: Description and Layout". ASTRON. Retrieved 12 May 2015.
"I-LOFAR : Exploring the Radio Universe From Ireland". I-LOFAR. Retrieved 13 June 2019
Birr radio telescope catches flaring red dwarf 75 trillion kilometres away Irish Times, 2018-03-27.

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