Rosse Six Foot Telescope
   HOME

TheInfoList



OR:

Leviathan of Parsonstown, or Rosse six-foot telescope, is a historic
reflecting telescope A reflecting telescope (also called a reflector) is a telescope that uses a single or a combination of curved mirrors that reflect light and form an image. The reflecting telescope was invented in the 17th century by Isaac Newton as an alternati ...
of
aperture In optics, an aperture is a hole or an opening through which light travels. More specifically, the aperture and focal length of an optical system determine the cone angle of a bundle of rays that come to a focus in the image plane. An ...
, which was the largest telescope in the world from 1845 until the construction of the
Hooker Telescope The Mount Wilson Observatory (MWO) is an astronomical observatory in Los Angeles County, California, United States. The MWO is located on Mount Wilson, a peak in the San Gabriel Mountains near Pasadena, northeast of Los Angeles. The observat ...
in California in 1917. The Rosse six-foot telescope was built by
William Parsons, 3rd Earl of Rosse William Parsons, 3rd Earl of Rosse (17 June 1800 – 31 October 1867), was an Irish astronomer, naturalist, and engineer. He was president of the Royal Society (UK), the most important association of naturalists in the world in the nineteenth ...
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 Speculum metal is a mixture of around two-thirds copper and one-third tin, making a white brittle alloy that can be polished to make a highly reflective surface. It was used historically to make different kinds of mirrors from personal grooming ...
, and constructed steam-powered grinding machines for parabolic mirrors. His 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 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.Michael Tubridy (1998). ''Reconstruction of the Rosse Six Foot Telescope''. Birr Castle. 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 ; 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 Altitude or height (also sometimes known as depth) is a distance measurement, usually in the vertical or "up" direction, between a reference datum and a point or object. The exact definition and reference datum varies according to the context ...
and also to be turned through a limited range of
azimuth An azimuth (; from ar, اَلسُّمُوت, as-sumūt, the directions) is an angular measurement in a spherical coordinate system. More specifically, it is the horizontal angle from a cardinal direction, most commonly north. Mathematical ...
. 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 apart, high, and 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.William Parsons (Lord Rosse) (1850). "Observations on the Nebulae". ''Philosophical Transactions of the Royal Society'', 140, 499–514
PDF online
The tube is of the Newtonian design with the
eyepiece An eyepiece, or ocular lens, is a type of lens that is attached to a variety of optical devices such as telescopes and microscopes. It is named because it is usually the lens that is closest to the eye when someone looks through the device. The ...
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 Charles Messier (; 26 June 1730 – 12 April 1817) was a French astronomer. He published an astronomical catalogue consisting of 110 nebulae and star clusters, which came to be known as the ''Messier objects''. Messier's purpose ...
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 Messier may refer to: People with the surname *Charles Messier, French astronomer *Éric Messier, former NHL defenseman *George Messier, French inventor *Jean-Marie Messier, former CEO of Vivendi Universal * Marc Messier, Canadian actor from Quebec ...
, which he resolved into stars.''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).
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 Equatorial may refer to something related to: *Earth's equator **the tropics, the Earth's equatorial region **tropical climate *the Celestial equator ** equatorial orbit **equatorial coordinate system ** equatorial mount, of telescopes * 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 A science museum is a museum devoted primarily to science. Older science museums tended to concentrate on static displays of objects related to natural history, paleontology, geology, industry and industrial machinery, etc. Modern trends in ...
in London. The walls remained. The tube, second mirror box, and universal joint survived.


Reconstruction

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 Amateur astronomy is a hobby where participants enjoy observing or imaging celestial objects in the sky using the unaided eye, binoculars, or telescopes. Even though scientific research may not be their primary goal, some amateur astronomers ...
Michael Tubridy Michael "Mick" Tubridy (born 1935 at Kilrush, County Clare, Ireland) is an Irish musician, step dancer and structural engineer. Career In November 1962, he was a founder member of the traditional Irish music group, The Chieftains, with whom ...
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 Mary Parsons, Countess of Rosse (; 14 April 1813 – 1885), was an Anglo-Irish amateur astronomer, architect, furniture designer, and pioneering photographer. Often known simply as Mary Rosse, she was one of the early practitioners of making pho ...
, 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.Telescope Restoration
". Birr Castle. Retrieved 22 November 2009.


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 A flare star is a variable star that can undergo unpredictable dramatic increases in brightness for a few minutes. It is believed that the flares on flare stars are analogous to solar flares in that they are due to the magnetic energy stored in th ...
, namely CN Leo (
Wolf 359 Wolf 359 is a red dwarf star located in the constellation Leo, near the ecliptic. At a distance of approximately 7.9 light years from Earth, it has an apparent magnitude of 13.54 and can only be seen with a large telescope. Wolf 359 i ...
), 7.9 light years away.Birr radio telescope catches flaring red dwarf 75 trillion kilometres away
Irish Times, 2018-03-27.


Pictures


See also

*
List of largest optical telescopes historically Telescopes have grown in size since they first appeared around 1608. The following tables list the increase in size over the years. Different technologies can and have been used to build telescopes, which are used to magnify distant views especia ...
* Craig telescope (refracting telescope of the 1850s) * List of largest optical telescopes in the British Isles *
List of largest optical telescopes of the 19th century List of largest optical telescopes in the 19th century, are listings of what were, for the time period of the 19th century large optical telescopes. See List of largest optical telescopes in the 20th century for the 1900s. The list includes various ...
*
Lists of telescopes This is a list of lists of telescopes. * List of astronomical interferometers at visible and infrared wavelengths *List of astronomical observatories *List of highest astronomical observatories *List of large optical telescopes * List of largest ...


References


Further reading

* Patrick Moore (1981). ''The Astronomy of Birr Castle''. The Tribune Printing and Publishing Group, Birr. * Patrick Moore (1997). "The Leviathan Reborn". ''Sky & Telescope'', 94.5, p. 52. * D.H. Levy (2004). "Miracle at Birr Castle". ''Sky & Telescope'', 107.1, p. 84. * Wolfgang Steinicke.
William Parsons, 3rd Earl of Rosse
. Retrieved 22 November 2009. * WGBH NOVA/Time-Life Video
Beyond the Milky Way
. Interviews the 7th Earl of Rosse, gives the history of the Leviathan and how it worked, starting at 1:50 {{Portal bar, Ireland, Astronomy, Stars, Spaceflight, Outer space, Solar System, Education, Science Astronomical observatories in the Republic of Ireland Buildings and structures in Birr, County Offaly Optical telescopes