Jump to content

Great refractor

From Wikipedia, the free encyclopedia
(Redirected fromGreat Refractor)
Treptow telescope (akaHimmelskanone) did away with a dome, and the telescope tube extends above the building in this image
Grande LunetteofNice Observatoryof 1886, with 76 cm aperture
James Lick telescopeof 1888, with 91 cm aperture

Great refractorrefers to a large telescope with a lens, usually the largest refractor at an observatory with anequatorial mount.The preeminence and success of this style in observational astronomy defines an era in modern telescopy[1]in the 19th and early 20th century.[1]Great refractors were largerefracting telescopesusingachromatic lenses(as opposed to the mirrors ofreflecting telescopes). They were often the largest in the world, or largest in a region. Despite typical designs having smaller apertures than reflectors, great refractors offered a number of advantages and were popular for astronomy.[1]It was also popular to exhibit large refractors at international exhibits, and examples of this include the Trophy Telescope at the1851 Great Exhibition,and the Yerkes Great Refractor at the1893 World's Fair in Chicago.

A great refractor was often the centerpiece of a new 19th century observatory, but was typically used with an entourage of other astronomical instruments such as aMeridian Circle,aHeliometer,anAstrograph,and a smaller refractor such as aComet Seekeror Equatorial. Great refractors were often used for observing double stars and equipped with aFilar micrometer.Pioneering work on astrophotography was done with great refractors.[2]

An example of prime achievements of refractors, over 7 million people have been able to view through the 12-inch Zeiss refractor atGriffith Observatorysince it opened in 1935; this is the most people to have viewed through any telescope.[3]In modern times many large refractors have become important historical items, and are often used for public astronomy outreaches. However, many have also been shut down or moved due to their difficulty of use as telescopes. Whereas in the modern era aperture and location are important, the older style observatories were often located near towns because astronomy was only one function; major tasks were simply to record the weather, make accurate determinations of location, and to determine the local time. In modern times many of these functions are performed elsewhere and communicated locally.

Some noted accomplishments of refractors were the discovery of Neptune, the discovery of the Moons of Mars, and the compilation of various star catalogs. A derivative instrument of refractors, theheliometerwas used to measure for the first time the distance to another star by geometricparallaxin the mid-1800s. As telescopes became larger and longer, the relatively modest increases in aperture belied their enormous size, with moving weights in the multiple tons in domes several stories tall; physically many of the biggest were larger than even some modern reflecting telescopes.

Beginnings

[edit]
An observer looking through the Markree's Cauchoix great telescope
Fraunhofer refractor of 1824, now an exhibit at the oldTartu Observatorymuseum in Estonia.

In the early 19th century a youngEdward Joshua Cooperbuilt in Ireland one of the most richly furnished astronomical observatories of the period.[4]Cooper had acquired the largest lens in the world, made by Cauchoix ofParis,with an objective of 13.3 inches (~34.8 cm) for 1200 pounds, and he placed it as the centerpiece of the observatory.[4][5]By 1834 it was mounted on an equatorial mounting supplied byThomas Grubbof Dublin. This was the largest refractor in the world in the early 1830s, and Cooper used the telescope to sketchHalley's cometin 1835 and to view the solar eclipse of 15 May 1836.[5]

In 1833 theDuke of Northumberlanddonated a Cauchoix of Paris objective lens to establish a large telescope for the new Observatory of Northumberland.[6]The telescope was used for over a century with some updates, but the original was an "achromatic doublet of 11.6 inches clear aperture and focal length 19ft 6in".[6]

Refractors come of age

[edit]
Percival LowellobservingVenusin the daytime from the observer's chair of the 24-inch (61 cm) Alvan Clark refracting telescope in Flagstaff, Arizona.


Although there had been very large (and unwieldy)Non-achromaticaerial telescopesof the late 17th century, andChester Moore Halland others had experimented with smallachromatic telescopesin the 18th century,John Dollond(1706–1761)invented and created an achromatic object glass and lens which permitted achromatic telescopes up to 3–5 in (8–13 cm) aperture.[7][8]The SwissPierre-Louis Guinand(1748–1824) discovered and developed a way to make much larger crown and flint glass blanks.[8]He worked with instrument makerJoseph von Fraunhofer(1787–1826)to use this technology for instruments in the early 19th century.[8]

The era ofgreat refractorsstarted with the first modern, achromatic, refracting telescopes built byJoseph von Fraunhoferin the early 1820s.[9][10][11][12]The first of these was the Dorpat Great Refractor, also known as the Fraunhofer 9-inch, at what was then Dorpat Observatory in theGovernorate of Estonia(Estland) (which later becameTartu Observatoryin southernEstonia). This telescope made by Fraunhofer had a 9Paris inch(about 9.6 in (24 cm)) aperture achromatic lens and a 4 m (13.4 ft) focal length. It was also equipped with the first modernequatorial mounttype called a "German equatorial mount" developed by Fraunhofer,[13]a mount that became standard for most large refractors from then on. A Fraunhofer "9-inch" (24 cm) atBerlin Observatorywas used byJohann Gottfried Gallein thediscovery of Neptune.[14]There is tendency to round apertures to the nearest large figure, which can create a sort of drift when conversions are made; the Fraunhofer "9-inch" were nineparis incheswhich is about 9.6 in or about 24 cm, not exactly nine English inches, and closer to ten inches. (Paris inches are also calledpouces)

Refractor at an exhibition, 1851

In 1851, at theGreat Exhibitionin Hyde Park, one of the noted exhibits was telescope with 5 m (16 feet) long tube, called the "Trophy telescope" and was featured in the exhibition.[15]The telescope was placed by the astronomerJames William Grant,and it had an 11-inch aperture (280mm) and a 16 feet (4.88m) focal length.[16][17]

At the 1861 International Exhibit, the size increased to showing a telescope with 21-inch objective lens.[18]The Buckingham or Walworth Common telescope's objective was manufactured by William Wray.[18]

On January 31, 1862, American telescope-maker and astronomerAlvan Graham Clarkfirst observed the faint companion, which is now called Sirius B, or affectionately "the Pup".[19]This happened during testing of an 18.5-inch (470 mm) aperture great refractor telescope forDearborn Observatory,which was one of the largest refracting telescope lens in existence at the time, and the largest telescope in the United States.[20]

A 25-inch (63.5 cm) objective refractor was installed in the Newall telescope.[18]This had an objective made by the makers Chance, with the overall telescope made by Thomas Cooke.[21]The telescope was made for Robert Stirling Newall, and when completed in 1869 was the largest refracting telescope in the world.[21]In the 1950s the University of Cambridge donated the Newall telescope to the National Observatory of Athens, who accepted the gift and it has been there ever since.[21]In Greece, it was installed in new custom dome building near thePendelimountain.[21]

The Golden era

[edit]

Refracting telescopes would quadruple in size by the end of the century, culminating with the largest practical refractor ever built, theYerkes Observatory40-inch (1 meter) aperture of 1895.[22][23]This great refractor pushed the limits of technology of the day; the fabrication of the two element achromatic lens (the largest lens ever made at the time), required 18 attempts and cooperation betweenAlvan Clark & SonsandCharles Feilof Paris.[23]To achieve its optical aperture it was actually slightly bigger physically, at 41 3/8 in.[24]Refractors had reached their technological limit; the problems oflens saggingfromgravitymeant refractors would not exceed around 1 meter,[25]althoughAlvan G. Clark,who had made the Yerkes 40-inch objective, said a 45-inch (114 cm) would be possible before he died.[24]In addition to the lens, the rest of the telescope needed to be a practical and highly precise instrument, despite the size. For example, the Yerkes tube alone weighed 75tons,and had to track stars just as accurately as a smaller instrument.[24]

Observer end of the Lick telescope

The choice between large refractors or reflectors was driven by the technology of the time.[26]For refractors, the difficulties of fabricating two disks of optical glass for a large achromatic lens were formidable. For reflectors in much of the 19th century, the preferred material of aprimary mirrorwasspeculum metal,a substance that reflected up to 66 percent of the light that hit it and tarnished in months. They had to be removed, polished, andre-figuredto the correct shape. This sometimes proved so difficult, that a telescope mirror was abandoned.[27]In the mid-19th century a technique for coating glass with metal offered a major advantage and this technology became more common in the following decades. In the 21st century metal-coated glass mirrors remain popular, including on space telescopes like theHubble Space Telescope.

TheGreat Paris Exhibition Telescope of 1900was fixed in a horizontal position to overcome gravitational distortion on its 1.25 m (49.2 in) lens and was aimed with a 2 msiderostat.This demonstration telescope was scrapped after theExposition Universelleclosed. The Treptow refractor was built forGreat Industrial Exposition of Berlinof 1896.

In the late 19th century, the big refractors reached some of their great successes including the discovery of themoons of Marsin 1877 and the Jovian moonAmaltheain 1892. That was the first new moon of Jupiter to be found since Galileo. In addition, they were used for groundbreaking work on astrophotography and spectroscopy. The discovery of interstellar calcium in 1904, by the Potsdam great refractor, rounded out their discoveries. However, through this time they were overshadowed by large reflectors such as theLeviathan of Parsonstown,and work with theCrossley Reflectorand increasingly larger silver-and-glass mirrors marked large refractors' obsolescence.

End of the era

[edit]
The 40-inch (1.02 m) Refractor, atYerkes Observatory,the largest by famed lens makers Alvin & Clark

The era slowly came to end as large reflecting telescopes superseded the great refractors. In 1856–57,Carl August von SteinheilandLéon Foucaultintroduced a process of depositing a layer of silver on glass telescope mirrors. Silvered glass mirrors were a vast improvement over speculum metal and made reflectors a practical instrument. The era of large reflectors had begun, with telescopes such as the 36-inch (91 cm)Crossley Reflector(1895), 60-inch (1.5 m)Mount Wilson ObservatoryHale telescope of 1908, and the 100-inch (2.5 m) Mount Wilson Hooker telescope in 1917.[28][29] Two other big telescopes that surpassed the largest refractors in aperture were theDominion Astrophysical Observatoryand theDavid Dunlap Observatoryin Canada, which came online in the early 1900s.

The largest refractor in Europe, with the exhibition scope dismantled, would be the double telescope, with 33-inch (84 cm) primary,La Grande Lunetteat Meudon (later part of Paris Observatory).[30]This was manufactured by the Henry Brothers and Gautier, who had also made the big Expo telescope of 1900.[30]

Photographic vs. Visual

[edit]
TheGrande LunetteofMeudon Observatory(France), is a double refractor with both a 83 cm and 62 cm on one shaft and came online in 1891.

The advent of chemical-based astrophotography in the late 19th century brought difficulties in adapting great refractors to this application.[31]Achromatic lenses were color corrected for what the human eye was sensitive to, yellow light, while photography plates at that time were more sensitive to light at the blue end of the spectrum, requiring a lens with a different color correction and focal plane. Solutions to this problem included:[31]

  • mounting two telescopes side by side, one with a visual objective and one with a photographic objective
  • mounting a single telescope but having an interchangeable visual objective and photographic objective
  • creating objective lenses for visual use which had an additional correcting lens that could be added for photographic work
  • make special objective lenses that could be reversed, one way it was a visual objective, flipped over it was a photographic objective

An example of the first case was theMeudon Great Refractorin Paris, which was finished in 1891.[31]This had a visual objective lens of 32.7 inches on one tube, and alongside it another tube with a lens of 24.4 inches intended for photographic work.[31]An example of converting to photographic work with a third corrector lens is the Lick telescope.[31]A 33-inch corrector lens was used to convert this telescope for photography.[31]

Examples

[edit]
Dome of Greenwich 28 inch Great refractor
Vienna Observatory'sGroßer Refraktor( "Great Refractor" )[32]of 1880, with 69 cm aperture
Modern astrophotograph of the moon with a refractor (27 cm ~10.6 inch) aperture at Kuffner Observatory of Vienna, Austria.

Great refractors were admired for their quality, durability, and usefulness which correlated to features such as lens quality, mount quality, aperture, and also length. Length was important because unlike reflectors (which can be folded and shortened), thefocal lengthof glass lens correlated to the physical length of the telescope and offered some optical and image quality advantages.

Aperture

[edit]

The progression of largest refracting telescopes in the 19th century, including some telescopes at private observatories that were not really used very much or had problems.[33][34]

Selected Largest 19th Century Great Refractors by Year[35]
Observatory Aperture Year(s) Lens Maker Note
Capodimonte Observatory 17,5 cm 1814 Fraunhofer see therecord
Dorpat Observatory 24 cm 1826 Fraunhofer
Kensington Observatory 30 cm 1829–1838 Cauchoix Defunct 1836[36]or 1838[37]
Markree Observatory 34 cm 1834 Cauchoix [38]
Pulkovo observatory 38 cm 1839 Merz and Mahler[citation needed]
– 61 cm 1852–1857[39] Chance Brothers Craig telescope
Dearborn Observatory 47 cm 1862 Alvan Clark & Sons Smaller than Craig
– 53 cm 1862 BuckinghamLondon Exhibitiontelescope[40]
Newall Observatory 64 cm 1871 Chance Brothers Hardly used until 1891[41]
U.S. Naval Observatory 66 cm 1873 Alvan Clark & Sons
Vienna Observatory 69 cm 1880 Grubb
Pulkovo observatory 76 cm 1885 Alvan Clark & Sons
Nice Observatory 77 cm 1886 Gautier & Henry Grande Lunette[34]
Lick Observatory 91 cm 1888 Alvan Clark & Sons
Yerkes Observatory 102 cm 1897 Alvan Clark & Sons
– 125 cm 1900 Gautier & Mantois Paris Exhibitiontelescope; Used 1 Year Only

Some of the second-largest refractors, or otherwise notable.

Other & Double Telescope Great Refractors
Observatory Name Aperture(s) Year Lens Maker
Berlin Observatory 24 cm 1835 Merz and Mahler
Harvard College Observatory Harvard Great Refractor[42] 38 cm 1847 Merz and Mahler[citation needed]
Cambridge Observatory Northumberland Equatorial 30 cm 1835 Cauchoix[43]
Royal Greenwich Observatory 28-inch Grubb Refractor 71 cm 1893[44] Chance Brothers[45]
Astrophysical Observatory Potsdam Potsdam Große Refraktor 80 cm + 50 cm 1899
Paris Observatory Meudon 33-inch 83 cm + 62 cm 1891 Henry Brothers & Gautier[30]

Focal length

[edit]

Approximate historical progression of some of the Great refactors of the late 19th century:

Selected Longest 19th Century Great Refractors after 1873
Observatory Length Aperture Year(s) Note
U.S. Naval Observatory 9.9 m 66 cm (26 ") 1873
Vienna Observatory 10.5 m 69 cm (27 ") 1880 [46]
Nice Observatory 17.9 m 77 cm (30.3 ")[34] 1886 Biscoffscheim
Treptow Observatory 21 m 68 cm (26.77 ") 1896 No dome
Yerkes 19 m[47] 102 cm (40 ") 1897 Alvan Clark & Sons's Biggest Lens
(Exhibition scope only) 57 m 125 cm (49.2 ") 1900 Great Paris Exhibition Telescope of 1900

As long as these were, they were actually much shorter than the longestsingletrefractors inaerial telescopes.[48]

The Paris exhibition scope, besides from using a mirror to aim, was not really an observatories 'great' refractor in that sense, but its possible it might have been and both the enormous Yerkes and Treptow refractors actually debuted at exhibitions, which were major events of the period.

[edit]
Dome of the Royal Observatory Greenwich 28-inch refractor, circa 1900

Observations

[edit]
The Moon through a 10-inch aperture Grubb refractor

See also

[edit]

References

[edit]
  1. ^abc"Era: Great Refractors".Amazing-space.stsci.edu.Retrieved2014-03-01.
  2. ^"Harvard College Observatory: Great Refractor".Cfa.harvard.edu. 2012-11-21.Retrieved2014-03-01.
  3. ^"Zeiss Telescopes - Griffith Observatory - Southern California's gateway to the cosmos!".
  4. ^abDrew, J. (1851)."Report of the Council to the Thirty-first Annual General Meeting".Monthly Notices of the Royal Astronomical Society.11(4).Royal Astronomical Society:104–105.Bibcode:1851MNRAS..11..104D.doi:10.1093/mnras/11.4.67a.
  5. ^abHistory of the Cauchoix objective
  6. ^ab"Northumberland Telescope | Institute of Astronomy".www.ast.cam.ac.uk.Archived fromthe originalon 2019-07-22.Retrieved2019-10-05.
  7. ^"History – British History in depth: The Airy Transit Circle".BBC.Retrieved2014-03-01.
  8. ^abc"the lens".The Craig Telescope.Retrieved2014-03-01.
  9. ^Waaland, J. Robert (1967)."Fraunhofer and the Great Dorpat Refractor".American Journal of Physics.35(4): 344.Bibcode:1967AmJPh..35..344W.doi:10.1119/1.1974076.
  10. ^"Fraunhoferi refraktor".Obs.ee.Retrieved2014-03-01.
  11. ^A.H. Batten (1988).Resolute and Undertaking Characters: The Lives of Wilhelm and Otto Struve.Springer Science & Business Media. p. 45.ISBN978-90-277-2652-0.
  12. ^Lequeux, James (2009)."The great nineteenth century refractors".Experimental Astronomy.25(1–3): 43–61 [43].Bibcode:2009ExA....25...43L.doi:10.1007/s10686-009-9154-9.S2CID119885380.
  13. ^John Woodruff (2003).Firefly Astronomy Dictionary.Firefly Books. p.71.ISBN978-1-55297-837-5.
  14. ^Brian Daugherty."Berlin – History of Astronomy in Berlin".Bdaugherty.tripod.com. Archived fromthe originalon 2011-07-19.Retrieved2014-03-01.
  15. ^Stimson, Thomas (2018-05-04)."This week in art history: The Great Exhibition of 1851".Medium.Retrieved2019-10-24.
  16. ^http://www.mbgrg.org/newsletters/newsletter20_July13.pdf[bare URL PDF]
  17. ^Lee, Sir Sidney (1903).Dictionary of National Biography: Index and Epitome.Smith, Elder & Company.
  18. ^abcAndrews, A. D. (2000)."2000IrAJ...27..150A Page 150".Irish Astronomical Journal.27:150.Bibcode:2000IrAJ...27..150A.Retrieved2019-10-24.
  19. ^Flammarion, Camille (August 1877). "The Companion of Sirius".The Astronomical Register.15(176): 186–189.Bibcode:1877AReg...15..186F.
  20. ^Craig, John; Gravatt, William; Slater, Thomas; Rennie, George."The Craig Telescope".craig-telescope.co.uk.Retrieved3 January2011.
  21. ^abcd"Newall Refractor | The Hellenic Archives of Scientific Instruments".www.hasi.gr.Retrieved2019-10-24.
  22. ^"Telescope: Yerkes 40-inch Refractor".Amazing-space.stsci.edu.Retrieved2014-03-01.
  23. ^abMisch, Tony; Remington Stone (1998)."The Building of Lick Observatory".Lick Observatory.Univ. of California.Retrieved2008-06-30.
  24. ^abcEdgar Sanderson;John Porter Lamberton;Charles Morris(1910).Six Thousand Years of History: Achievements of the nineteenth century.T. Nolan. p. 286.
  25. ^Physics DemystifiedBy Stan Gibilisco,ISBN0-07-138201-1,page 515 Since a lens can only be held in place by its edge, the center of a large lens will sag due to gravity, distorting the image it produces. The largest practical lens size in a refracting telescope is around 1 meter,
  26. ^The Massachusetts Teacher.1848. p. 367.
  27. ^Pettit, Edison (1956). "1956ASPL 7..249P Page 253".Astronomical Society of the Pacific Leaflets.7(331). Articles.adsabs.harvard.edu: 249.Bibcode:1956ASPL....7..249P.
  28. ^Pettit, Edison (1956). "1956ASPL 7..249P Page 255".Astronomical Society of the Pacific Leaflets.7(331). Articles.adsabs.harvard.edu: 249.Bibcode:1956ASPL....7..249P.
  29. ^https://docs.google.com/viewer?a=v&q=cache:DqLUutQdc2gJ:www.astrosurf.com/re/building_large_telescopes_refractors.pdf[bare URL PDF]
  30. ^abcEnglish, Neil (2018-10-31).Chronicling the Golden Age of Astronomy: A History of Visual Observing from Harriot to Moore.Springer.ISBN9783319977072.
  31. ^abcdefKing, Henry C. (2003-01-01).The History of the Telescope.Courier Corporation.ISBN9780486432656.
  32. ^"World's Biggest Refractors".Archived fromthe originalon 2006-10-03.Retrieved2009-08-14.
  33. ^Reed Business Information (1982).New Scientist.Reed Business Information. p. 573.{{cite book}}:|author=has generic name (help)[permanent dead link]
  34. ^abc"1914Obs 37..245H Page 248".Articles.adsabs.harvard.edu.Retrieved2014-03-01.
  35. ^Reed Business Information (1982)."The Refracting Telescopes of the 19th Century".New Scientist.Reed Business Information. p. 573.{{cite magazine}}:|author=has generic name (help)[permanent dead link]
  36. ^"BARDOU: Established in Paris in 1818 by D.F. Bardou, then run by his son P.G. Bardou, and grandson, Albert D. Bardou".Europa.com.Retrieved2014-02-28.
  37. ^Dictionary of National Biography, 1885–1900, Volume 53, "South, James", by Agnes Mary Clerke (WikiSource 2010)
  38. ^Fred Watson (2006).Stargazer: The Life and Times of the Telescope.Perseus Books Group. p. 200.ISBN978-0-306-81483-9.
  39. ^"Welcome to the Online Museum of the Craig Telescope".Craig-telescope.co.uk.Retrieved2014-03-01.
  40. ^"How it was constructed".The Craig Telescope.Retrieved2014-03-01.
  41. ^"Kavli Institute for Cosmology".www.kicc.cam.ac.uk.Archived fromthe originalon March 16, 2010.
  42. ^"Harvard College Observatory: Great Refractor".www.cfa.harvard.edu.Retrieved2019-10-25.
  43. ^www.ast.cam.ac.ukhttps://web.archive.org/web/20100325215726/http://www.ast.cam.ac.uk/about_ioa/history/northumberland.php.Archived fromthe originalon March 25, 2010.{{cite web}}:Missing or empty|title=(help)
  44. ^"28-inch telescope: Scenic attractions: Visit the museum: NMM".webarchive.nationalarchives.gov.uk.Archived fromthe originalon 2008-11-14.Retrieved2019-10-25.
  45. ^"The 28-inch photo-visual refractor:: RMG".Nmm.ac.uk. 1944-07-15. Archived fromthe originalon 2011-10-24.Retrieved2014-03-01.
  46. ^The Observatory.Editors of the Observatory. 1881. p. 192.
  47. ^Barnard, E. E. (1917)."Focal length of the 40-inch telescope of the Yerkes Observatory".The Astronomical Journal.31:24.Bibcode:1917AJ.....31...24B.doi:10.1086/104239.
  48. ^Peter L. Manly (1995).Unusual Telescopes.Cambridge University Press. p. 181.ISBN978-0-521-48393-3.

Further reading

[edit]
[edit]
Retrieved from "https://en.wikipedia.org/w/index.php?title=Great_refractor&oldid=1229991360"