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See also:GREAT See also:BRITAIN AND See also:IRELAND A . Public Observatories . ' See also:Greenwich, royal obs., See also:lat . +51 ° 28' 38.4" . Founded in 1675 for the promotion of See also:astronomy and See also:navigation . The obs. have therefore from the first been principally intended to determine the positions of See also:standard stars, the See also:sun and See also:planets, and above all to follow the See also:motion of the See also:moon with as little interruption as possible, both on and outside the See also:meridian . Since 1873 spectroscopic obs. and a daily phot. See also:record of sun-spots have been taken . The eighth See also:satellite of See also:Jupiter was discovered photographically in 1908 . The obs. is under the direction of the astronomer-royal; and from the See also:time of its first astronomer, See also:Flamsteed, the institution has always maintained its See also:place in the foremost See also:rank of obs . Thus the obs. of See also:Bradley (ob . 1762) See also:form the See also:foundation of See also:modern stellar astronomy ; but it was especially during the directorship of See also:Airy (1835–1881) that the obs. See also:rose to its See also:present high See also:state of efficiency . There are now two See also:chief assistants, six assistants, and a See also:staff of computers employed . The See also:principal See also:instruments now in use are: a meridian circle by See also:Simms (and Ransomes and May as See also:engineers), erected in 1850, having a circle of 6-ft. See also:diameter and a See also:telescope of 8-in. ap., Lassell's 2-ft. refl., erected 1884; 13-in. phot. ref r. with 10-in. vis. o.g. by Grubb; 28-in. refr. by Grubb; 26-in. phot. refr. by Grubb, with the old 12.8-in. refr. as guiding telescope; 9-in. phot. refr. by Grubb, and 3o-in. s.g. refl. by See also:Common, the last four being on one stand; 8-in. altazimuth by Simms, erected 1896 . The 26-in. and the 9-in. were presented by See also:Sir H . See also:Thompson . The standard " motor See also:clock " is the centre of a See also:system of electrically-controlled clocks scattered over the See also:United See also:Kingdom . The magnetic and meteorological See also:department was founded in 1838; it contains a See also:complete set of instruments giving continuous phot. records . The Observations are published with all details from 1750, beginning with 1836 in See also:annual bulky See also:quarto volumes; See also:special results—e.g., See also:Star Catalogues, Reductions of Lunar and Planetary Observations—are published in See also:separate volumes . See also:South See also:Kensington, See also:Solar physics obs., lat . +51° 29' 48.0", See also:long. o h. o m . 41.5 s . W . Founded 1879, under Sir N . See also:Lockyer; 3-ft. refl. and 3o-in. refl. by Common; 10-in. refr. by See also:Cooke, and several siderQstats with attachments for spectroscopic and phot. See also:work .
See also:Oxford, See also:Radcliffe obs., lat
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+51 ° 45' 35.4 long. o h
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5 m
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2.6 s
.
W
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Founded in 1771 by the Radcliffe trustees
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Obs. were regularly made, but none were published until 1839, when systematic obs. were begun with an 8-ft. transit See also:instrument by See also:Bird (1773) and a 6-ft. mural circle by See also: 5 m . 0.4 S . W . Finished in 1875; is under the Savilian See also:professor of astronomy; 12i-in. ref r. by Grubb, and a refl. made and presented by Ike La See also:Rue . The former has been used for photometric obs.; the latter for taking lunar photographs, by means of which the See also:late Professor See also:Pritchard investigated the See also:libration of the moon; 13-in. phot. ref r . by Grubb attached to the 12i-in., used for phot. work . See also:Cambridge, lat . +52° 12' 51.6", long. o h. o m . 22.8 s . E . Founded by the univ. See also:senate in 1820 . Chiefly devoted to meridian work—up to 187o with a 5-in. transit by See also:Dollond and a mural circle by Jones; a new meridian circle by Simms, of 8-in. ap. and 3-ft. circles, was then erected . The " See also:Northumberland See also:equatorial " was mounted in the " See also:English " See also:fashion in 1838; the o.g. by Cauchoix is of 111-in. ap . R . S . Newall's 25-in. refr. by Cooke, erected 1891, used for spectrographic work; siderostatic refr. with 12-in. o.g. by Cooke, 1898 . In 1908 the instruments of Sir W . See also:Huggins' obs. were presented by the Royal Society . See also:Durham, univ. obs., lat . +54° 46' 6.2" long. o h . 6 m . 19.8 s . W . Founded in 1841; small meridian circle by Simms, refr. by See also:Fraunhofer of 61-in. ap., Almucantar of 6-in. ap. by Cooke (1900) . See also:Liverpool (Bidston, See also:Birkenhead), lat . +53° 24' 4.8", long. o h . 12 m . 17.3 s . W . Founded in 1838 by the municipal See also:council; transferred in 1856 to the Docks and See also:Harbour See also:Board; moved to Birkenhead in 1867 . Specially intended for testing the rates of chronometers under different temperatures . Transit instrument by Troughton and Simms, and an 8-in. refr. by Merz . See also:Kew (See also:Richmond), lat . +51° 28' 6", long. o h . I m . 15.1 s .
W
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The central meteorological obs. of the United Kingdom, with self-registering meteorological and magnetical instruments
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Established' in 1842 under the auspices of the See also:British Association, afterwards transferred to the Royal Society
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Since 1900 a department of the See also:National Laboratory
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A photoheliograph was employed at De La Rue's expense to take daily sun-pictures from 1863 to 1872
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See also:Edinburgh, royal obs., Blackford See also: Since 1834 the obs. has been under the direction of the astronc mer-rcyal for See also:Scotland, who is also professor of See also:practical astronomy in the univ . Professor T . See also:Henderson (1833–1845) began extensive meridian obs. of fixed stars with a mural circle of 6-ft. diameter and an 8-ft. transit . A 2-ft. s.g. refl. by Grubb was erected in 1872 . New obs. erected on Blackford Hill 1893–1895 for the instruments presented by See also:Lord See also:Crawford; 15-in. refr. by Grubb, transit circle by Simms of 8-in. ap., 12-in. s.g. refl. by See also:Browning, two 6-in. refrs. and a very See also:fine library; also the 2-ft. refl . The old obs. on Calton Hill now belongs to the See also:city and is used for instruction; a 21-in. refr. by Wragge has been erected . See also:Glasgow, univ. obs., lat . +55° 52' 42.8", long. c h . 17 M . Io•6 s . W . Organized in 184o by subscription, aided by subsidies from the univ. and the state .
Meridian circle by Ertel of 6-in. ap.; 9-in. refr. by Ccoke, 20-in. s.g. refl. by Grubb with spectrograph
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Two catalogues of stars were published by the late director, R
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See also:
South), which has been used for researches on stellar See also:parallax
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A meridian circle by Pistor and Martins of 6.4-in. ap. was mounted in 1873, and a 15-in. s.g. refl. for phot. work in 1889
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Astronomical Observations and Researches made at Dunsink in 4to parts
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See also:Armagh, lat
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+54° 21 12.7", long. o h
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26 m
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35.4 s
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W
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Founded and endowed by See also:Archbishop R
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See also:Robinson in 1790
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Possessed very few instruments until the obs. was enlarged by Archbishop Lord See also:
Principal Private Observatories in z9o8
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Mr W
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Coleman's obs., See also:Buckland, See also:Dover, lat
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+51° 8' 12", long. o h
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5 m
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11 s
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E
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Cooke 8-in. refr. used for obs. of See also:double stars
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Mr J
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See also:Franklin-See also: 30-2 s . W . Erected 1903; twin equatorial by Cooke with 12-in. and 6-in. lenses, another with 8-in. and 6-in. lenses, used for phot. survey of the heavens with special reference to the Milky Way . The former instrument was used at the Cape in 1903–1904 . Rev . T . E . Espin's obs., See also:Tow See also:Law, See also:Darlington, lat . +54° 43' 30", long. o h . 7 m . 14 S . W . 17i-in. refl. by Calver, used since 1888 for See also:spectroscopy and obs. of double stars . Mr W . H . Maw's ohs., Kensington, lat . +51° 30' 2.8", long. o h. o m . 49.4 s . W., 6-in. refr. by Cooke (1886) . Also at Outwood, Surrey, lat . +51° II' 38", long. o h. o m . 23.7 s . W., 8-in. refr. by Cooke (1896), both used on double stars . Sir See also:Wilfrid Peek's obs., Rousdon, Lyme Regis, lat .
+5o° 42' 38", long. o h
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11 m
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59.0 s
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W
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Erected by the late Sir See also:Cuthbert Peek in 1885; 6.4-in. refr. by Merz used for obs. variable stars
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See also:Earl of See also:Rosse's obs., See also:Birr See also:Castle, See also: These instruments, particularly the latter, were used from 1848 to 1878 for ohs. of nebulae, and revealed many new features in these bodies; results published in the Phil . Trans. and collected systematically in the Trans . See also:Roy . Dubl . See also:Soc . (1879–188o) . Experiments were made by the present earl tc determine the amount of See also:heat radiated from the moon . See also:Rugby School (See also:Temple Obs.), lat . +52° 22' 7", long. o h . 5 M . 2 s . W . Founded in 1872; 8i-in. refr. by See also:Clark, used for obs. of double stars and of stellar spectra . Stonyhurst See also:College obs., See also:Lancashire, lat . +53° 50' 40", long. o h . 9 M . 52.7 s . W . An 8-in. refr. by Troughton and Simms, mounted in 1867, used for spectroscopic and micrometric obs.; 15-in . See also:Perry memorial refr. by Grubb mounted in 1893, used chiefly for solar work . C . Private Observatories now discontinued . Mr J . G . See also:Barclay's obs., See also:Leyton, See also:Essex, lat . +51° 34' 34", long. o h. o m . 0.9 s . W . In activity from 1862 till 1886, Ic-in. refr. by Cooke; chiefly devoted to double stars . Mr G . See also:Bishop's obs., South See also:Villa, See also:Regent's See also:Park, See also:London, lat . +51° 31' 29.9", long. o h. o m . 37.1 s . W . In activity from 1836 to 1861, then removed to See also:Twickenham, and discontinued in 1874; had a 7-in. refr. by Dollond, with which Mr J . R . See also:Hind discovered ten See also:minor planets and several comets, and constructed maps of stars near the See also:ecliptic . Mr R . C . Carrington's obs., Redhill, lat . +51° 14' 25'3", long. o h. o m . 41.3 s . W . Established in 1854; had a 41-in. refr. and transit circle of 5-in. ap . (now at Radcliffe Ohs.) . With the latter a See also:catalogue of the positions of 3735 stars within 9° of the See also:pole, with the former See also:regular obs. of sun-spots, were made from 1853 to 1861 . 956 Mr A . A .
Common's obs., See also:Ealing, London, W
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(1876-1903)
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18-in. s.g. refl. erected in 1876, s.g. refl. of 36-in. ap
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(See also:mirror by Calver, mounting by the owner), erected in 1879; chiefly used for See also:celestial See also:photography, replaced by a refl. of 5-ft. ap. in 1889
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See also:Colonel See also: Cooper, who in 1834 erected a refr. of 13.3-in. ap . (o.g. by Cauchoix) . This instrument was from 1848 to 1856 used for determining the approximate places of 60,000 stars near the ecliptic . The obs. was restored in 1874, and the refr. was used for double-star obs. till 1883 . Earl of Crawford's obs., Dunecht, See also:Aberdeenshire, lat . +57° 9' 36", long. o h . 9 M . 40 s . W . Founded in 1872; 15-10. refr. by Grubb, 12-in. s.g. refl. by Browning, two 6-in. and several smaller refrs. meridian circle by Simms similar to the one at Cambridge, numerous spectroscopes and minor instruments, also a large library and a collection of See also:physical instruments . Chiefly devoted to spectroscopic and cometary obs . Whole equipment presented to Edinburgh obs. in 1888 . Mr E . Crossley's obs., Bermerside, See also:Halifax, See also:Yorkshire . Equatorial refr. by Cooke of 9.3 in. ap., erected in 1871, chiefly used for obs. of double stars till 1902 . Rev W . R . See also:Dawes's obs., first at See also:Ormskirk (1830-1839), lat . +53° 43' 18", long. o h . II m . 36 s . W.; afterwards at See also:Cranbrook, See also:Kent (1844-185o), lat . +51° 6' 31", long. o h . 2 M. io•8 s . E.; then at Wateringbury, near See also:Maidstone, lat . +51° 15' 12", long. o h . I m . 39.8 s . E., till 1857; and finally at Hopefield, Haddenham, lat . +51° 45' 54", long. o h . 3 M . 43.4 s . W., till Mr Dawes's See also:death in 1868 . Possessed at first only small instruments, then successively a 6-in. refr. by Merz, a 72-in. and an 8i-in. refr. by Clark, and an 8-in. refr. by Cooke, with all of which a See also:great many See also:measures of double stars were made . Mr W . De La Rue's obs., Cranford, See also:Middlesex, lat . +51° 28' 57.8", long. o h . I m . 37.5 s . W . Established in 1857; with 13-in. refl , de-voted to solar and lunar photography . The Kew photoheliograph was employed here from 1858 to 1863 to take daily photographs of the sun . The refl. was presented to the Oxford univ. obs. in 1874 . Mr S . Groombridge's obs., See also:Blackheath, lat . +51° 28' 2.7", long. o h. o m. o•6 s . E . In 1806 Mr Groombridge obtained a new transit circle of 4-ft. diameter by Troughton, with which he up to 1816 observed stars within 5o° of the pole forming a catalogue of 4243 stars .
Sir See also: 27.7 s . W . Founded in 1856; furnished with an 8-in. refr . (by Clark and Cooke) . In 187o was erected an equat. mounting with a I5-in. refr. and a Cassegrain refl. of 18-in. ap., both made by Grubb for the Royal Society . With these Sir W . Huggins has made his well-known spectroscopic observations and photographs of stellar spectra . The instruments were transferred to the Cambridge obs. in 1908 . Rev T . J . Hussey's obs., See also:Hayes, Kent, lat . +51° 22' 38", long. o h. o m . 3.6 s . E . In activity from about 1825 for about twelve years; 62-in. refr. by Fraunhofer, used for making one of the star maps published by the See also:Berlin See also:Academy . Mr G . Knott's obs., Cuckfield, See also:Sussex (from 186o to 1873 at Woodcroft, lat . +51° 0' 41", long. o h. o m . 34 s . W., afterwards at See also:Knowles See also:Lodge, Cuckfield) ; 7.3-in. refr. by Clark, used for observing double stars and variable stars till 1894 . Mr W . Lassell's obs., from 184o to 1861 at Starfield near See also:Liver-See also:pool, lat . +53° 25' 28", long. o h . 11 m .
38.7 S
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W.; contained refl. of 9- and 24-in. ap.; employed for obs. of the satellites of Saturn, Uranus and See also:Neptune, and of nebulae
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The 2-ft. refl. was used at See also:Malta in 1852-1853, and a 4-ft. refl. was mounted in 1861, also at Malta, and used till 1864 for obs. of satellites and nebulae
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The eighth satellite of Saturn, the two inner satellites of Uranus and the satellite of Neptune were discovered at Starfield by Mr Lassell
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Dr J
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See also: McClean's obs., Rusthall House, Tunbridge See also:Wells . Phot . 12-in. refr. and o.g. See also:prism by Grubb used for photos. of star spectra, 1895-1904 . Mr R . S . Newall's obs., See also:Gateshead, See also:Newcastle-on-See also:Tyne . A 25-in. ref r. by Cooke was mounted in 1870 but never used; presented to Cambridge obs. in 1891 . Dr See also:Isaac See also:Roberts's obs., Crowborough, Sussex, lat . +51° 3' 7" long. o h. o m . 37 s . E . 20-in. s.g. refl. by Grubb (with 7-in. refr.) used for phot. of nebulae and clusters 1890-1904 .
Captain W
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H
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Smyth's obs., See also:Bedford, lat
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+52° 8' 27.6", long.. o h
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I m
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52.0 s
.
W
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In 183o Captain (afterwards See also:Admiral) Smyth erected a 6-in. refr. by Tulley, and observed the double stars and nebulae contained in his " Bedford Catalogue " (1844)
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Sir See also: Herschel measured double stars, in 1821-1823 . In 1826 South erected an obs. at Campden Hill, Kensington, lat . +51° 30' 12", long. o h. o m . 46.8 s . W., and procured a 12-in. o.g. from Cauchoix . As 'Troughton, however, failed to make a satisfactory mounting, the See also:glass was never used till after it had been presented to Dublin ohs. in 1862 . Colonel Tomline's obs. at Orwell Park, See also:Ipswich, lat . +52° 0' 33", long. o h . 4 M . 55.8 s . E. lo-in. refr. by Merz, used for obs. of comets from 1874 to 1889 . Mr W .
E
.
See also:
E., where a catalogue of the right ascensions of 1318 stars was formed from obs. with a transit instrument by Jones
.
In 1842 a new obs. was built at Wrottesley See also:
Founded in 1667, when the construction of a large and monumental building was commenced by the architect See also:Claude See also:Perrault
.
J
.
D
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See also:Cassini's obs. made the institution for some time the most celebrated obs. existing, but later the activity declined, although several eminent men, as Bouvard and See also:Arago, have held the See also:post of director
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Since 1854, when See also:Leverrier assumed the directorship, the obs. have been conducted with regularity, and, together with a number of most important theoretical See also:works, published in the See also:Annals (Observations and See also:Memoirs)
.
The principal instruments now in use are: a meridian circle by Secretan and Eichens, with an o.g. of 9:5-in. ap., another by Eichens (given by M
.
Bischoffsheim) of 7.5-in. ap., a 15-in. refr. by Lerebours and See also:Brunner, a 12-in. refr. by Secretan and Eichens, a refr. of 9.5-in. ap., an equat. coud6e by See also: +48° 51' 29", where See also:Lacaille observed from 1746 to 1750, and from 1754 to 1762, and the obs. at the E°See also:cole Militaire, lat . +48° 51' 5", built in 1768 and furnished with an 8-ft. mural quadrant by Bird, with which J . L. d'Agelet observed telescopic stars (1782-1785), and which was afterwards (1789-1801), under See also:Lalande's direction, employed for observing more than 50,000 stars, published in the Histoire See also:Celeste (18oi) . See also:Meudon, See also:close to Paris, lat . +48° 48' 18", long. o h . 8 m . 55.6 s . E . Founded in 1875; devoted to physical astronomy, and especially to celestial photography, under the direction of J . See also:Janssen; 32-in. vis. and 24i-in. phot. ref r. by Henry and Gautier, refl. by the same of 39-in. ap . There is a See also:branch obs. on Mont See also:Blanc, where a polar siderostat with 12-in. o.g. and 20-in. mirror is occasionally used for solar and spectroscopic work (15,780 ft. above See also:sea-level) . Montsouris, situated in the Montsouris Park, south of Paris, lat . +48° 49' 18", long. o h . 9 M . 20.7 S . E . Founded in 1875 for the training of See also:naval See also:officers . Juvissy (See also:Seine-et-See also:Oise), private obs. of N . C . Flammarion, lat . +48° 41' 37", long. o h . 9 M . 29.0 s . E . 91-in. refr. used for obs. of planets . Chevreuse (Seine-et-Oise), private obs. of M . Farman (1903), lat, +48° 42' 33", long. o h . 8 m . 4.5 s . E.; 8-in. refr. by Mailhat used on double stars . See also:Besancon, chronometric and meteorol. obs., lat . +470 14' 59.0", long. o h . 23 M . 57.1 s . E . Opened 1884; 8-in. refr., 12-in. equat, coud6e, 72-in. transit circle, all by Gautier . See also:Lyons, old obs. in lat . 45° 45' 46", long. o h . 19 M . 18 s . E., at the Jesuit college . A new obs. was erected in 1877 at St G6nis-See also:Laval, at some distance from the city, lat . + 45° 41' 41 .o", long. o h . 19 M . 8.5 s . E . Transit circle by Eichens (6-in. o.g.), i2-in. equat. coud6e by Gautier, 12-in. siderostat . See also:Bordeaux, univ. obs. at Floirac, 4 km . N.W. of the city, lat . +44° 50' 7.3", long. o h . 2 M . 5.5 s . W . Founded 1882; 7-in. transit circle by Eichens, I4-in. refr. by Merz and Gautier, 13-in. phot. refr. by Henry and Gautier . See also:Marseilles, lat . 43° i8' 17.5", long. o h . 21 M . 34.6 s . E . Originally belonging to the See also:Jesuits, taken over by the See also:ministry of the See also:navy in 1749 . It was here that J . L . Pons made his numerous discoveries of comets . New buildings erected in 1869; 9i-in . Merz. refr., refl. of 32-in. ap. s.g. by See also:Foucault, 71-in. transit circle . See also:Toulouse, lat . 430 36' 45.0", long. o h . 5 M . 49.9 S . E . Erected in 1841 (Darquier had observed at the See also:Lyceum towards the end of the 18th century); reorganized 1873; 9-in. refr. and phot. refr. by Gautier, i3-in. and 32-in. refl . See also:Nice, lat . + 43° 43' 16.9" long. o h . 29 M . 12.2 s . E., founded and endowed by R . L . Bischoffsheim for the See also:Bureau de See also:Longitude (188o), situated at Mont See also:Gros, See also:north-See also:east of Nice; a refr. of 3o-in. ap. by Henry and Gautier, a meridian circle by Brunner of 8-in. ap., 15-in. refr. and 151-in. equat. coudee by Henry and Gautier . A bbadia (Basses See also: |