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There is a page named "Template:Variable star" on Wikipedia

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  • Vmax = ±nnm, Vmin = ±nnm, P = n.nn d Usage: {{Variable star|visual magnitude at maximum|visual maximum at minimum|period in days}} See also Template:VSA...
    484 bytes (26 words) - 20:32, 18 November 2014
  • Template documentation Stub hierarchy Var-star-stub Star-stub Stub This template is used to identify a variable star–related stub. It uses {{asbox}}, which...
    295 bytes (312 words) - 03:37, 5 August 2013
  • [history] [purge] The above documentation is transcluded from Template:Variable star topics/doc. (edit | history) Editors can experiment in this template's...
    3 KB (42 words) - 09:07, 9 October 2023
  • ΔV = ?m ΔVmax = nnm, P = n.nn d Usage: {{VSA|amplitude of visual magnitude variation|period in days}} See also Template:Variable star...
    342 bytes (23 words) - 07:10, 18 September 2014
  • radius = | rotation = | temperature = | stellar = | variable = | planets = }} By default, {{Infobox star}} displays a map of a constellation, set by the constellation...
    18 KB (1,571 words) - 13:03, 24 September 2019
  • 2008 March 12 2008 March 14 > Picture of the day Mira A is a red giant variable star in the constellation Cetus. This ultraviolet-wavelength image mosaic...
    705 bytes (94 words) - 19:02, 15 March 2015
  • ALT1 ...that RZ Gruis is a cataclysmic variable star, a type which the American Association of Variable Star Observers recommends be watched in case...
    3 KB (233 words) - 07:01, 13 May 2021
  • double star 1,000 light-years from Earth with apparent magnitude 4.03; CS Cam, a 4.21-magnitude variable star; and α Cam, a blue-hued supergiant star of magnitude...
    1 KB (191 words) - 05:23, 19 March 2019
  • October 31 > Picture of the day Eta Carinae, a hypergiant luminous blue variable star in the Carina constellation and one of the most massive and most luminous...
    792 bytes (97 words) - 23:54, 17 March 2019
  • {{Nearest star systems|2}} displays {{Nearest star systems|3}} displays The above documentation is transcluded from Template:Nearest star systems/doc...
    1 KB (97 words) - 21:24, 22 November 2023
  • |state= parameter may be used: {{Star|state=expanded}} will show the template expanded, i.e. fully visible. {{Star|state=autocollapse}} will show the...
    8 KB (125 words) - 15:24, 7 June 2024
  • be used: {{Neutron star|state=collapsed}} will show the template collapsed, i.e. hidden apart from its title bar. {{Neutron star|state=expanded}} will...
    2 KB (125 words) - 16:56, 4 January 2024
  • Star Catalogue --> | SCR = <!-- Super-COSMOS RECONS --> | TOI = <!-- Tess Object of Interest --> | TYC = <!-- Tycho Catalogue --> | V = <!-- Variable...
    12 KB (509 words) - 14:31, 21 May 2024
  • amended if appropriate. The above documentation is transcluded from Template:Star systems within 10–15 light-years/doc. (edit | history) Editors can experiment...
    2 KB (60 words) - 00:49, 6 January 2024
  • amended if appropriate. The above documentation is transcluded from Template:Star systems within 10 light-years/doc. (edit | history) Editors can experiment...
    2 KB (59 words) - 00:31, 6 January 2024
  • Back to T:TDYK Article history ) ... that Chi Cygni (pictured) is a variable star that is over 10,000 times brighter at its maximum than at its minimum...
    5 KB (629 words) - 05:51, 17 April 2021
  • 2023 October 12 > Picture of the day AG Carinae is a luminous blue variable star in the constellation Carina. It is one of the most luminous stars in...
    2 KB (195 words) - 00:00, 11 November 2023
  • amended if appropriate. The above documentation is transcluded from Template:Star systems within 15–20 light-years/doc. (edit | history) Editors can experiment...
    3 KB (60 words) - 16:35, 6 March 2024
  • (UTC) ( Back to T:TDYK Article history ) ... that the W Ursae Majoris variable star system V1191 Cygni has one of the highest known rates of mass transfer...
    1 KB (130 words) - 12:29, 23 March 2015
  • T:TDYK Article history ) ... that active galaxy 3C 120 was given the variable star designation BW Tauri because of its variability in the visible spectrum...
    3 KB (201 words) - 12:54, 26 July 2023
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