File:Planetary transit de.svg

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If you can, help make this description accessible to all by translating it into other languages. – Thanks!
Català: Imatge d'un planeta que passa per davant d'un estel, per a il·lustrar el mètode de trànsit per a descobrir planetes extrasolars. Les mides de l'estel, del planeta i de l'òrbita són semblants a les de HD 209458b.
Deutsch: Bild eines Planeten beim Transit eines Sterns, beispielsweise zur Veranschaulichung der Transit-Methode bei der Entdeckung extrasolarer Planeten. Die Größenverhältnisse von Stern und Planet sind grob angenähert an diejenigen von HD 209458b. Inspiriert durch ein Bild auf http://www.iac.es/proyect/tep/transitmet.html
English: Image of a planet transiting a star, for illustration of transit method of discovery of extrasolar planets. Sizes of the star, the planet and its orbit are roughly like HD 209458b.
Español: Imagen de un planeta que transita por delante de una estrella, para una ilustración del método de tránsitos para descubrimiento de planetas extrasolares. Tamaños de la estrella, del planeta y de su órbita son aproximadamente similares a los de HD 209458 b.
Ripoarisch: Beld vun enem Planeet, dä aan enem Stääb vorbei fleesch, jemaat, öm de Dorschjangsmetoodee ze zeije, för Plateete ußerhallef vum Sunnesüßteem ze äntdäcke. Dem Stään, däm Planeet, un de bahn iehr Jrüße paße ent ätwa zom HD 209458b}
Македонски: Планета како преминува ѕвезда. Ова е методот за откривање на егзопланети.
Русский: Иллюстрация транзитного метода обнаружения экзопланет: изображение планеты, проходящей на фоне звезды. Соотношение размеров планеты и звезды примерно соответствуют HD 209458b.
Српски / srpski: Слика планете како пролази испред звезде, за илустрацију транзитног метода откривања планета ван Сунчевог система. Величине звезде, планете и њене орбите грубо одговарају HD 209458b. Инспирисано сликом на http://www.iac.es/proyect/tep/transitmet.html
தமிழ் : வான்கோள் கடக்கை
മലയാളം : ഒരു ഗ്രഹം നക്ഷത്രത്തെ സംതരണം ചെയ്യുന്നതിന്റെ ചിത്രീകരണം, സൗരയൂഥത്തിനുമപ്പുറമുള്ള ഗ്രഹങ്ങളെ സൂചിപ്പിക്കുന്നതിനായി ചിത്രീകരിച്ചത്. വസ്തുക്കളുടെ വലുപ്പം തോതനുസരിച്ചല്ല.
العربية : عبور كوكب عبر قرص النجم التابع له. ويبين المنحنى أسفله تغير شدة الضوء المسجلة مع زمن العبور (منحنى ضوئي).
Date (translation), 2005-12-31 (upload to Commons)
Source translated from Planetary transit.svg
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This licensing tag was added to this file as part of the GFDL licensing update.
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attribution share alike
This file is licensed under the Creative Commons Attribution-Share Alike 2.5 Generic, 2.0 Generic and 1.0 Generic license.
You are free:
  • to share – to copy, distribute and transmit the work
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Original upload log[edit]

This image is a derivative work of the following images:

  • File:Planetary transit.svg licensed with Cc-by-sa-2.5,2.0,1.0, Cc-by-sa-3.0-migrated, GFDL,
    • 2007-04-13T15:36:28Z Tene 1134x354 (3712 bytes) Cleanup
    • 2006-01-02T22:12:24Z Nikola Smolenski 1134x354 (9695 bytes) Fixed bug about orbit
    • 2006-01-02T22:05:23Z Nikola Smolenski 1134x354 (9696 bytes) Larger default size (I hope)
    • 2005-12-31T09:02:21Z Nikola Smolenski 283x89 (9579 bytes) Image of a [[planet]] transiting a [[star]], for illustration of transit method of discovery of extrasolar planets. Sizes of the star, the planet and its orbit are roughly like [[w:HD 209458b|]]. Inspired by image at http://w

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Date/TimeThumbnailDimensionsUserComment
current20:09, 31 August 2011Thumbnail for version as of 20:09, 31 August 20111,134 × 354 (8 KB)-donald- (talk | contribs)Anpassung
19:09, 29 August 2011Thumbnail for version as of 19:09, 29 August 20111,134 × 354 (6 KB)-donald- (talk | contribs)Bugfix
18:30, 29 August 2011Thumbnail for version as of 18:30, 29 August 20111,134 × 354 (6 KB)-donald- (talk | contribs)Text verschoben
14:26, 12 August 2011Thumbnail for version as of 14:26, 12 August 20111,134 × 354 (4 KB)File Upload Bot (Jarry1250) (talk | contribs){{Information |Description= == {{int:filedesc}} == {{de|Bild eines Planeten beim Transit eines Sterns, beispielsweise zur Veranschaulichung der Transit-Methode bei der Entdeckung extrasolarer Planeten. Die Größenverhältni

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