File:BlackHole Lensing.gif

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BlackHole_Lensing.gif(320 × 256 pixel, tamaño di fail: 12.35 MB, MIME type: image/gif, looped, 150 frames, 1.5 s)

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Deskripshon
English: Animated simulation of gravitational lensing caused by a black hole going past a background galaxy. A secondary image of the galaxy can be seen within the black hole Einstein ring on the opposite direction of that of the galaxy. The secondary image grows (remaining within the Einstein ring) as the primary image approaches the black hole. The surface brightness of the two images remains constant, but their angular size varies, hence producing an amplification of the galaxy luminosity as seen from a distant observer. The maximum amplification occurs when the background galaxy (or in the present case a bright part of it) is exactly behind the black hole.
Français : Simulation animée de la lentille gravitationnelle causée par un trou noir passant en arrière-plan d'une galaxie. Une image secondaire de la galaxie peut être vue dans le trou noir de l' anneau d'Einstein dans la direction opposée à celle de la galaxie. L'image secondaire grandit (restant dans l'anneau d'Einstein) lorsque l'image principale s'approche du trou noir. La Brillance de surface des deux images reste constante, mais leur taille apparente varie, produisant ainsi une amplification de la luminosité de la galaxie vue d'un observateur distant. L'amplification maximale se produit lorsque la galaxie d'arrière-plan (ou, dans le cas présent, une partie brillante de celle-ci) est exactement derrière le trou noir.
Fecha 4 yanüari 2006 (original upload date)
Fuente No machine-readable source provided. Own work assumed (based on copyright claims).
Outor No machine-readable author provided. Alain r assumed (based on copyright claims).

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This licensing tag was added to this file as part of the GFDL licensing update.
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This file is licensed under the Creative Commons Attribution-Share Alike 2.5 Generic, 2.0 Generic and 1.0 Generic license.
Bo ta liber:
  • pa kompartí – pa kopia, distribuí i transmití e obra
  • pa rekombiná – pa adaptá e obra
Di akuerdo ku e próksimo kondishonnan:
  • atribushon – Bo mester duna krédito na e outor, duna un lenk na e lisensia, i indiká si a hasi kambio. Bo por hasi esei na kualke manera rasonabel, perono na manera ku por sugerí ku esun ku ta otorgá e lisensia ta respaldá abo òf bo uzo.
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physics ingles

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checksum ingles

54968280b9898ae12094037f881ad437e5a58301

determination method ingles: SHA-1 ingles

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256 pixel

width ingles

320 pixel

Historia di fail

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Fecha/OraMiniaturaDimenshonnanUsuarioKomentario
aktual01:43, 16 febrüari 2006Miniatura di e vershon di 01:43, 16 febrüari 2006320 × 256 (12.35 MB)Falcorian
22:42, 4 yanüari 2006Miniatura di e vershon di 22:42, 4 yanüari 2006320 × 256 (13 MB)Alain rLensing by a black hole Effet de lentille gravitationnelle par un trou noir

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