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ຈາກ Wiktionary

BlackHole_Lensing.gif (໓໒໐ × ໒໕໖ ປິກເຊລ, ຂະໜາດໄຟລ໌: ໑໒,໓໕ MB, MIME type: image/gif, looped, ໑໕໐ frames, ໑,໕ s)

ໄຟລ໌ນີ້ແມ່ນມາຈາກ Wikimedia Commons ແລະອາດຈະຖືກນໍາໃຊ້ໂດຍໂຄງການອື່ນ ລາຍ​ລະ​ອຽດ​ກ່ຽວ​ກັບຫນ້າ​ລາຍ​ລະ​ອຽດ​ໄຟລ​໌​ສະແດງ​ຢູ່​ຂ້າງ​ລຸ່ມ​ນີ້​

ສະຫຼຸບ

ລາຍລະອຽດ
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.
ວັນທີ ໔ ມັງກອນ ໒໐໐໖ (original upload date)
Source No machine-readable source provided. Own work assumed (based on copyright claims).
ຜູ້ຂຽນ No machine-readable author provided. Alain r assumed (based on copyright claims).

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You are free:
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Under the following conditions:
  • ສະແດງທີ່ມາ – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
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This licensing tag was added to this file as part of the GFDL licensing update.
w:en:Creative Commons
ສະແດງທີ່ມາ ແບ່ງປັນຄືກັນ
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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Under the following conditions:
  • ສະແດງທີ່ມາ – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
  • ແບ່ງປັນຄືກັນ – If you remix, transform, or build upon the material, you must distribute your contributions under the same or compatible license as the original.
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checksum ອັງກິດ

54968280b9898ae12094037f881ad437e5a58301

determination method or standard ອັງກິດ: SHA-1 ອັງກິດ

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12951779 ໄບຕ໌

height ອັງກິດ

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width ອັງກິດ

໓໒໐ pixel

duration ອັງກິດ

1.5 second

ປະຫວັດໄຟລ໌

ຄລິກທີ່ ວັນທີ/ເວລາ ເພື່ອເບິ່ງໄຟລ໌ດັ່ງທີ່ມັນປາກົດໃນເວລານັ້ນ

ວັນເວລາຮູບຍໍ່ມິຕິຜູ້ໃຊ້ຄວາມເຫັນ
ປະຈຸບັນ໐໑:໔໓, ໑໖ ກຸມພາ ໒໐໐໖ຮູບຍໍ່ສຳລັບເວີຊັນ ໐໑:໔໓, ໑໖ ກຸມພາ ໒໐໐໖໓໒໐ × ໒໕໖(໑໒,໓໕ MB)Falcorian
໒໒:໔໒, ໔ ມັງກອນ ໒໐໐໖ຮູບຍໍ່ສຳລັບເວີຊັນ ໒໒:໔໒, ໔ ມັງກອນ ໒໐໐໖໓໒໐ × ໒໕໖(໑໓ MB)Alain rLensing by a black hole Effet de lentille gravitationnelle par un trou noir

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