Fichier:Quasar PG 0052+251 (opo9635a1).tiff
Quasar_PG_0052+251_(opo9635a1).tiff (296 × 296 pixels, taille du fichier : 122 kio, type MIME : image/tiff)
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Description
DescriptionQuasar PG 0052+251 (opo9635a1).tiff |
English: This image shows quasar PG 0052+251, which is 1.4 thousand million light-years from Earth, at the core of a normal spiral galaxy. Astronomers are surprised to find host galaxies, such as this one, that appear undisturbed by the strong quasar radiation.Quasars reside in a variety of galaxies, from normal to highly disturbed. When seen through ground-based telescopes, these compact, enigmatic light sources resemble stars, yet they are thousand of millions of light-years away and several hundred thousand million times brighter than normal stars. Astronomers believe that a quasar turns on when a massive black hole at the nucleus of a galaxy feeds on gas and stars. As the matter falls into the black hole, intense radiation is emitted. Eventually, the black hole will stop emitting radiation once it consumes all nearby matter. Then it needs debris from a collision of galaxies or another process to provide more fuel.This image shows quasar PG 0052+251, which is 1.4 billion light-years from Earth, at the core of a normal spiral galaxy. Astronomers are surprised to find host galaxies, such as this one, that appear undisturbed by the strong quasar radiation. |
Date | 19 novembre 1996 (date de téléversement) |
Source | Quasar PG 0052+251 |
Auteur | John Bahcall (Institute for Advanced Study, Princeton) Mike Disney (University of Wales) and NASA/ESA |
Autres versions |
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Conditions d’utilisation
Public domainPublic domainfalsefalse |
This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.
The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org. For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag. |
Éléments décrits dans ce fichier
dépeint
image/tiff
296 pixel
296 pixel
125 144 octet
03eb47eff5160df3e081faad043322c8738ccbb1
19 novembre 1996
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Historique du fichier
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Date et heure | Vignette | Dimensions | Utilisateur | Commentaire | |
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actuel | 22 juin 2024 à 00:34 | 296 × 296 (122 kio) | OptimusPrimeBot | #Spacemedia - Upload of https://esahubble.org/media/archives/images/original/opo9635a1.tif via Commons:Spacemedia |
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Métadonnées
Ce fichier contient des informations supplémentaires, probablement ajoutées par l'appareil photo numérique ou le numériseur utilisé pour le créer.
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Largeur | 296 px |
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Hauteur | 296 px |
Bits par composante |
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Schéma de compression | LZW |
Composition des pixels | RVB |
Titre de l’image | This image shows quasar PG 0052+251, which is 1.4 billion light-years from Earth, at the core of a normal spiral galaxy. Astronomers are surprised to find host galaxies, such as this one, that appear undisturbed by the strong quasar radiation. |
Nombre de composantes | 3 |
Nombre de rangées par bande | 295 |
Résolution horizontale | 72 pt/po |
Résolution verticale | 72 pt/po |
Arrangement des données | Format tronçonné |
Logiciel utilisé | Adobe Photoshop CS Windows |
Date de modification du fichier | 9 décembre 2003 à 17:47 |
Espace colorimétrique | Non calibré |