Fișier:NGC 4388 - HST - Potw1649a.tif

Mărește rezoluția imaginii (3.807 × 2.679 pixeli, mărime fișier: 20,21 MB, tip MIME: image/tiff)

Acest fișier se află la Wikimedia Commons. Consultați pagina sa descriptivă acolo.
Descriere

A transformation in Virgo

The constellation of Virgo (The Virgin) is especially rich in galaxies, due in part to the presence of a massive and gravitationally-bound collection of over 1300 galaxies called the Virgo Cluster. One particular member of this cosmic community, NGC 4388, is captured in this image, as seen by the NASA/ESA Hubble Space Telescope’s Wide Field Camera 3 (WFC3).

Located some 60 million light-years away, NGC 4388 is experiencing some of the less desirable effects that come with belonging to such a massive galaxy cluster. It is undergoing a transformation, and has taken on a somewhat confused identity.

While the galaxy’s outskirts appear smooth and featureless, a classic feature of an elliptical galaxy, its centre displays remarkable dust lanes constrained within two symmetric spiral arms, which emerge from the galaxy’s glowing core — one of the obvious features of a spiral galaxy. Within the arms, speckles of bright blue mark the locations of young stars, indicating that NGC 4388 has hosted recent bursts of star formation. Despite the mixed messages, NGC 4388 is classified as a spiral galaxy. Its unusual combination of features are thought to have been caused by interactions between NGC 4388 and the Virgo Cluster. Gravitational interactions — from glancing blows to head-on collisions, tidal influencing, mergers, and galactic cannibalism — can be devastating to galaxies. While some may be lucky enough to simply suffer a distorted spiral arm or newly-triggered wave of star formation, others see their structure and contents completely and irrevocably altered.

Credit:

ESA/Hubble & NASA

Coordinates
Position (RA): 	12 25 46.52
Position (Dec):	12° 39' 54.49"
Field of view: 	2.51 x 1.77 arcminutes
Orientation:   	North is 26.4° left of vertical

Colours & filters Band	Wavelength	Telescope
Optical           U	336 nm  	Hubble Space Telescope WFC3
Optical           B	438 nm  	Hubble Space Telescope WFC3
Optical           I	814 nm  	Hubble Space Telescope WFC3
Optical           B	438 nm  	Hubble Space Telescope WFC3
Optical           I	814 nm  	Hubble Space Telescope WFC3
.
Dată 5 December 2016, 6:00 (Release)
Sursă http://spacetelescope.org/images/potw1649a/ http://spacetelescope.org/static/archives/images/original/Potw1649a.tif
Autor Credit: ESA/Hubble & NASA
Permisiune
(Reutilizarea acestui fișier)
w:ro:Creative Commons
atribuind
atribuind
ESA/Hubble images, videos and web texts are released by the ESA under the Creative Commons Attribution 4.0 International license and may on a non-exclusive basis be reproduced without fee provided they are clearly and visibly credited. Detailed conditions are below; see the ESA copyright statement for full information. For images created by NASA or on the hubblesite.org website, or for ESA/Hubble images on the esahubble.org site before 2009, use the {{PD-Hubble}} tag.
Conditions:
  • The full image or footage credit must be presented in a clear and readable manner to all users, with the wording unaltered (for example: "ESA/Hubble"). Web texts should be credited to ESA/Hubble (except when used by media). The credit should not be hidden or disassociated from the image footage. Links should be active if the credit is online. See the usage rights Q&A section on the ESA copyright page for guidance.
  • ESA/Hubble materials may not be used to state or imply the endorsement by ESA/Hubble or any ESA/Hubble employee of a commercial product or service.
  • ESA/Hubble requests a copy of the product sent to them to be indexed in their archive.
  • If an image shows an identifiable person, using that image for commercial purposes may infringe that person's right of privacy, and separate permission should be obtained from the individual.
  • If images or visuals are changed significantly from the original work (apart from resizing, cropping), we suggest that the changes are mentioned after the credit line. For example "Original image by ESA/Hubble (M. Kornmesser), warping and recolouring by NN".

Notes:

  • Note that this general permission does not extend to the use of ESA/Hubble's logo, which shall remain protected and may not be used or reproduced without prior and individual written consent of ESA/Hubble.
  • Also note that music, scientific papers and code on the esahubble.org site are not released under this license and can not be used for non-ESA/Hubble products.
  • By reproducing ESA/Hubble material, in part or in full, the user acknowledges the terms on which such use is permitted.
w:ro:Creative Commons
atribuind
Acest fișier a fost eliberat sub licența Creative Commons Atribuire 4.0 Internațională.
Atribuire: ESA/Hubble
Sunteți liber:
  • să partajați cu alții – aveți dreptul de a copia, distribui și transmite opera
  • să adaptați – aveți dreptul de a adapta opera
În următoarele condiții:
  • atribuind – Trebuie să atribuiți opera corespunzător, introducând o legătură către licență și indicând dacă ați făcut schimbări. Puteți face asta prin orice metodă rezonabilă, dar nu într-un fel care ar sugera faptul că persoana ce a licențiat conținutul v-ar susține sau ar aproba folosirea de către dumneavoastră a operei sale.

Captions

Add a one-line explanation of what this file represents

Items portrayed in this file

subiectul reprezentat

Istoricul fișierului

Apăsați pe Data și ora pentru a vedea versiunea trimisă atunci.

Data și oraMiniaturăDimensiuniUtilizatorComentariu
actuală5 decembrie 2016 08:32Miniatură pentru versiunea din 5 decembrie 2016 08:323.807x2.679 (20,21 MB)Fabian RRRR{{Information |Description=A transformation in Virgo The constellation of Virgo (The Virgin) is especially rich in galaxies, due in part to the presence of a massive and gravitationally-bound collection of over 1300 galaxies called the Virgo Cluster....

Următoarele pagini conțin această imagine:

Utilizarea globală a fișierului

Următoarele alte proiecte wiki folosesc acest fișier:

Informații