Toggle search
Toggle menu
243,3 tis.
110
18
643,2 tis.
Hrvatska internetska enciklopedija
Toggle preferences menu
Toggle personal menu
Niste prijavljeni
Your IP address will be publicly visible if you make any edits.

Datoteka:Hubble Interacting Galaxy NGC 3256 (2008-04-24).jpg

Izvor: Hrvatska internetska enciklopedija
More actions

Vidi sliku u punoj veličini ‎((3.640 × 3.640 piksela, veličina datoteke: 13,24 MB, <a href="/wiki/MIME" title="MIME">MIME</a> tip: image/jpeg))


Logo Wikimedijinog spremnika Ova je datoteka sa stranica Zajedničkog poslužitelja Zaklade Wikimedije i smiju je rabiti drugi projekti. Opis s njezine stranice s opisom datoteke prikazan je ispod.
Opis

NGC 3256 is an impressive example of a peculiar galaxy that is actually the relict of a collision of two separate galaxies that took place in a distant past. The telltale signs of the collision are two extended luminous tails swirling out from the galaxy. NGC 3256 belongs to the Hydra-Centaurus supercluster complex and provides a nearby template for studying the properties of young star clusters in tidal tails. The system hides a double nucleus and a tangle of dust lanes in the central region. The tails are studded with a particularly high density of star clusters.

This image is part of a large collection of 59 images of merging galaxies taken by the Hubble Space Telescope and released on the occasion of its 18th anniversary on 24th April 2008.

About the object
Object name NGC 3256, VV 065, AM 1025-433
Object description Interacting Galaxies
Position (J2000) 10 27 51.57
-43 54 13.4
Constellation Vela
Distance 100 million light-years (50 million parsecs)
About the data
Data description The Hubble image was created using HST data from proposal 10592: A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)
Instrument ACS/WFC
Exposure date(s) November 5, 2001
Exposure time 35 minutes
Filters F435W (B) and F814W (I)
Datum
Izvor http://hubblesite.org/newscenter/archive/releases/2008/16/image/br/ (direct link)
Autor NASA, ESA, the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)
Dopuštenje
(Naknadna uporaba ove datoteke)
Public domain
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.

Opisi

Dodajte kratko objašnjenje što predstavlja ova datoteka

Predmeti prikazani u ovoj datoteci

motiv

nastanak

24. travnja 2008

Povijest datoteke

Kliknite na datum/vrijeme kako biste vidjeli datoteku kakva je tada bila.

Datum/VrijemeMinijaturaDimenzijeSuradnikKomentar
sadašnja19:44, 27. travanj 2008.Minijatura za inačicu od 19:44, 27. travanj 2008.3.640 × 3.640 (13,24 MB)wikimediacommons>とある白い猫{{Information |Description=NGC 3256 is an impressive example of a peculiar galaxy that is actually the relict of a collision of two separate galaxies that took place in a distant past. The telltale signs of the collision are two extended luminous tails sw

Na ovu sliku vode poveznice sa sljedećih stranica:

Metapodatci

Ova datoteka sadržava dodatne podatke koje je vjerojatno dodala digitalna kamera ili skener u procesu snimanja odnosno digitalizacije. Ako je datoteka mijenjana, podatci možda nisu u skladu sa stvarnim stanjem.

Dobavljeno iz "https://enciklopedija.cc/wiki/Datoteka:Hubble_Interacting_Galaxy_NGC_3256_(2008-04-24).jpg"