[go: nahoru, domu]

Μετάβαση στο περιεχόμενο

Αρχείο:Hubble Interacting Galaxy NGC 6090 (2008-04-24).jpg

Τα περιεχόμενα της σελίδας δεν υποστηρίζονται σε άλλες γλώσσες.
Αυτό το αρχείο προέρχεται από το Wikimedia Commons
Από τη Βικιπαίδεια, την ελεύθερη εγκυκλοπαίδεια

Εικόνα σε υψηλότερη ανάλυση (3.481 × 3.481 εικονοστοιχεία, μέγεθος αρχείου: 13,65 MB, τύπος MIME: image/jpeg)

Περιγραφή

NGC 6090 is a beautiful pair of spiral galaxies with an overlapping central region and two long tidal tails formed from material ripped out of the galaxies by gravitational interaction. The two visible cores are approximately 10,000 light-years apart, suggesting that the two galaxies are at an intermediate stage in the merging process. The Hubble image reveals bright knots of newborn stars in the region where the two galaxies overlap. The right hand component has a clear spiral structure if viewed face-on, while the other is seen edge-on with no spiral arms visible. NGC 6090 is located in the constellation of Draco, the Dragon, about 400 million light-years away from Earth. A number of fainter, and more distant, background galaxies is seen in the image. This system has much in common with the famous Antennae galaxies both in terms of how far the merger has progressed and in our viewing angle.

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 November 2008.

About the object
Object name NGC 6090, Mrk 0496, VV 626, I Zw 135, KPG 486
Object description Interacting Galaxies
Position (J2000) 16 11 40.30
+52 27 25.0
Constellation Draco
Distance 400 million light-years (100 million parsecs)
About the data
Data description The Hubble image was created using HST data from proposals 10592 and 10575: A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University) and G. Ostlin (Stockholm University)
Instrument ACS/WFC
Exposure date(s) September 18, 2005 and November 12, 2005
Exposure time 1 hour
Filters F435W (B), FR656N (Halpha), and F814W (I)
Ημερομηνία
Πηγή http://hubblesite.org/newscenter/archive/releases/2008/16/image/bx/ (direct link)
Δημιουργός NASA, ESA, the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University), and G. Ostlin (Stockholm University)
Άδεια
(Επαναχρησιμοποίηση αυτού του αρχείου)
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.

Λεζάντες

Δεν ορίστηκε λεζάντα

Items portrayed in this file

απεικονίζει

Ιστορικό αρχείου

Κλικάρετε σε μια ημερομηνία/ώρα για να δείτε το αρχείο όπως εμφανιζόταν εκείνη τη στιγμή.

Ώρα/Ημερομ.ΜικρογραφίαΔιαστάσειςΧρήστηςΣχόλια
τελευταία20:58, 27 Απριλίου 2008Μικρογραφία για την έκδοση της 20:58, 27 Απριλίου 20083.481 × 3.481 (13,65 MB)とある白い猫{{Information |Description=NGC 6090 is a beautiful pair of spiral galaxies with an overlapping central region and two long tidal tails formed from material ripped out of the galaxies by gravitational interaction. The two visible cores are approximately 10

Τα παρακάτω λήμματα συνδέουν σε αυτό το αρχείο:

Καθολική χρήση αρχείου

Τα ακόλουθα άλλα wiki χρησιμοποιούν αυτό το αρχείο:

Μεταδεδομένα