Fichier:NGC1156 - HST - Potw2234a.jpg

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Fichier d’origine (3 621 × 3 699 pixels, taille du fichier : 4,29 Mio, type MIME : image/jpeg)

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Description

Description
English: A Marvel of Galactic Morphology

The galaxy featured in this Picture of the Week has a shape unlike many of the galaxies familiar to Hubble. Its thousands of bright stars evoke a spiral galaxy, but it lacks the characteristic ‘winding’ structure. The shining red blossoms stand out as well, twisted by clouds of dust — these are the locations of intense star formation. Yet it also radiates a diffuse glow, much like an elliptical galaxy and its core of older, redder stars. This galactic marvel is known to astronomers as NGC 1156.

NGC 1156 is located around 25 million light-years from Earth, in the constellation Aries. It has a variety of different features that are of interest to astronomers. A dwarf irregular galaxy, it’s also classified as isolated, meaning no other galaxies are nearby enough to influence its odd shape and continuing star formation. The extreme energy of freshly formed young stars gives colour to the galaxy, against the red glow of ionised hydrogen gas, while its centre is densely-packed with older generations of stars.

Hubble has captured NGC 1156 before — this new image features data from a galactic gap-filling programme simply titled “Every Known Nearby Galaxy”. Astronomers noticed that only three quarters of the galaxies within just over 30 million light-years of Earth had been observed by Hubble in sufficient detail to study the makeup of the stars within them. They proposed that in between larger projects, Hubble could take snapshots of the remaining quarter — including NGC 1156. Gap-filling programmes like this one ensure that the best use is made of Hubble’s valuable observing time.

Credit:

ESA/Hubble & NASA, R. B. Tully, R. Jansen, R. Windhorst 

Coordinates
Position (RA):	2 59 41.66
Position (Dec):	25° 14' 18.32"
Field of view:	3.02 x 3.08 arcminutes
Orientation:	North is 82.1° right of vertical

Colours & filters
Band	Wavelength	Telescope
Optical V	606 nm	Hubble Space Telescope ACS
Optical r	625 nm	Hubble Space Telescope ACS
Optical I	814 nm	Hubble Space Telescope WFPC2
Optical I	814 nm	Hubble Space Telescope ACS
Optical NII	658 nm	Hubble Space Telescope ACS
Ultraviolet UV 300 nm Hubble Space Telescope WFPC2
Date 22 August 2022, 06:00(released)
Source https://esahubble.org/images/potw2234a/
Auteur

Credit:

ESA/Hubble & NASA, R. B. Tully, R. Jansen, R. Windhorst
Autorisation
(Réutilisation de ce fichier)

paternité
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paternité
Ce fichier est disponible selon les termes de la licence Creative Commons Attribution 4.0 International.
Attribution:
Credit: ESA/Hubble & NASA, R. B. Tully, R. Jansen, R. Windhorst
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dépeint

NGC 1156

type MIME

image/jpeg

taille des données

4 496 811 octet

hauteur

3 699 pixel

largeur

3 621 pixel

somme de contrôle

861686e264fcb81712a23917dc1ce7e9a325138c

méthode ou standard de détermination : SHA-1

Historique du fichier

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Date et heureVignetteDimensionsUtilisateurCommentaire
actuel22 août 2022 à 06:37Vignette pour la version du 22 août 2022 à 06:373 621 × 3 699 (4,29 Mio)wikimediacommons>Fabian RRRR== {{int:filedesc}} == {{Information |description={{en|1='''A Marvel of Galactic Morphology The galaxy featured in this Picture of the Week has a shape unlike many of the galaxies familiar to Hubble. Its thousands of bright stars evoke a spiral galaxy, but it lacks the characteristic ‘winding’ structure. The shining red blossoms stand out as well, twisted by clouds of dust — these are the locations of intense star formation. Yet it also radiates a diffuse glow, much like an elliptical galaxy...

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