NGC 5477
| Galaxie NGC 5477 | |
|---|---|
 | |
| Aufnahme des Hubble-Weltraumteleskops | |
| AladinLite | |
| Sternbild | Großer Bär |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 14h 05m 33,3s[1] |
| Deklination | +54° 27′ 40″[1] |
| Erscheinungsbild | |
| Morphologischer Typ | SA(s)m[1][2] |
| Helligkeit (visuell) | 13,7 mag[2] |
| Helligkeit (B-Band) | 14,3 mag[2] |
| Winkelausdehnung | 1′,6 × 1′,3[2] |
| Positionswinkel | 95°[2] |
| Flächenhelligkeit | 14,3 mag/arcmin²[2] |
| Physikalische Daten | |
| Zugehörigkeit | M 101-Gruppe LGG 371[1] |
| Rotverschiebung | 0.001014 ± 0.000017[1] |
| Radialgeschwindigkeit | 304 ± 5 km/s[1] |
| Hubbledistanz vrad / H0 | (19 ± 1) · 106 Lj (5,81 ± 0,42) Mpc [1] |
| Geschichte | |
| Entdeckung | Wilhelm Herschel |
| Entdeckungsdatum | 14. April 1789 |
| Katalogbezeichnungen | |
| NGC 5477 • UGC 9018 • PGC 50262 • CGCG 272-25 • MCG +09-23-034 • IRAS F14038+5441 • KUG 1403+546 • VV 561 • GC 3787 • H III 790 • DDO 186 | |
NGC 5477 ist eine irregulären Zwerggalaxie im Sternbild Großer Bär am Nordsternhimmel. Sie ist schätzungsweise 19 Millionen Lichtjahre vom Milchstraße entfernt und gehört zu einer Gruppe von Galaxien rund um Messier 101.
Das Objekt wurde am 14. April 1789 von dem deutsch-britischen Astronomen Wilhelm Herschel entdeckt.[3]
Weblinks
- astronews.com: Bild des Tages 7. Januar 2013
- Spektrum.de: Umgebungskarte
Einzelnachweise
Auf dieser Seite verwendete Medien
Autor/Urheber: Credit: ESA/Hubble & NASA, Lizenz: CC BY 3.0
An archetypal dwarf galaxy
The constellation of Ursa Major (The Great Bear) is home to Messier 101, the Pinwheel Galaxy. One of the biggest and brightest spiral galaxies in the night sky, Messier 101 is also the subject of one of Hubble's most famous images (heic0602). Like the Milky Way, Messier 101 is not alone, with smaller dwarf galaxies in its neighbourhood.
NGC 5477, one of these dwarf galaxies in the Messier 101 group, is the subject of this image from the NASA/ESA Hubble Space Telescope. Without obvious structure, but with visible signs of ongoing starbirth, NGC 5477 looks much like an archetypal dwarf irregular galaxy. The bright nebulae that extend across much of the galaxy are clouds of glowing hydrogen gas in which new stars are forming. These glow pinkish red in real life, although the selection of green and infrared filters through which this image was taken makes them appear almost white.
The observations were taken as part of a project to measure accurate distances to a range of galaxies within about 30 million light-years from Earth, by studying the brightness of red giant stars.
In addition to NGC 5477, the image includes numerous galaxies in the background, including some that are visible right through NGC 5477. This serves as a reminder that galaxies, far from being solid, opaque objects, are actually largely made up of the empty space between their stars.
This image is a combination of exposures taken through green and infrared filters using Hubble's Advanced Camera for Surveys. The field of view is approximately 3.3 by 3.3 arcminutes.
Credit: ESA/Hubble & NASA
About the Object
Name: NGC 5477
Type: • Local Universe : Galaxy : Type : Irregular
• Local Universe : Galaxy : Size : Dwarf
Distance: 20 million light years
Colours & filters Band Wavelength Telescope
Optical V 606 nm Hubble Space Telescope ACS Infrared I 814 nm Hubble Space Telescope ACS.
