NGC 4951
| Galaxie NGC 4951 | |
|---|---|
 | |
| AladinLite | |
| Sternbild | Jungfrau |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 13h 05m 07,7s [1] |
| Deklination | −06° 29′ 38″ [1] |
| Erscheinungsbild | |
| Morphologischer Typ | SAB(rs)cd:[1] |
| Helligkeit (visuell) | 12,0 mag[2] |
| Helligkeit (B-Band) | 12,7 mag[2] |
| Winkelausdehnung | 3,8′ × 1,6′[2] |
| Positionswinkel | 90°[2] |
| Flächenhelligkeit | 13,8 mag/arcmin²[2] |
| Physikalische Daten | |
| Zugehörigkeit | LGG 314[1] |
| Rotverschiebung | 0.003923 ± 0.000013[1] |
| Radialgeschwindigkeit | (1176 ± 4) km/s[1] |
| Hubbledistanz H0 = 73 km/(s • Mpc) | (49 ± 3) 𐄁 106 Lj (14,9 ± 1,0) Mpc [1] |
| Geschichte | |
| Entdeckung | Wilhelm Herschel |
| Entdeckungsdatum | 17. April 1784 |
| Katalogbezeichnungen | |
| NGC 4951 • PGC 45246 • MCG -01-33-081 • IRAS 13025-0613 • 2MASX J13050769-0629377 • GC 3390 • H II 188 • h 1523 • HIPASS J1305-06 • LDCE 904 NED296 | |
NGC 4951 ist eine Balken-Spiralgalaxie vom Hubble-Typ SBc im Sternbild Jungfrau auf der Ekliptik. Sie ist rund 49 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 65.000 Lichtjahren.
Im selben Himmelsareal befinden sich u. a. die Galaxien NGC 4941 und NGC 4981.
Das Objekt wurde am 17. April 1784 von Wilhelm Herschel[3] mit einem 18,7-Zoll-Spiegelteleskop entdeckt, der sie dabei mit „F, cL, E, r“[4] beschrieb.
(c) ESA/Hubble, CC BY 4.0Aufnahme des Hubble-Weltraumteleskops
Weblinks
- NGC 4951. SIMBAD, abgerufen am 22. Februar 2015 (englisch).
- NGC 4951. DSO Browser, abgerufen am 22. Februar 2015 (englisch).
- A maelstrom of matter and energy (engl.)
Einzelnachweise
Auf dieser Seite verwendete Medien
NGC 4951 legacy dr10.jpg
Autor/Urheber: Legacy Surveys / D.Lang (Perimeter Institute) & Meli thev, Lizenz: CC BY 4.0
NGC 4951 with Legacy Surveys DR10
Autor/Urheber: Legacy Surveys / D.Lang (Perimeter Institute) & Meli thev, Lizenz: CC BY 4.0
NGC 4951 with Legacy Surveys DR10
Image Credit: Legacy Surveys / D. Lang (Perimeter Institute), NERSC
Filters: g, r, z
Download website: https://portal.nersc.gov/cfs/cosmo/data/legacysurvey/dr10/south/coadd/196/1962m065/
Found via: https://www.legacysurvey.org/viewer?ra=196.2834&dec=-6.4949&layer=ls-dr10-grz&zoom=14&bricks&ngc
I created this image with FITS-Files with SAO Image DS9 & Photoshop Elements.jpg)
A maelstrom of matter and energy (potw2427a).jpg
(c) ESA/Hubble, CC BY 4.0
This Picture of the Week from the NASA/ESA Hubble Space Telescope depicts the galaxy NGC 4951, a spiral galaxy that’s located 49 million light-years from Earth in the constellation Virgo.The data used to make this image were captured by Hubble as part of a programme to examine how matter and energy travel in nearby galaxies. Galaxies continuously undergo a cycle of star formation whereby the gas in a galaxy forms molecular clouds, which collapse to create new stars, which then disperse the clouds they formed from with powerful radiation or stellar winds in a process called feedback. The remaining gas is left to form new clouds elsewhere. This cycle of moving matter and energy determines how fast a galaxy forms stars and how quickly it burns through its supplies of gas — that is, how it evolves over the course of its life. Understanding this evolution depends on the nebulae, stars and star clusters in the galaxy: when they formed and their past behaviour. Hubble has always excelled at measuring populations of stars, and the task of tracking gas and star formation in galaxies including NGC 4951 is no exception.NGC 4951 is also a Seyfert galaxy, a type of galaxy that has a very bright and energetic nucleus called an active galactic nucleus. This image demonstrates well how energetic the galaxy is, and some of the dynamic galactic activity which transports matter and energy throughout it: a shining core surrounded by swirling arms, glowing pink star-forming regions, and thick dust.[Image Description: A spiral galaxy, tilted diagonally. It has thick, cloudy spiral arms wrapping around the core. They are filled with pink patches marking new star formation, young blue stars, and dark wisps of dust that block light. The galaxy glows brightly from its core. It is on a dark background, with a few distant galaxies and unrelated stars around it.]
(c) ESA/Hubble, CC BY 4.0
This Picture of the Week from the NASA/ESA Hubble Space Telescope depicts the galaxy NGC 4951, a spiral galaxy that’s located 49 million light-years from Earth in the constellation Virgo.The data used to make this image were captured by Hubble as part of a programme to examine how matter and energy travel in nearby galaxies. Galaxies continuously undergo a cycle of star formation whereby the gas in a galaxy forms molecular clouds, which collapse to create new stars, which then disperse the clouds they formed from with powerful radiation or stellar winds in a process called feedback. The remaining gas is left to form new clouds elsewhere. This cycle of moving matter and energy determines how fast a galaxy forms stars and how quickly it burns through its supplies of gas — that is, how it evolves over the course of its life. Understanding this evolution depends on the nebulae, stars and star clusters in the galaxy: when they formed and their past behaviour. Hubble has always excelled at measuring populations of stars, and the task of tracking gas and star formation in galaxies including NGC 4951 is no exception.NGC 4951 is also a Seyfert galaxy, a type of galaxy that has a very bright and energetic nucleus called an active galactic nucleus. This image demonstrates well how energetic the galaxy is, and some of the dynamic galactic activity which transports matter and energy throughout it: a shining core surrounded by swirling arms, glowing pink star-forming regions, and thick dust.[Image Description: A spiral galaxy, tilted diagonally. It has thick, cloudy spiral arms wrapping around the core. They are filled with pink patches marking new star formation, young blue stars, and dark wisps of dust that block light. The galaxy glows brightly from its core. It is on a dark background, with a few distant galaxies and unrelated stars around it.]