| NGC 7582 | |
|---|---|
Hubble Space Telescope image of NGC 7582 | |
| Observation data ( J2000 epoch) | |
| Constellation | Grus |
| Right ascension | 23h 18m 23.5s [1] |
| Declination | −42° 22′ 14″ [1] |
| Redshift | 0.005254 [1] |
| Distance | 69.1 ± 6.719
Mly (21.2 ± 2.060 Mpc) [1] |
| Apparent magnitude (V) | 11.37 [1] |
| Characteristics | |
| Type | SB(s)ab [1] |
| Apparent size (V) | 5.0' × 2.1' [1] |
| Other designations | |
| 2MASX J23182362-4222140, MCG -07-47-029, PGC 071001 [1] | |
NGC 7582 is a
spiral galaxy of the
Hubble type SB(s)ab in the constellation
Grus. It has an angular size of 5.0' × 2.1' and an
apparent magnitude of 11.37. It is about 70 million
light years away from
Earth and has a diameter of about 100,000 light years. The galaxy is classified as a
Seyfert 2 galaxy, a type of
active galaxy. This galaxy is in the upper middle west part of the
Virgo Supercluster.
[1] The
supermassive black hole at the core has a mass of 5.5+2.6
−1.9×107
M☉.
[2]
Gallery
-
-
NGC 7582 by Hubble Space Telescope
References
- ^ a b c d e f g h i "NASA/IPAC Extragalactic Database". Results for NGC 7582. Retrieved January 7, 2017.
- ^ Graham, Alister W. (November 2008), "Populating the Galaxy Velocity Dispersion - Supermassive Black Hole Mass Diagram: A Catalogue of (Mbh, σ) Values", Publications of the Astronomical Society of Australia, 25 (4): 167–175, arXiv: 0807.2549, Bibcode: 2008PASA...25..167G, doi: 10.1071/AS08013, S2CID 89905.
External links
-
Media related to
NGC 7582 at Wikimedia Commons
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 | This spiral galaxy article is a stub. You can help Wikipedia by expanding it. |
| NGC 7582 | |
|---|---|
|
Hubble Space Telescope image of NGC 7582 | |
| Observation data ( J2000 epoch) | |
| Constellation | Grus |
| Right ascension | 23h 18m 23.5s [1] |
| Declination | −42° 22′ 14″ [1] |
| Redshift | 0.005254 [1] |
| Distance | 69.1 ± 6.719
Mly (21.2 ± 2.060 Mpc) [1] |
| Apparent magnitude (V) | 11.37 [1] |
| Characteristics | |
| Type | SB(s)ab [1] |
| Apparent size (V) | 5.0' × 2.1' [1] |
| Other designations | |
| 2MASX J23182362-4222140, MCG -07-47-029, PGC 071001 [1] | |
NGC 7582 is a
spiral galaxy of the
Hubble type SB(s)ab in the constellation
Grus. It has an angular size of 5.0' × 2.1' and an
apparent magnitude of 11.37. It is about 70 million
light years away from
Earth and has a diameter of about 100,000 light years. The galaxy is classified as a
Seyfert 2 galaxy, a type of
active galaxy. This galaxy is in the upper middle west part of the
Virgo Supercluster.
[1] The
supermassive black hole at the core has a mass of 5.5+2.6
−1.9×107
M☉.
[2]
Gallery
-
-
NGC 7582 by Hubble Space Telescope
References
- ^ a b c d e f g h i "NASA/IPAC Extragalactic Database". Results for NGC 7582. Retrieved January 7, 2017.
- ^ Graham, Alister W. (November 2008), "Populating the Galaxy Velocity Dispersion - Supermassive Black Hole Mass Diagram: A Catalogue of (Mbh, σ) Values", Publications of the Astronomical Society of Australia, 25 (4): 167–175, arXiv: 0807.2549, Bibcode: 2008PASA...25..167G, doi: 10.1071/AS08013, S2CID 89905.
External links
-
Media related to
NGC 7582 at Wikimedia Commons
| Stars |
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|---|---|---|---|---|---|---|---|---|---|---|---|
| |||||||||||
| Galaxies |
| ||||||||||
| |||||||||||
|
| This spiral galaxy article is a stub. You can help Wikipedia by expanding it. |