File:NGC_7331_Acquired_with_the_Schulman_Telescope_at_the_Mount_Lemmon_SkyCenter.jpg · Wikimedia Commons · See Wikimedia Commons
Q671450
Sign in to saveAlso known as New General Catalogue 7331, C 30
spiral galaxy in the constellation Pegasus
In the Vinony graph
Vinony's link graph records 455 inbound references to Q671450, and connects out to list of NGC objects (7001–7840), Veil Nebula and epoch.
Vinony files it under Astronomical objects discovered in 1784, Caldwell objects and IRAS catalogue objects.
Vinony links it to 44 Wikipedia language editions.
Key facts
- Constellation
- Pegasus
- Right ascension
- 22 37 04.0624
- Declination
- +34 ° 24 ′ 56.72 ″
- Redshift
- 0.002 722 ± 0.000 003
- Heliocentric radial velocity
- 816 ± 1 km/s
- Galactocentric velocity
- 1,030 ± 9 km/s
- Distance
- 43.79 ± 8.800 Mly (13.427 ± 2.698 Mpc )
- Type
- SA(s)b; HII LINER
- Size
- 146,250 ly , (44.84 kpc ), ( diameter ; 25.0 B-mag arcsec ) , 112,920 ly × 55,316 ly, (34.62 kpc × 16.96 kpc), ( diameter ; "total" magnitude )
- Apparent size v
- 10.5 ′ × 3.7 ′
via Wikipedia infobox
Wikidata facts
- Distance from Earth
- 15.7
- Image
- NGC7331Visible.jpg
Show 9 more facts
- catalog code
- [VDD93] 245
- Commons category
- NGC 7331
- time of discovery or invention
- 1784-09-06
- apparent magnitude
- 9.614
- galaxy morphological type
- SAb
- redshift
- 0.002739
- right ascension
- 339.2670917
- declination
- 34.4159194
- radial velocity
- 794
Sources (2)
via Wikidata · CC0
~3 min read
Encyclopedic overview
NGC 7331, also known as Caldwell 30, is an unbarred spiral galaxy about 13.427 megaparsecs (43.79 million light-years) away in the constellation Pegasus. It was discovered by William Herschel on 6 September 1784.
The galaxy appears similar almost in size and structure to the Milky Way, and is sometimes referred to as "the Milky Way's twin". However, discoveries in the 2000s regarding the structure of the Milky Way may call this similarity into doubt, particularly because the latter is now believed to be a barred spiral, compared to the unbarred status of NGC 7331. In spiral galaxies the central bulge typically co-rotates with the disk but the bulge in the galaxy NGC 7331 is rotating in the opposite direction to the rest of the disk. In both visible light and infrared photos of the NGC 7331, the core of the galaxy appears to be slightly off-center, with one side of the disk appearing to extend further away from the core than the opposite side.
Excerpted from Wikipedia’s “Q671450” article, available under the CC BY-SA 4.0 licence.