Key facts
- Constellation
- Ursa Major
- Right ascension
- 09 50 22.2
- Declination
- +72 ° 16 ′ 43 ″
- Redshift
- 0.004410 ± 0.0000237
- Heliocentric radial velocity
- 1,322 ± 7 km / s
- Distance
- 70.1 ± 4.1 Mly (21.5 ± 1.3 Mpc )
- Type
- (R')SA(rs)ab
- Apparent size v
- 4.6 ′ × 3.6 ′
via Wikipedia infobox
Wikidata facts
- Distance from Earth
- 22.90
- Image
- NGC 2985 DSS.jpg
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- Commons category
- NGC 2985
- catalog code
- RX J095022+72162
- galaxy morphological type
- Sb
- time of discovery or invention
- 1785-00-00
- redshift
- 0.004306
- apparent magnitude
- 7.360
- right ascension
- 147.5926375
- declination
- 72.2786472
- radial velocity
- 1288
Sources (1)
via Wikidata · CC0
~2 min read
Article
NGC 2985 is a spiral galaxy located in the constellation Ursa Major. It is located at a distance of circa 70 million light years from Earth, which, given its apparent dimensions, means that NGC 2985 is about 95,000 light years across. It was discovered by William Herschel on April 3, 1785.
The galaxy is seen with an inclination of 37 degrees. The galaxy has a bright nucleus from which emanate multiple tightly wound spiral fragments. Numerous blue knots are visible at the galactic disk. At the outer part of the galaxy lies a massive spiral arm that forms a pseudoring that encircles the galaxy. The inner part of the galaxy, where active star formation has been observed, has been found to be unstable, contrary to the outer stable one. It has been suggested that the presence of molecular clouds accounts for the instability of the region.
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via Wikidata sitelinks · CC0