In the Vinony graph
Vinony's link graph records 491 inbound references to Q291059, and connects out to list of stars in Hydra, Q1105445 and New General Catalogue.
It is catalogued under topics including Astronomical objects discovered in 1786, Barred lenticular galaxies and Discoveries by William Herschel.
Vinony links it to 32 Wikipedia language editions.
Key facts
- Constellation
- Hydra
- Right ascension
- 09 59 29.5
- Declination
- −22 ° 49 ′ 35 ″
- Redshift
- 0.007976 ± 0.000010
- Heliocentric radial velocity
- 2,391 ± 3 km / s
- Distance
- 83 Mly (25.3 Mpc )
- Type
- (R_1)SAB(r)0/a
- Apparent size v
- 2.1 ′ × 1.6 ′
- Notable features
- Seyfert galaxy
via Wikipedia infobox
Wikidata facts
- Distance from Earth
- 34.50
- Image
- NGC 3081-HST-R814-G555-B439.png
Show 9 more facts
- catalog code
- Gaia DR2 5660737587274519040
- Commons category
- NGC 3081
- time of discovery or invention
- 1786-12-21
- apparent magnitude
- 8.910
- right ascension
- 149.87309835235190
- declination
- -22.82631889481360
- redshift
- 0.0072
- radial velocity
- 2413
- galaxy morphological type
- S0:r
via Wikidata · CC0
~5 min read
Encyclopedic overview
NGC 3081 is a barred lenticular ring galaxy in the constellation of Hydra. NGC 3081 is located about 85 million light-years away from Earth, which means, given its apparent dimensions, that NGC 3081 is approximately 60,000 light-years across. It is a type II Seyfert galaxy, characterised by its bright nucleus. It was discovered by William Herschel on 21 December 1786.
NGC 3081 is seen nearly face-on. The galaxy's barred spiral centre is surrounded by a bright loop known as a resonance ring. This ring is full of bright clusters and bursts of new star formation, and frames the supermassive black hole thought to be lurking within NGC 3081—which glows brightly as it gobbles up infalling material.
Excerpted from Wikipedia’s “Q291059” article, available under the CC BY-SA 4.0 licence.
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