Astronomical data · SIMBAD
- Object type
- GiC
- Redshift
- z = 0.003344569634776473
- Morphology
- SA
- Coordinates
- RA 175.2448° · Dec 11.4711°
via SIMBAD · CDS Strasbourg
Key facts
- Constellation
- Leo
- Right ascension
- 11 40 58.7659
- Declination
- +11 ° 28 ′ 16.371 ″
- Heliocentric radial velocity
- 992 ± 1 km/s
- Distance
- 51.2 ± 10.6 Mly (15.7 ± 3.2 Mpc )
- Type
- SA(rs)c
- Size
- ~64,200 ly (19.67 kpc ) (estimated)
- Apparent size v
- 4.3 ′ × 3.0 ′
via Wikipedia infobox
Wikidata facts
- Instance of
- spiral galaxy
- Constellation
- Leo
- Distance from Earth
- 15
- Image
- The difference between distance and dust (potw2428a).jpg
Show 11 more facts
- catalog code
- [NKB95] N3810
- Commons category
- NGC 3810
- discoverer or inventor
- William Herschel
- time of discovery or invention
- 1784-03-15
- apparent magnitude
- 10.298
- galaxy morphological type
- SAc
- right ascension
- 175.2447375
- declination
- 11.4711306
- redshift
- 0.00333
- radial velocity
- 988
- epoch
- J2000.0
via Wikidata · CC0
~2 min read
Encyclopedic overview
NGC 3810 is a spiral galaxy located in the constellation Leo. It is about 50 million light years from Earth, and estimated to be about 60,000 light years in diameter. William Herschel discovered it on 15 March 1784.
The bright galaxy NGC 3810 demonstrates spiral structure similar to that of Messier 77. The central part of the galaxy disk is of high surface brightness and features tightly wound spirals. Outside this disk lie more open arms with lower surface brightness. The bright central region is thought to be forming many new stars and is outshining the outer areas of the galaxy by some margin. Further out, the galaxy displays strikingly rich dust clouds along its spiral arms. Hot young blue stars show up in giant clusters far from the centre and the arms are also littered with bright red giant stars.
Excerpted from Wikipedia’s “NGC 3810” article, available under the CC BY-SA 4.0 licence.
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