In the Vinony graph
Within Vinony's link graph, NGC 1819 is referenced by 480 other articles, and connects out to list of stars in Orion, list of NGC objects (1001–2000) and NGC 1854.
It sits within the topics Astronomical objects discovered in 1885, Discoveries by Lewis Swift and IRAS catalogue objects.
Its subject is documented across 29 Wikipedia language editions.
Astronomical data · SIMBAD
- Object type
- GiC
- Redshift
- z = 0.01488
- Morphology
- SO
- Coordinates
- RA 77.9423° · Dec 5.2006°
via SIMBAD · CDS Strasbourg
Key facts
- Constellation
- Orion
- Right ascension
- 05 11 46.150
- Declination
- +05 ° 12 ′ 02.21 ″
- Redshift
- 0.014880 ± 0.000047
- Heliocentric radial velocity
- 4,483 km/s
- Distance
- 197.4 Mly (60.53 Mpc )
- Surface brightness
- 23.34 mag/arcsec2
- Type
- SB0
via Wikipedia infobox
Wikidata facts
- Instance of
- lenticular galaxy
- Constellation
- Orion
- Distance from Earth
- 60.53
- Image
- NGC 1819 DSS.jpg
Show 11 more facts
- redshift
- 0.014880
- catalog code
- LEDA 16899
- discoverer or inventor
- Lewis A. Swift
- time of discovery or invention
- 1885-12-26
- apparent magnitude
- 9.227
- galaxy morphological type
- SB0
- right ascension
- 77.9422917
- declination
- 5.2006139
- radial velocity
- 4428
- epoch
- J2000.0
- Commons category
- NGC 1819
Sources (1)
via Wikidata · CC0
~1 min read
Encyclopedic overview
NGC 1819 is a lenticular galaxy in the constellation of Orion. It was discovered on December 26, 1885, by American astronomer Lewis A. Swift. This galaxy is located at a distance of 197.4 million light-years (60.53 Mpc) from the Milky Way, and is receding with a heliocentric radial velocity of 4,483 km/s.
The morphological classification of NGC 1819 is SB0 in the De Vaucouleurs system, indicating this is a lenticular galaxy with a barred spiral organization. It is a gas-rich galaxy with a circumnuclear ring structure that is undergoing intense star formation.
Excerpted from Wikipedia’s “NGC 1819” article, available under the CC BY-SA 4.0 licence.
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