In the Vinony graph
Within Vinony's link graph, NGC 377 is referenced by 952 other articles, and connects out to list of NGC objects (1–1000), epoch and NGC 241.
It sits within the topics Astronomical objects discovered in 1885, Cetus and NGC objects.
Its subject is documented across 33 Wikipedia language editions.
Key facts
- Constellation
- Cetus
- Right ascension
- 01 06 34.8
- Declination
- −20 ° 19 ′ 57 ″
- Heliocentric radial velocity
- 16,051 km/s
- Type
- Sc
- Apparent size v
- 1.2' × 0.3'
via Wikipedia infobox
Wikidata facts
- Instance of
- spiral galaxy
- Constellation
- Cetus
- Image
- NGC 0377 DSS.jpg
Show 11 more facts
- catalog code
- APMBGC 541-014+029
- galaxy morphological type
- Sbc
- discoverer or inventor
- Francis Preserved Leavenworth
- time of discovery or invention
- 1886-00-00
- apparent magnitude
- 11.466
- redshift
- 0.053540
- right ascension
- 16.6462250
- declination
- -20.3322222
- radial velocity
- 16051
- epoch
- J2000.0
- Commons category
- NGC 377
Sources (2)
via Wikidata · CC0
~1 min read
Encyclopedic overview
NGC 377 is a spiral galaxy located in the constellation Cetus. It was discovered on October 15, 1885, by Francis Leavenworth. It was described by Dreyer as "very faint, very small, much extended, suddenly brighter middle and nucleus."
References
Excerpted from Wikipedia’s “NGC 377” article, available under the CC BY-SA 4.0 licence.