File:NGC_128_Mount_Lemmon_Sky_Center.jpg · Wikimedia Commons · See Wikimedia Commons
NGC 127
Sign in to saveAlso known as New General Catalogue 127, UGC 292
lenticular galaxy in the constellation Pisces
Key facts
- Constellation
- Pisces
- Right ascension
- 00 29 12.396
- Declination
- +02 ° 52 ′ 21.24 ″
- Heliocentric radial velocity
- 4,061 ± 15 km/s
- Distance
- 190 Mly (57 Mpc ) h , 0.73
- Group or cluster
- NGC 128
- Type
- Sa
- Apparent size v
- 0.8′ x 0.6′
via Wikipedia infobox
Wikidata facts
- Instance of
- lenticular galaxy
- Constellation
- Pisces
- Image
- NGC 0127 SDSS.jpg
Show 11 more facts
- catalog code
- Gaia DR2 2547812193837647872
- radial velocity
- 4050
- discoverer or inventor
- William Parsons, 3rd Earl of Rosse
- time of discovery or invention
- 1850-11-04
- apparent magnitude
- 13.437
- galaxy morphological type
- S...
- Commons category
- NGC 127
- redshift
- 0.013509
- right ascension
- 7.30165119071980
- declination
- 2.87256704937590
- epoch
- J2000.0
Sources (1)
via Wikidata · CC0
~1 min read
Encyclopedic overview
NGC 127 is a lenticular galaxy that was discovered on November 4, 1850, by Bindon Stoney, the same day he discovered NGC 126 and NGC 130. NGC 127 is a gas-rich, star-forming galaxy showing emission lines. It is an interacting companion to the peculiar, edge-on galaxy NGC 128, and the pair are connected by a bridge of material. The south-east part of NGC 127 is asymmetrical in the direction of NGC 128. It may have recently passed the more massive NGC 128, from which an infall of gas is flowing onto NGC 127.
References
Excerpted from Wikipedia’s “NGC 127” article, available under the CC BY-SA 4.0 licence.