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Q695514

File:NGC1042-hst-R606GB450.jpg · Wikimedia Commons · See Wikimedia Commons

EntityQ695514· pop 39· linked from 718 articles

galaxy

Astronomical data · SIMBAD

Object type
SyG
Distance
101,291 light-years
Redshift
z = 0.0046
Morphology
SAB
Coordinates
RA 40.0999° · Dec -8.4335°
View on SIMBAD →

via SIMBAD · CDS Strasbourg

Key facts

Constellation
Cetus
Right ascension
02 40 24.0
Declination
−08 ° 26 ′ 01 ″
Redshift
0.004573 ± 0.000007
Heliocentric radial velocity
1,371 ± 2 km/s
Distance
55.5 Mly (17.02 Mpc )
Group or cluster
NGC 1052 group
Type
SAB(rs)cd
Size
39,200 ly
Apparent size v
2.3 ′ × 1.0 ′

via Wikipedia infobox

Wikidata facts

Distance from Earth
18.55
Image
NGC1042-hst-R606GB450.jpg
Show 12 more facts
redshift
0.00462
catalog code
LEDA 10122
time of discovery or invention
1885-11-10
Commons category
NGC 1042
apparent magnitude
8.848
galaxy morphological type
SABcd
right ascension
40.09988562369000
declination
-8.43354149858340
radial velocity
1376
parallax
0.1069
right ascension component of proper motion
0.771
declination component of proper motion
0.644
Sources (1)

via Wikidata · CC0

~2 min read

Article

NGC 1042 is a spiral galaxy located in the constellation Cetus. It was discovered on 10 November 1885 by American astronomer Lewis Swift. The galaxy has an apparent magnitude of 14.0.

NGC 1042 is a low-luminosity active galaxy. Furthermore, its luminosity class is III–IV and it has a broad HI line. It is known that NGC 1042 also hosts an intermediate-mass black hole in its center.

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