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EntityQ1044058· pop 30· linked from 38 articles

galaxy

Astronomical data · SIMBAD

Object type
Sy2
Redshift
z = 0.020504
Coordinates
RA 65.6784° · Dec -40.6010°
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via SIMBAD · CDS Strasbourg

Key facts

Constellation
Caelum
Right ascension
04 22 42.8080
Declination
−40 ° 36 ′ 03.037 ″
Redshift
0.020 384 ± 0.000 0330
Heliocentric radial velocity
6,111 ± 10 km/s
Distance
223.69 ± 9.42 Mly (68.583 ± 2.888 Mpc )
Type
(R')SB(s)a
Size
~221,400 ly (67.89 kpc ) (estimated)
Apparent size v
2.5′ × 1.2′

via Wikipedia infobox

Wikidata facts

Image
NGC 1572 imaged by Legacy Surveys.jpg
Show 9 more facts
catalog code
APMBGC 303-011+031
time of discovery or invention
1835-10-23
redshift
0.020291
galaxy morphological type
SBb
Commons category
NGC 1572
apparent magnitude
9.301
right ascension
65.6783917
declination
-40.6009722
radial velocity
6021
Sources (1)

via Wikidata · CC0

~1 min read

Article

NGC 1572 is a large barred spiral galaxy in the constellation of Caelum. Its velocity with respect to the cosmic microwave background is 6,081±10 km/s, which corresponds to a Hubble distance of 292.5 ± 20.5 Mly (89.68 ± 6.28 Mpc). However, six non-redshift measurements give a closer mean distance of 223.69 ± 9.42 Mly (68.583 ± 2.888 Mpc). It was discovered by British astronomer John Herschel on 23 October 1835.

NGC 1572 is a Seyfert II galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.

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