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EntityQ957278· pop 33· linked from 835 articles

galaxy

Key facts

Constellation
Sculptor
Right ascension
01 11 27.6390
Declination
−38 ° 05 ′ 00.452 ″
Heliocentric radial velocity
3,527 km/s
Distance
165.36 ± 24.14 Mly (50.700 ± 7.400 Mpc )
Type
Sa
Size
~134,600 ly (41.26 kpc ) (estimated)
Apparent size v
2.3′ × 0.8′

via Wikipedia infobox

~1 min read

Encyclopedic overview

NGC 424 is a spiral galaxy in the constellation of Sculptor. Its velocity with respect to the cosmic microwave background is 3,303±18 km/s, which corresponds to a Hubble distance of 158.9 ± 11.2 Mly (48.72 ± 3.42 Mpc). Also, two non-redshift measurements give a similar mean distance of 165.36 ± 24.14 Mly (50.700 ± 7.400 Mpc). It was discovered by British astronomer John Herschel on November 30, 1837.

NGC 424 is a Seyfert I 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.

Excerpted from Wikipedia’s “Q957278” article, available under the CC BY-SA 4.0 licence.