NGC 4567 and NGC 4568

NGC 4567 and NGC 4568
The Butterfly Galaxies with NGC 4567 (top) and NGC 4568 (bottom)
Observation data (J2000.0 epoch)
Constellation	Virgo
Right ascension	12h 36m 34.3s
Declination	+11° 14′ 17″
Distance	62 Mly (19.1 Mpc)[1]
Apparent magnitude (V)	+10.9
Absolute magnitude (V)	-13.3
Characteristics
Type	SA(rs)bc / SA(rs)bc
Apparent size (V)	4.6′ × 2.1′
Notable features	colliding galaxies
Other designations
NGC 4567/8, UGC 7776/7, PGC 42064/9, VV 219,[2] KPG 347,[3] Butterfly Galaxies,[4] Siamese Twin Galaxies, Siamese Twins Galaxies, Siamese Twins[5][NB 1]

NGC 4567 and NGC 4568 (nicknamed the Butterfly Galaxies^[4] or Siamese Twins^{[NB 1][5]}) are a set of unbarred spiral galaxies about 60 million light-years away^[1] in the constellation Virgo. They were both discovered by William Herschel in 1784. They are part of the Virgo Cluster of galaxies.

These galaxies are in the process of colliding and merging with each other, as studies of their distributions of neutral and molecular hydrogen show, with the highest star-formation activity in the part where they overlap. However, the system is still in an early phase of interaction.^[6] In about 500 million years the galaxies will coalesce into a single elliptical galaxy.^[7]

Four supernovae have been observed in the Butterfly Galaxies: SN 1990B (type Ib, mag. 16),^[8] SN 2004cc (type Ic, mag. 17.5),^[9] SN 2020fqv (type IIb, mag. 19),^[10] and SN 2023ijd (type II, mag. 16.8).^[11]

Naming controversy

The two galaxies were nicknamed "Siamese Twins" because they appear to be connected. On August 5, 2020, NASA announced that they would not use that nickname in an effort to avoid systemic discrimination in their terminology.^[12][13]

See also

Wikimedia Commons has media related to NGC 4567.