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Arp 220

Luminous infrared galaxy in the constellation Serpens

Arp 220
A combination of James Webb Space Telescope and Hubble Space Telescope data showing a new view infrared galaxy Arp 220
Observation data (J2000 epoch)
Constellation	Serpens
Right ascension	15h34m 57.1s[1]
Declination	+23° 30′ 11″[1]
Redshift	0.01840 +/- 0.00002[1]
Heliocentric radial velocity	5434 ± 7 km/s[1]
Apparent magnitude (V)	13.9[1]
Characteristics
Type	S?[1]
Size	33.7 kpc (110,000 ly)
Apparent size (V)	1′.5 x 1′.2[1]
Other designations
IC 1127,[1] IC 4553,[1] UGC 9913,[1] PGC 55497[1]

Arp 220 is the result of a collision between two galaxies which are now in the process of merging. It is the 220th object in Halton Arp's Atlas of Peculiar Galaxies.

Arp 220 is the closest ultraluminous infrared galaxy (ULIRG) to Earth, at 250 million light years away. Its energy output was discovered by IRAS to be dominated by the far-infrared part of the spectrum.^[3] It is often regarded as the prototypical ULIRG and has been the subject of much study as a result. Most of its energy output is thought to be the result of a massive burst of star formation, or starburst, probably triggered by the merging of two smaller galaxies. Hubble Space Telescope observations of Arp 220 in 2002 and 1997, taken in visible light with the ACS, and in infrared light with NICMOS, revealed more than 200 huge star clusters in the central part of the galaxy. The most massive of these clusters contains enough material to equal about 10 million suns.^[4] X-ray observations by the Chandra and XMM-Newton satellites have shown that Arp 220 probably includes an active galactic nucleus (AGN) at its core, which raises interesting questions about the link between galaxy mergers and AGN, since it is believed that galactic mergers often trigger starbursts, and may also give rise to the supermassive black holes that appear to power AGN.

Luminous far-infrared objects like Arp 220 have been found in surprisingly large numbers by sky surveys of submillimetre wavelengths using instruments such as the Submillimetre Common-User Bolometer Array (SCUBA) at the James Clerk Maxwell Telescope (JCMT). Arp 220 and other relatively local ULIRGs are being studied as equivalents of this kind of object.

Astronomers from the Arecibo Observatory have detected organic molecules in the galaxy.^[5]

Arp 220 contains at least two bright maser sources, an OH megamaser, and a water maser.^[6] In October 2011, astronomers spotted a record-breaking seven supernova all found at the same time in Arp 220.^[7][8] The merging of the two galaxies started around 700 million years ago.^[9]

Recent observations^[10] from NASA's James Webb Space Telescope have provided further insight into Arp 220's remarkable characteristics. Capturing a stunning image of the galaxy, Webb's observations highlight Arp 220's status as the closest Ultraluminous Infrared Galaxy (ULIRG) to Earth, situated at a distance of 250 million light-years. Webb's imaging showcases the galaxy's intense luminosity in infrared light, revealing its status as a prototypical ULIRG dominated by far-infrared energy. The telescope's Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI) have unveiled intricate details of Arp 220's structure, including its core remnants separated by 1,200 light-years, rotating star-forming rings emitting dazzling infrared light, and faint tidal tails indicative of gravitational interactions. These observations underscore Arp 220's significance as a prime target for studying galaxy mergers, star formation, and the evolution of supermassive black holes at the centers of galaxies.

Wikimedia Commons has media related to Arp 220.

• "Hubble Sees Star Birth Gone Wild" (SpaceDaily) Jun 16, 2006
• Arp 220 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images