Maffei 2 is an intermediate spiral galaxy about 10 million light-years away[2] in the constellation Cassiopeia. Maffei 2 and Maffei 1 were both discovered by Paolo Maffei in 1968 from their infrared emission. Maffei 2 lies in the Zone of Avoidance and is about 99.5% obscured by the Milky Way's foreground dust clouds,[3] and as a result is barely detectable at optical wavelengths. It had been suggested soon after its discovery that Maffei 2 may be a member of the Local Group, but it is now thought to be a member of another nearby group, the IC 342/Maffei Group, the galaxy group that is the closest to the Local Group.

Maffei 2
Image by Two Micron All Sky Survey (2MASS)
Observation data (J2000 epoch)
Constellation	Cassiopeia
Right ascension	02h 41m 55.1s[1]
Declination	+59° 36′ 15″[1]
Redshift	-17 ± 5 km/s[1]
Distance	9.8 Mly[2]
Apparent magnitude (V)	16.0[1]
Characteristics
Type	SAB(rs)bc[1]
Apparent size (V)	15.2′ × 7.0′[1]
Other designations
UGCA 39,[1] PGC 10217,[1] Sharpless 197

Gallery

• 
  Near the bottom middle of this image, Maffei 2 is nearly obscured by the gas and dust in our own Galaxy

See also

• Dwingeloo 1
• NGC 1300

References

External links

Wikimedia Commons has media related to Maffei 2.

• "Maffei 2". Spider. SEDS.
• "Maffei 2". UA Astronomy. University of Alabama.
• Maffei 2 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
• Nemiroff, R.; Bonnell, J., eds. (9 March 2010). "Galaxies Beyond the Heart: Maffei 1 and 2". Astronomy Picture of the Day. NASA.
• "UGCA 39". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 25 March 2018.

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