Article · Wikipedia archive · Last revised Jun 17, 2026

Andromeda IX

Andromeda IX is a dwarf spheroidal satellite of the Andromeda Galaxy. It was discovered in 2004 by resolved stellar photometry from the Sloan Digital Sky Survey (SDSS), by Zucker et al. (2004). At the time of its discovery, it was the galaxy with the lowest known surface brightness, ΣV ≃ 26.8mags arcsec−2 and the faintest galaxy known from its intrinsic absolute brightness.

Last revised
Jun 17, 2026
Read time
≈ 1 min
Length
275 w
Citations
9
Source
Andromeda IX
Observation data (J2000 epoch)
ConstellationAndromeda
Right ascension00h 52m 53.0s1
Declination+43° 11′ 45″1
Redshift-216 ± ? km/s1
Distance2.50 ± 0.08 Mly (766 ± 25 kpc)2
Apparent magnitude (V)16.2
Characteristics
TypedE1
Notable featuresSatellite galaxy
M31
Other designations
And IX, PGC 46892223

Andromeda IX (And 9) is a dwarf spheroidal satellite of the Andromeda Galaxy. It was discovered in 2004 by resolved stellar photometry from the Sloan Digital Sky Survey (SDSS), by Zucker et al. (2004).2 At the time of its discovery, it was the galaxy with the lowest known surface brightness, ΣV ≃ 26.8mags arcsec−2 and the faintest galaxy known from its intrinsic absolute brightness.2

It was found from data acquired within an SDSS scan along the major axis of M31, on October 5, 2002. Its distance was estimated to be almost exactly the same as that of M31 by McConnacrchie et al. (2005). Star formation history and dust production in Andromeda IX, as the closest satellite to M31, have also been investigated by Abdollahi et al. (2023).4

See also

See also

References

References

External links