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]
Andromeda IX | |
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Observation data (J2000 epoch) | |
Constellation | Andromeda |
Right ascension | 00h 52m 53.0s[1] |
Declination | +43° 11′ 45″[1] |
Redshift | -216 ± ? km/s[1] |
Distance | 2.50 ± 0.08 Mly (766 ± 25 kpc)[2] |
Apparent magnitude (V) | 16.2 |
Characteristics | |
Type | dE[1] |
Notable features | Satellite galaxy M31 |
Other designations | |
And IX, PGC 4689222[3] |
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).
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Location | Andromeda Galaxy → Andromeda subgroup →
Local Group → Local Sheet → Virgo Supercluster → Laniakea Supercluster → KBC Void → Observable universe → Universe Each → may be read as "within" or "part of". | |
Satellite galaxies |
*It is uncertain whether these are companion galaxies of the Andromeda Galaxy | |
Catalogued stars | ||
Other |
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Constellation of Andromeda | |||||||||||
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Stars |
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Star clusters |
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Nebulae |
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Galaxies |
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