Astronomy:NGC 52

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Short description: Edge-on Spiral galaxy in the constellation of Pegasus
NGC 52
NGC 52 SDSS
NGC 52 and nearby PGC 1563523 (lower right) as seen on legacy survey
Observation data (2000.0 epoch)
ConstellationPegasus
Right ascension 00h 14m 40.2s [1]
Declination+18° 34′ 48″ [1]
Redshift0.017986
Helio radial velocity5390 km/s
Distance243,000,000ly[2] (73,000,000 Parsecs)[3]
Apparent magnitude (V)14.6 [4]
Characteristics
TypeSc [2]
Size150,000[2]
Apparent size (V)2.6' × 0.5' [1]
Other designations
UGC 140, CGCG 456-042, CGCG 12.0+1817, MCG+03-01-030, 2MFGC 00177, 2MASX J00144010+1834551, 2MASXi J0014401+183455, IRAS 00120+1818, IRAS F00120+1818, AKARI J0014401+183453, LDCE 0011 NED002, PGC 978, UZC J001440.2+183454, NVSS J001440+183455 [5]

NGC 52 (PGC 978) is an edge-on spiral galaxy in the constellation Pegasus. It was discovered on September 18, 1784, by William Herschel. He described it as "very faint, small, extended."[2]

Physical characteristics

The galaxy is approximately 150,000 light years across.[2] This makes it, in comparison, about 1.5 times as large as the Milky Way. The galaxy also has a satellite elliptical galaxy called PGC (Principal Galaxies Catalogue) 1563523.

See also

NGC 52 (2MASS)

References

External links

Coordinates: Sky map 00h 14m 40.2s, +18° 34′ 48″