Sombrero Galaxy

The Sombrero Galaxy (also known as Messier Object 104, M104 or NGC 4594) is a peculiar galaxy of unclear classification in the constellation borders of Virgo and Corvus, being about 9.55 megaparsecs (31.1 million light-years) from the Milky Way galaxy. It is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster. It has an isophotal diameter of approximately 29.09 to 32.32 kiloparsecs (94,900 to 105,000 light-years), making it slightly bigger in size than the Milky Way.

Sombrero Galaxy
Image taken by Hubble Space Telescope, May−June 2003
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension12h 39m 59.4s
Declination−11° 37 23
Redshift0.003416±0.000017
Heliocentric radial velocity1,024±5 km/s
Galactocentric velocity904±7 km/s
Distance9.55 ± 0.31 Mpc
(31.1 ± 1.0 Mly)
Apparent magnitude (V)8.0
Absolute magnitude (B)−21.8
Characteristics
TypeSA(s)a or E
Size32.32 kpc × 17.45 kpc
(105.4 kly × 56.91 kly)
(diameter; 2MASS K-band total isophote)
29.09 kpc (94.88 kly)
(diameter; D25.0 B-band isophote)
Apparent size (V)9 × 4
Notable featuresUnusually bright center, intriguingly detailed dust band
Other designations
M104, NGC 4594, UGC 293, PGC 42407

It has a bright nucleus, an unusually large central bulge, and a prominent dust lane in its outer disk, which is viewed almost edge-on. The dark dust lane and the bulge give it the appearance of a sombrero hat (thus the name). Astronomers initially thought the halo was small and light, indicative of a spiral galaxy; but the Spitzer Space Telescope found that the dust ring was larger and more massive than previously thought, indicative of a giant elliptical galaxy.

The galaxy has an apparent magnitude of +8.0, making it easily visible with amateur telescopes, and is considered by some authors to be the galaxy with the highest absolute magnitude within a radius of 10 megaparsecs of the Milky Way. Its large bulge, central supermassive black hole, and dust lane all attract the attention of professional astronomers.

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