Galaxies · Constellation Virgo

Sombrero Galaxy (Messier 104 / NGC 4594)

Coordinates, TRGB distance (9.55 Mpc / 31.1 Mly), edge-on dust lane, 1-billion-M☉ central black hole, and observing guide for M104.

Right Ascension (J2000.0)12h 39m 59.43s
Declination (J2000.0)-11° 37′ 23.0″
Primary ClassificationUnbarred early-type spiral / lenticular-halo galaxy with edge-on dust ring
Best Observing SeasonSpring (April–June)

Provenance-Backed Scientific Measurements

Every measurement below preserves its unit, uncertainty interval, observational method, reference epoch, quality status, and primary catalog source. See Uncertainty & Provenance for how competing measurements are handled.

Astrometric, Photometric, and Physical Parameters for Sombrero Galaxy (Messier 104 / NGC 4594)
ParameterValueUncertaintyMethod & EpochQuality StatusSource Archive
Integrated visual magnitude (V)8 mag± 0.1 magIntegrated CCD aperture photometrydefinitiveRevised New General Catalogue and Index Catalogue (RNGC/IC)
Extragalactic distance9550000 pc± 310000 pcHST Tip of the Red Giant Branch (TRGB, McQuinn et al. 2016: 9.55 ± 0.31 Mpc / 31.1 Mly)definitiveSIMBAD Astronomical Database (CDS)
Apparent major axis8.7 arcmin± 0.3 arcminOptical isophotal dimensions (8.7′ × 3.5′)definitiveRevised New General Catalogue and Index Catalogue (RNGC/IC)
Heliocentric recession velocity1091 km/s± 5 km/sSlipher 1912 / modern optical absorption spectroscopydefinitiveSIMBAD Astronomical Database (CDS)
Measurement Uncertainties & Competing Solutions: HST TRGB measurements place M104 at 9.55 ± 0.31 Mpc (31.1 Mly), securely in the foreground south of the main 16.4 Mpc Virgo Cluster core.

J2000 Equatorial Sky Chart & Culmination Altitude

The chart below plots Sombrero Galaxy (Messier 104 / NGC 4594) at RA 12h 39m 59.43s, Dec -11° 37′ 23.0″ within Virgo, alongside peak meridian transit altitudes for 40°N and 30°S observers. Use the RA/Dec Coordinate Converter to compute exact culmination altitude for your latitude.

J2000 Equatorial Sky Position (Virgo) +90° 0° −90° 24h 12h RA 0h Peak Meridian Altitude 38° 40°N Lat 72° 30°S Lat RA: 12h 39m 59.43s Dec: -11° 37′ 23.0″ Epoch: J2000.0 · V = 8 mag First-party vector diagram derived from IAU / CDS SIMBAD / Gaia DR3 astrometry.

Astrophysical Context & Structure

The Sombrero Galaxy (Messier 104, NGC 4594) is a striking SA(s)a galaxy situated 9.55 ± 0.31 megaparsecs (31.1 million light-years) away on the southern border of Virgo and Corvus. Discovered by Pierre Méchain in May 1781 and handwritten by Charles Messier into his personal copy of the catalog (officially added as M104 by Camille Flammarion in 1921), M104 was the galaxy used by Vesto Slipher at Lowell Observatory in 1912–1914 to measure a +1,090 km/s Doppler redshift and rotational tilt—providing the first spectroscopic evidence of receding extragalactic systems.

Tilted just 6 degrees from edge-on, the Sombrero combines two distinct structural components: an enormous, nearly spherical stellar halo and bulge populated by ~2,000 globular clusters (resembling an elliptical galaxy), bisected by a razor-sharp, symmetric ring of cold molecular gas and dark interstellar dust.

In 2024 the James Webb Space Telescope's Mid-Infrared Instrument (MIRI) imaged M104 at 7.7 to 21 microns, causing the smooth optical stellar halo to vanish and revealing that the outer dust lane is actually a clumpy, bullseye-like ring surrounding a 1-billion-solar-mass low-luminosity active black hole.

Practical Visual Observing Guide

Minimum Instrument60–80 mm telescope (150 mm+ to clearly trace the dark equatorial dust lane)
Recommended Magnification100×–180×
Best Evening SeasonSpring (April–June)
  • Situated 11.5° west of Spica (α Virginis) and 5.5° northeast of Algorab (δ Corvi); star-hop through the telescopic asterisms nicknamed the 'Stargate' (STT 256) and 'Jaws' right to M104.
  • Because M104 has a high surface brightness (magnitude 8.0 packed into 8.7 × 3.5 arcminutes), its glowing spindle is visible in 10×50 binoculars and any 60 mm refractor.
  • In a 150–200 mm telescope at 120×–180×, the dark equatorial dust lane slicing just south of the blazing nucleus is unmistakable.

Catalog Cross-Identifications & Aliases

Common Aliases: M104 · NGC 4594

Cross-Catalog Identifiers for Sombrero Galaxy (Messier 104 / NGC 4594)
Catalog AuthorityIdentifier
MESSIERM 104
NGCNGC 4594
SIMBADM 104
WIKIDATAQ14359
Related Object · Ursa Major

Bode's Galaxy (Messier 81 / NGC 3031)

Coordinates, Cepheid/TRGB distance (3.63 Mpc / 11.8 Mly), magnitude 6.94, M81–M82 tidal pair, and observing guide for Bode's Galaxy in Ursa Major.

Related Object · Andromeda

Andromeda Galaxy (Messier 31 / NGC 224)

Coordinates, Cepheid/TRGB distance (765 kpc / 2.50 Mly), magnitude 3.44, blueshift (−300 km/s), and observing guide for Andromeda (M31).

Observing Guide

Spring Galaxy Season: Ursa Major to Virgo

Spring galaxy observing guide from Ursa Major (M81, M82, Whirlpool M51) across Coma/Virgo to giant elliptical M87, the Sombrero Galaxy (M104), and 3C 273.

Reference Guide

Proper Motion, Radial Velocity & Redshift

How astronomers combine tangential proper motion (mas/yr), Doppler radial velocity (km/s), and cosmological redshift (z) to reconstruct 3D space motion.

Catalog · NGC / IC

NGC & Caldwell Deep-Sky Cross-Walk Catalog

Cross-reference guide to Dreyer's New General Catalogue (NGC) showpieces, including southern gems Omega Centauri, 47 Tucanae, Carina Nebula, and the Veil.

Scientific Sources & Dataset Provenance

  • Revised New General Catalogue and Index Catalogue (RNGC/IC) (2024/2026 edition): Steinicke, W. 2010, Observing and Cataloguing Nebulae and Star Clusters (Cambridge Univ. Press); Verga, M. OpenNGC (CC-BY-SA 4.0 / data tables) — Wolfgang Steinicke / OpenNGC
  • JWST / MAST Science Archive & Mission Documentation (Cycle 1–4 Public Releases (2022–2026)): Rigby, J., et al. 2023, PASP, 135, 048001 (The Science Performance of JWST as Characterized in Commissioning) — NASA / ESA / CSA / STScI
  • SIMBAD Astronomical Database (CDS) (2026-10 release): Wenger, M., et al. 2000, A&AS, 143, 9 (The SIMBAD astronomical database) — Centre de Données astronomiques de Strasbourg