Galaxies · Constellation Virgo

Messier 49 (NGC 4472 / Arp 134)

J2000 coordinates, SBF distance (55.9 Mly), magnitude 8.40, globular cluster halo, X-ray bow shock, and observing guide for Messier 49 in Virgo.

Right Ascension (J2000.0)12h 29m 46.80s
Declination (J2000.0)+08° 00′ 01.5″
Primary ClassificationGiant E2/S0 elliptical galaxy (Virgo B subcluster dominant member)
Best Observing SeasonSpring (March–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 Messier 49 (NGC 4472 / Arp 134)
ParameterValueUncertaintyMethod & EpochQuality StatusSource Archive
Integrated visual magnitude (V)8.4 mag± 0.08 magWide-aperture CCD surface photometrydefinitiveRevised New General Catalogue and Index Catalogue (RNGC/IC)
Distance in light-years55900000 ly± 1900000 lyHST ACS Virgo Cluster Survey surface-brightness fluctuations (17.14 ± 0.58 Mpc)definitiveSH0ES Local Distance Ladder Hubble Constant
Apparent major axis10.2 arcmin± 0.5 arcminOptical isophotal dimensions (10.2′ × 8.3′)definitiveRevised New General Catalogue and Index Catalogue (RNGC/IC)
Heliocentric recession velocity981 km/s± 5 km/sOptical stellar absorption spectroscopydefinitiveSIMBAD Astronomical Database (CDS)
Measurement Uncertainties & Competing Solutions: Hubble Space Telescope ACS surface-brightness fluctuation (SBF) measurements fix M49's distance at 17.14 ± 0.58 Mpc (55.9 ± 1.9 Mly), placing its Virgo B southern subcluster roughly 0.7 Mpc behind the M87 Virgo A core.

J2000 Equatorial Sky Chart & Culmination Altitude

The chart below plots Messier 49 (NGC 4472 Virgo Giant Elliptical) at RA 12h 29m 46.80s, Dec +08° 00′ 01.5″ 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 58° 40°N Lat 52° 30°S Lat RA: 12h 29m 46.80s Dec: +08° 00′ 01.5″ Epoch: J2000.0 · V = 8.4 mag First-party vector diagram derived from IAU / CDS SIMBAD / Gaia DR3 astrometry.

Astrophysical Context & Structure

Found by Charles Messier on February 19, 1771, Messier 49 (NGC 4472) holds two historic distinctions: it was the very first member of the Virgo Galaxy Cluster ever discovered and the first elliptical galaxy outside the Local Group ever recorded. Shining at integrated magnitude 8.40 from a distance of 55.9 million light-years, M49 is optically the most luminous galaxy in the entire Virgo Cluster—slightly outshining even central Messier 87 in visual starlight—and anchors the dynamical center of the southern 'Virgo B' subcluster located 4.3 degrees south of M87.

Spanning more than 160,000 light-years across its stellar envelope, M49 hosts an estimated 5,900 globular clusters and a central supermassive black hole of roughly 2.5 billion solar masses. Chandra and XMM-Newton X-ray observations reveal a sharp thermodynamic bow shock along M49's northern edge, demonstrating that the entire galaxy and its surrounding halo of 10-million-kelvin gas are plunging northward into the main Virgo A intracluster medium at more than 1,000 kilometers per second.

Halton Arp cataloged M49 as Arp 134 because it is actively tidally shredding the gas-rich dwarf irregular galaxy UGC 7636 located 5.5 arcminutes to its southeast. Neutral hydrogen and optical debris stripped from UGC 7636 trail across the space between the two systems, where supernova SN 1969Q was also observed inside M49's outer halo.

Practical Visual Observing Guide

Minimum Instrument10×50 binoculars or 60 mm telescope
Recommended Magnification60×–150×
Best Evening SeasonSpring (March–June)
  • Located 4.1° west-southwest of Vindemiatrix (ε Virginis), forming the southern apex of the main Virgo realm of galaxies.
  • As the brightest galaxy in Virgo (V = 8.4), M49 is visible in 10×50 binoculars under dark skies and stands out immediately in a 60–80 mm refractor as a luminous, condensed circular glow.
  • In 200–250 mm telescopes at 100×–160×, M49 shows a brilliant core fading smoothly into an 8′×6′ oval halo, flanked within the same field by faint dwarf galaxies NGC 4465, NGC 4467, and NGC 4470.

Catalog Cross-Identifications & Aliases

Common Aliases: M49 · NGC 4472 · UGC 7629 · Arp 134

Cross-Catalog Identifiers for Messier 49 (NGC 4472 / Arp 134)
Catalog AuthorityIdentifier
MESSIERM 49
NGCNGC 4472
SIMBADM 49
WIKIDATAQ13951
Reference Guide

Apparent vs Absolute Magnitude Explained

Understand the logarithmic Pogson astronomical magnitude scale, apparent visual magnitude (m), absolute magnitude (M at 10 parsecs), and bolometric corrections.

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
  • SH0ES Local Distance Ladder Hubble Constant (2022 Baseline Cepheid + SN Ia): Riess, A. G., et al. 2022, ApJL, 934, L7 (A Comprehensive Measurement of the Local Value of the Hubble Constant) — SH0ES Collaboration (HST / JWST)
  • 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