Galaxies · Constellation Virgo

Messier 87 (Virgo A / NGC 4486)

Coordinates, distance (16.4 Mpc / 53.5 Mly), EHT 6.5-billion M☉ black hole M87*, relativistic jet, and observing guide for Messier 87.

Right Ascension (J2000.0)12h 30m 49.42s
Declination (J2000.0)+12° 23′ 28.0″
Primary ClassificationSupergiant cD elliptical galaxy & active galactic nucleus (Virgo Cluster center)
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 87 (Virgo A / NGC 4486)
ParameterValueUncertaintyMethod & EpochQuality StatusSource Archive
Integrated visual magnitude (V)8.6 mag± 0.1 magIntegrated CCD aperture photometrydefinitiveRevised New General Catalogue and Index Catalogue (RNGC/IC)
Extragalactic distance16400000 pc± 500000 pcSurface-brightness fluctuations (SBF) & TRGB (16.4 ± 0.5 Mpc / 53.5 Mly)definitiveEvent Horizon Telescope Collaboration Horizon-Scale Results
Central black hole mass (M87*)
EHT horizon-scale imaging (6.5 ± 0.9 × 10^9 M☉) agrees closely with stellar-dynamical orbit modeling (~6.1 × 10^9 M☉), whereas earlier ionized-gas-disk kinematics yielded ~3.5 × 10^9 M☉ due to non-gravitational gas turbulence.
6500000000 M☉± 900000000 M☉Event Horizon Telescope 1.3-mm VLBI photon-ring diameter (42 ± 3 μas)definitiveEvent Horizon Telescope Collaboration Horizon-Scale Results
Heliocentric recession velocity1284 km/s± 5 km/sOptical stellar absorption spectroscopy (z = 0.00428)definitiveSIMBAD Astronomical Database (CDS)
Measurement Uncertainties & Competing Solutions: For two decades M87*'s black hole mass differed by nearly a factor of two between gas-kinematic models (~3.5 × 10^9 M☉) and stellar-dynamical models (~6.2 × 10^9 M☉); the Event Horizon Telescope's 42-microarcsecond shadow measurement decisively confirmed the high stellar-dynamical mass (6.5 ± 0.9 × 10^9 M☉).

J2000 Equatorial Sky Chart & Culmination Altitude

The chart below plots Messier 87 (Virgo A Giant Elliptical Galaxy) at RA 12h 30m 49.42s, Dec +12° 23′ 28.0″ 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 62° 40°N Lat 48° 30°S Lat RA: 12h 30m 49.42s Dec: +12° 23′ 28.0″ Epoch: J2000.0 · V = 8.6 mag First-party vector diagram derived from IAU / CDS SIMBAD / Gaia DR3 astrometry.

Astrophysical Context & Structure

Messier 87 (Virgo A, NGC 4486) is the colossal central cD supergiant elliptical galaxy dominating the dynamical heart of the Virgo Galaxy Cluster, situated 16.4 ± 0.5 megaparsecs (53.5 million light-years) from Earth. Assembled over billions of years through hierarchical mergers of smaller galaxies, M87 has a total mass inside its outer halo exceeding 2.4 trillion solar masses and is surrounded by an extraordinary swarm of roughly 12,000 to 15,000 globular clusters—compared to only ~150–200 globular clusters around our Milky Way.

On April 10, 2019, the Event Horizon Telescope (EHT) Collaboration unveiled the first direct image of a black hole in human history by linking millimeter-wavelength radio telescopes across the globe to resolve M87*, the supermassive black hole at M87's core. Weighing 6.5 ± 0.9 billion solar masses (with a Schwarzschild event horizon ~38 billion kilometers across—three times the diameter of Pluto's orbit), M87* casts a 42-microarcsecond dark shadow surrounded by an asymmetric ring of relativistic synchrotron plasma.

Powered by the black hole's spin and magnetic fields (the Blandford-Znajek mechanism), M87* launches a collimated relativistic plasma jet discovered optically by Heber Curtis at Lick Observatory in 1918—a blue synchrotron beam extending 1,500 parsecs (~4,900 light-years) from the nucleus at position angle 290°.

Practical Visual Observing Guide

Minimum Instrument60–80 mm telescope (10×50 binoculars under dark skies)
Recommended Magnification60×–150× (350×+ in 450 mm+ scope to attempt the optical jet)
Best Evening SeasonSpring (March–June)
  • Located midway between Denebola (β Leonis) and Vindemiatrix (ε Virginis) at the southeastern anchor of Markarian's Chain in the Virgo Cluster.
  • At magnitude 8.6 with a bright, concentrated core, M87 is one of the easiest Virgo galaxies to spot in a 60–100 mm telescope at 50×–100×, appearing as a round, bright, slightly oval ball with a stellar-like nucleus.
  • Visual detection of M87's 20-arcsecond optical relativistic jet (integrated mag ~15.0) is a famous bucket-list challenge for experienced observers using 450–600 mm (18–24 inch) apertures at 350×–500× under sub-arcsecond seeing.

Catalog Cross-Identifications & Aliases

Common Aliases: M87 · Virgo A · NGC 4486 · 3C 274 · M87*

Cross-Catalog Identifiers for Messier 87 (Virgo A / NGC 4486)
Catalog AuthorityIdentifier
MESSIERM 87
NGCNGC 4486
SIMBADM 87
WIKIDATAQ14041
Related Object · Sagittarius

Sagittarius A* (Galactic Center Black Hole)

Coordinates, GRAVITY S2 stellar orbit distance (8,277 pc) & mass (4.297 × 10^6 M☉), EHT 51.8 μas shadow, and Galactic Center guide for Sgr A*.

Related Object · Virgo

3C 273 (Brightest Quasar in Virgo)

Coordinates, redshift z = 0.1583 (~2.4 billion ly), magnitude 12.85, supermassive black hole accretion, and observing guide for quasar 3C 273.

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

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.

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

  • Event Horizon Telescope Collaboration Horizon-Scale Results (2019 ApJL 875 L1 & 2022 ApJL 930 L12): Event Horizon Telescope Collaboration 2019, ApJL, 875, L1; 2022, ApJL, 930, L12 — Event Horizon Telescope Collaboration
  • 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
  • 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