Messier 86 (NGC 4406)
J2000 coordinates, SBF distance (55.4 Mly), magnitude 8.90, −244 km/s blueshift, ram-pressure X-ray plume, and observing guide for Messier 86 in Virgo.
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.
| Parameter | Value | Uncertainty | Method & Epoch | Quality Status | Source Archive |
|---|---|---|---|---|---|
| Integrated visual magnitude (V) | 8.9 mag | ± 0.08 mag | Integrated CCD aperture photometry | definitive | Revised New General Catalogue and Index Catalogue (RNGC/IC) |
| Distance in light-years | 55400000 ly | ± 1800000 ly | HST ACS Virgo Cluster Survey surface-brightness fluctuations (17.0 ± 0.55 Mpc) | definitive | SH0ES Local Distance Ladder Hubble Constant |
| Apparent major axis | 8.9 arcmin | ± 0.4 arcmin | Optical isophotal dimensions (8.9′ × 5.8′) | definitive | Revised New General Catalogue and Index Catalogue (RNGC/IC) |
| Heliocentric radial velocity | -244 km/s | ± 5 km/s | Optical absorption spectroscopy (highest blueshift of any Messier galaxy after M31) | definitive | SIMBAD Astronomical Database (CDS) |
J2000 Equatorial Sky Chart & Culmination Altitude
The chart below plots Messier 86 (NGC 4406 Blueshifted Lenticular) at RA 12h 26m 11.74s, Dec +12° 56′ 45.5″ 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.
Astrophysical Context & Structure
Discovered by Charles Messier on March 18, 1781, right alongside its neighbor M84 just 17 arcminutes to the west, Messier 86 (NGC 4406) is a giant E3 elliptical or lenticular galaxy dominating the western head of Markarian's Chain from a distance of 55.4 million light-years. Spanning roughly 140,000 light-years across and surrounded by ~3,800 globular clusters, M86 is slightly larger and 0.2 magnitudes brighter than M84.
Spectroscopically, M86 is one of the most extreme objects in the local universe: even though it resides 55.4 million light-years away inside the receding Virgo Cluster (whose average recession velocity is +1,100 km/s), M86 displays a heliocentric blueshift of −244 km/s! Dynamically accelerated by the immense gravitational well of the Virgo Cluster, M86 is plunging from the far side of the cluster almost directly toward the Milky Way at an astonishing relative velocity of ~1,350 km/s.
As M86 screams supersonically through the Virgo intracluster medium, intense ram pressure strips a 380,000-light-year-long tail of superheated X-ray gas behind the galaxy (mapped by Chandra and XMM-Newton), while H-alpha filaments also link M86 to the tidally disturbed spiral NGC 4438 ('The Eyes') 23 arcminutes to its east.
Practical Visual Observing Guide
- Paired with M84 (17′ WSW) at the heart of the Virgo Cluster; in any telescope at 40×–70×, M86 is the larger, slightly more oval eastern member of the pair.
- A 150–250 mm telescope frames M86 and M84 with edge-on spirals NGC 4402 (just 10′ north of M86) and NGC 4388 (15′ south) plus the interacting pair NGC 4435/4438 ('The Eyes') 23′ east.
Catalog Cross-Identifications & Aliases
Common Aliases: M86 · NGC 4406 · UGC 7532 · PGC 40653
| Catalog Authority | Identifier |
|---|---|
| MESSIER | M 86 |
| NGC | NGC 4406 |
| SIMBAD | M 86 |
| WIKIDATA | Q14036 |
Related Objects, Comparisons & Guides
Messier 84 (NGC 4374 Markarian Chain Core)
J2000 coordinates, SBF distance (54.8 Mly), magnitude 9.10, western Markarian's Chain anchor, twin radio jets, and observing guide for Messier 84.
Messier 87 (Virgo A Giant Elliptical Galaxy)
Coordinates, distance (16.4 Mpc / 53.5 Mly), EHT 6.5-billion M☉ black hole M87*, relativistic jet, and observing guide for Messier 87.
Messier 90 (NGC 4569 Ram-Stripped Spiral)
J2000 coordinates, distance (53.8 Mly), magnitude 9.52, −235 km/s blueshift, truncated H II disk, IC 3583 companion, and observing guide for Messier 90.
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.
Angular Size, Separation & Field of View
How angular diameter (degrees, arcminutes, arcseconds), spherical angular separation, and small-angle physical diameter relate to telescope field of view.
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