Messier 61 (NGC 4303)
J2000 coordinates, distance (52.5 Mly), magnitude 9.65, nuclear starburst ring, eight recorded supernovae, and observing guide for Messier 61.
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) | 9.65 mag | ± 0.1 mag | Integrated CCD aperture photometry | definitive | Revised New General Catalogue and Index Catalogue (RNGC/IC) |
| Distance in light-years | 52500000 ly | ± 3600000 ly | Type II-P supernova standardized candle & Tully-Fisher relation (16.1 ± 1.1 Mpc) | high-confidence | SIMBAD Astronomical Database (CDS) |
| Apparent major axis | 6.5 arcmin | ± 0.3 arcmin | Optical isophotal dimensions (6.5′ × 5.8′) | definitive | Revised New General Catalogue and Index Catalogue (RNGC/IC) |
| Heliocentric recession velocity | 1566 km/s | ± 3 km/s | H I 21-cm and optical H II region emission spectroscopy | definitive | SIMBAD Astronomical Database (CDS) |
J2000 Equatorial Sky Chart & Culmination Altitude
The chart below plots Messier 61 (NGC 4303 Supernova-Rich Spiral) at RA 12h 21m 54.90s, Dec +04° 28′ 25.6″ 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
Barnabus Oriani discovered Messier 61 (NGC 4303) on May 5, 1779, just six hours before Charles Messier spotted it on the same night—though Messier initially mistook the galaxy for the Comet of 1779 for two consecutive nights until he realized it had not moved! Situated 52.5 million light-years away in the southern extension of the Virgo Cluster, M61 is a nearly face-on SAB(rs)bc barred spiral galaxy measuring ~100,000 light-years across.
Unlike the gas-depleted spirals deeper inside the Virgo Cluster core, M61 retains rich reservoirs of cold molecular gas channeled along its central stellar bar into a dazzling 750-light-year-wide circumnuclear starburst ring. Inside that ring, young super-star clusters fewer than 4 million years old surround a ~5-million-solar-mass active black hole, while the outer spiral arms show sharp polygonal kinks caused by past tidal interactions with neighboring dwarf companions NGC 4292 and NGC 4303A.
Because of its furious star-formation rate, M61 is one of the most prolific supernova factories in the entire sky, having produced eight documented supernovae since 1926: SN 1926A, 1961I, 1964F, 1999gn, 2006ov, 2008in, 2014dt (a rare Type Iax event), and 2020jfo.
Practical Visual Observing Guide
- Located in southern Virgo, 1.3° north of the 5th-magnitude star 16 Virginis.
- In 80–120 mm telescopes at 50×–80×, M61 appears as a ghostly, nearly circular 6′ glow with a sharp, star-like central nucleus.
- Under dark Bortle 1–3 skies, a 250–350 mm (10–14 inch) reflector at 140×–180× resolves the short inner bar and two hooked spiral arms giving the galaxy a slightly square-shouldered outline.
Catalog Cross-Identifications & Aliases
Common Aliases: M61 · NGC 4303 · UGC 7420 · Swelling Spiral
| Catalog Authority | Identifier |
|---|---|
| MESSIER | M 61 |
| NGC | NGC 4303 |
| SIMBAD | M 61 |
| WIKIDATA | Q13982 |
Related Objects, Comparisons & Guides
Messier 49 (NGC 4472 Virgo Giant Elliptical)
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.
Mirror Galaxy (Messier 100 / NGC 4321)
J2000 coordinates, HST Cepheid distance (53.8 Mly), magnitude 9.35, grand-design spiral arms, five supernovae, and observing guide for Messier 100.
Fireworks Galaxy (NGC 6946 / Caldwell 12)
J2000 coordinates, TRGB distance (25.2 Mly), magnitude 9.60, ten recorded supernovae, BH1 direct-collapse candidate, and NGC 6946 observing guide.
Surface Brightness & Extended Objects Guide
Why surface brightness (mag/arcsec²) governs nebula and galaxy visibility more than integrated magnitude, and how exit pupil controls eyepiece contrast.
Bortle Dark-Sky Scale & Sky Brightness Guide
Reference guide to the 9-class Bortle Dark-Sky Scale, zenith Sky Quality Meter (SQM) readings in mag/arcsec², naked-eye limiting magnitude, and light pollution.
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
- 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