Southern Pinwheel Galaxy (Messier 83 / NGC 5236)
J2000 coordinates, Cepheid/TRGB distance (15.2 Mly), magnitude 7.54, barred spiral starburst core, six supernovae, and observing guide for Messier 83.
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) | 7.54 mag | ± 0.06 mag | Wide-field integrated CCD photometry | definitive | Revised New General Catalogue and Index Catalogue (RNGC/IC) |
| Distance in light-years | 15200000 ly | ± 500000 ly | VLT Cepheids + HST Tip of the Red Giant Branch (4.66 ± 0.15 Mpc) | definitive | SH0ES Local Distance Ladder Hubble Constant |
| Apparent major axis | 12.9 arcmin | ± 0.5 arcmin | Optical isophotal dimensions (12.9′ × 11.5′) | definitive | Revised New General Catalogue and Index Catalogue (RNGC/IC) |
| Heliocentric recession velocity | 513 km/s | ± 2 km/s | H I 21-cm synthesis velocity field | definitive | SIMBAD Astronomical Database (CDS) |
J2000 Equatorial Sky Chart & Culmination Altitude
The chart below plots Southern Pinwheel (Messier 83 / NGC 5236) at RA 13h 37m 00.91s, Dec -29° 51′ 56.7″ within Hydra, 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
Nicolas-Louis de Lacaille discovered Messier 83 (NGC 5236), the Southern Pinwheel Galaxy, on February 23, 1752, from the Cape of Good Hope, making it the first galaxy outside the Local Group ever identified by humanity. Added to Messier's catalog in March 1781, M83 lies just 15.2 million light-years away on the southern Hydra–Centaurus border, where it anchors the northern sub-group of the nearby Centaurus A / M83 galaxy complex.
Measuring ~55,000 light-years across and viewed almost face-on, M83 is one of the brightest and closest barred spiral galaxies in the sky (V = 7.54). Hubble Wide Field Camera 3 and Chandra X-ray panoramas of M83 resolve thousands of young stellar clusters, crimson H-alpha emission nebulae, and nearly 300 supernova remnants threading its dusty spiral arms, along with a double nuclear structure driven by gas inflows along its prominent central stellar bar.
Over the past century M83 has produced six observed supernovae—SN 1923A, 1945B, 1950B, 1957D, 1968L, and 1983N (the prototype of stripped-envelope Type Ib core-collapse supernovae)—placing it among the top supernova-producing galaxies known.
Practical Visual Observing Guide
- Located 18° south of Spica on the Hydra–Centaurus border; at declination −29° 52′, it climbs only ~20°–30° above the southern horizon from mid-northern latitudes but passes near the zenith from the Southern Hemisphere.
- Easily visible in 7×50 or 10×50 binoculars as a round 10′ glow with a bright center.
- In a 200–300 mm telescope at 80×–140× under steady dark skies, M83 is one of the very few galaxies where visual observers can clearly trace a bright northeast-southwest central bar transitioning directly into two sweeping S-shaped spiral arms.
Catalog Cross-Identifications & Aliases
Common Aliases: M83 · NGC 5236 · UGCA 366 · Southern Pinwheel Galaxy
| Catalog Authority | Identifier |
|---|---|
| MESSIER | M 83 |
| NGC | NGC 5236 |
| SIMBAD | M 83 |
| WIKIDATA | Q14030 |
Related Objects, Comparisons & Guides
Centaurus A (NGC 5128 Active Radio Galaxy)
J2000 coordinates, TRGB/Cepheid distance (12.4 Mly), magnitude 6.84, warped dust lane, relativistic radio lobes, and observing guide for Centaurus A.
Pinwheel Galaxy (Messier 101 / NGC 5457)
J2000 coordinates, Cepheid/TRGB distance (21.6 Mly), magnitude 7.86, giant H II regions, SN 2011fe & SN 2023ixf, and observing guide for M101.
Whirlpool Galaxy (Messier 51 / NGC 5194)
Coordinates, SN II-P / TRGB distance (8.58 Mpc / 28.0 Mly), grand-design spiral arms, NGC 5195 tidal companion, and observing guide for M51.
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.
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