Messier 23 (NGC 6494)
Coordinates, Gaia DR3 distance (728 pc), magnitude 5.5, foreground Sagittarius dust lane geometry, and observing guide for M23.
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) | 5.5 mag | ± 0.1 mag | Wide-aperture integrated photometry | definitive | Revised New General Catalogue and Index Catalogue (RNGC/IC) |
| Heliocentric distance | 2375 ly | ± 35 ly | Gaia DR3 astrometric parallax of cluster members (728 ± 11 pc) (J2016.0) | definitive | ESA Gaia Archive — Data Release 3 |
| Apparent diameter | 27 arcmin | ± 2 arcmin | Member star-count boundary | high-confidence | Revised New General Catalogue and Index Catalogue (RNGC/IC) |
| Main-sequence turnoff age | 0.33 Gyr | ± 0.04 Gyr | Gaia DR3 color-magnitude diagram isochrone fitting | high-confidence | ESA Gaia Archive — Data Release 3 |
J2000 Equatorial Sky Chart & Culmination Altitude
The chart below plots Messier 23 (NGC 6494 Sagittarius Cluster) at RA 17h 57m 04.00s, Dec -18° 59′ 06.0″ within Sagittarius, 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
Messier 23 (NGC 6494) is a wide, uniform open cluster located 2,375 light-years (728 ± 11 parsecs) away in northwestern Sagittarius, perched directly in front of the dark dust clouds bordering the Small Sagittarius Star Cloud (M24). Discovered by Charles Messier on June 20, 1764, M23 spans 27 arcminutes across the sky—nearly the full diameter of the Moon—corresponding to a physical width of about 19 light-years.
Classified as Trumpler Class III 1 m, M23 is striking because its ~400 confirmed member stars have a remarkably narrow brightness range: lacks a dense central cusp, and its brightest 100 stars all shine closely between visual magnitudes 9.4 and 11.5. Isochrone fitting to Gaia DR3 astrometry yields an age of ~330 million years and near-solar metallicity ([Fe/H] ≈ −0.04 dex), with the cluster's main sequence turning off around spectral type B9 V alongside half a dozen evolved red-clump giants.
Because M23 sits on the near side of the Carina–Sagittarius arm while dark molecular clouds lie immediately behind it, the dark background acts like a natural velvet curtain that blocks out distant Milky Way bulge stars and makes M23's looping chains of stars stand out in sharp relief.
Practical Visual Observing Guide
- Located 4.5° northwest of Mu Sagittarii (Polis) and 2.5° northwest of the Trifid Nebula (M20).
- In 7×50 or 10×50 binoculars M23 is a large, mottled 5.5-magnitude patch bordered on the northwest by a bright 6.5-magnitude foreground star (HD 163245).
- Best viewed in an 80–150 mm telescope at low power (25×–50×), where over 100 stars of similar 10th-magnitude brightness form graceful bat-wing arcs radiating from the center.
Catalog Cross-Identifications & Aliases
Common Aliases: M23 · NGC 6494
| Catalog Authority | Identifier |
|---|---|
| MESSIER | M 23 |
| NGC | NGC 6494 |
| SIMBAD | M 23 |
| WIKIDATA | Q11369 |
Related Objects, Comparisons & Guides
Messier 25 (IC 4725 Cepheid Calibrator Cluster)
Coordinates, Gaia DR3 distance (661 pc), magnitude 4.6, U Sagittarii Cepheid distance-ladder calibrator, and observing guide for M25.
Lagoon Nebula (Messier 8 / NGC 6523)
Coordinates, Gaia DR3 distance (1.25 kpc), NGC 6530 cluster, Hourglass core, and observing guide for the Lagoon Nebula (M8) in Sagittarius.
Trifid Nebula (Messier 20 / NGC 6514)
Coordinates, Gaia DR3 distance (1.26 kpc), Barnard 85 trisecting dust lanes, HN 40 multiple star, and observing guide for M20 in Sagittarius.
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.
Trigonometric Parallax, Parsecs & Gaia DR3
How trigonometric parallax (d_pc = 1 / p_arcsec), the distance modulus equation, Hipparcos, and Gaia DR3 microarcsecond astrometry measure cosmic distances.
Scientific Sources & Dataset Provenance
- ESA Gaia Archive — Data Release 3 (DR3 (2022-06-13)): Gaia Collaboration, Vallenari, A., et al. 2023, A&A, 674, A1 (Gaia Data Release 3) — European Space Agency / Gaia DPAC
- 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