King Cobra Cluster (Messier 67 / NGC 2682)
Coordinates, Gaia DR3 distance (855 pc), 4.0 Gyr solar-twin age, exoplanet hosts, and observing guide for ancient open cluster M67 in Cancer.
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) | 6.1 mag | ± 0.1 mag | Wide-aperture integrated photometry | definitive | Revised New General Catalogue and Index Catalogue (RNGC/IC) |
| Heliocentric distance | 2790 ly | ± 40 ly | Gaia DR3 astrometric parallax of ~1,500 members (855 ± 12 pc) (J2016.0) | definitive | ESA Gaia Archive — Data Release 3 |
| Apparent diameter | 30 arcmin | ± 2.5 arcmin | Member star-count boundary | high-confidence | Revised New General Catalogue and Index Catalogue (RNGC/IC) |
| Turnoff, asteroseismology & white-dwarf age | 4 Gyr | ± 0.2 Gyr | Kepler K2 giant asteroseismology + Gaia DR3 turnoff & white-dwarf cooling | definitive | ESA Gaia Archive — Data Release 3 |
J2000 Equatorial Sky Chart & Culmination Altitude
The chart below plots King Cobra Cluster (Messier 67 / NGC 2682) at RA 08h 51m 18.00s, Dec +11° 48′ 00.0″ within Cancer, 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 67 (NGC 2682, the King Cobra or Golden Eye Cluster) is one of the oldest and most scientifically pivotal open clusters in the Milky Way, situated 2,790 light-years (855 ± 12 parsecs) away in southern Cancer. Discovered by Johann Gottfried Koehler before 1779 and independently cataloged by Charles Messier on April 6, 1780, M67 has survived for 4.0 ± 0.2 billion years—nearly ten times longer than typical open clusters—because its inclined Galactic orbit lifts it 1,500 light-years above the dusty midplane where destructive giant molecular clouds reside.
Because M67 has an iron abundance virtually identical to our Sun ([Fe/H] = 0.00 ± 0.02 dex) and an age close to the Sun's 4.6 billion years, it hosts more than 100 true 'solar twins' (such as YBP 1194, which shares the Sun's mass, temperature, and chemical fingerprint to within 1%). Its color-magnitude diagram is the foundational textbook benchmark for testing the morphological 'hook' at the main-sequence turnoff where 1.25-solar-mass stars develop convective hydrogen-burning cores.
M67 also contains ~30 prominent blue stragglers, over 200 cooling white dwarfs, and at least five confirmed exoplanets—including the hot Jupiter YBP 1194 b orbiting a solar twin and the giant planet S364 b orbiting an evolved red giant.
Practical Visual Observing Guide
- Located just 1.8° directly west of the 4.2-magnitude double star Acubens (α Cancri) in southern Cancer, about 8.5° south-southeast of the Beehive Cluster (M44).
- In 10×50 binoculars M67 is an easy 6.1-magnitude oval patch anchored on its northeastern corner by a 7.8-magnitude foreground star (HD 75700).
- Through a 100–200 mm telescope at 60×–120×, over 100 golden-yellow and orange subgiants and red-clump giants curve into the famous hooded 'King Cobra' shape.
Catalog Cross-Identifications & Aliases
Common Aliases: M67 · NGC 2682 · King Cobra Cluster · Golden Eye Cluster
| Catalog Authority | Identifier |
|---|---|
| MESSIER | M 67 |
| NGC | NGC 2682 |
| SIMBAD | M 67 |
| WIKIDATA | Q11483 |
Related Objects, Comparisons & Guides
Beehive Cluster (Messier 44 Praesepe)
Coordinates, Gaia DR3 distance (186.2 pc), magnitude 3.1, exoplanet hosts, and observing guide for the Beehive Cluster (M44 / NGC 2632).
Messier 71 (NGC 6838 Disk Globular Cluster)
Coordinates, Gaia DR3 distance (4.00 kpc), magnitude 8.19, metal-rich thick-disk chemistry, and observing guide for Messier 71 in Sagitta.
Hyades (Melotte 25 Nearest Cluster)
Coordinates, Gaia DR3 distance (47.0 pc), age 650 Myr, moving-group kinematics, and observing guide for the Hyades cluster in Taurus.
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.
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
- 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