King 2
(MWSC 79; OCL 311)
0.92
UTI
0.89
CN
1.0
Cdens
0.75
CC3
0.97
Clit
1.0
Cdup
Nm (P>50%)
476
Core radius and density
2.2 [pc], 8.3 [pc-2]
- CN 0.89 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.97 Very well-studied
- Cdup 1.0 Unique
Overview
King 2 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 12.739 | 58.192 | 0.135 | -1.399 | -0.869 | -137.646 |
| Otto et al. | 2026 | 12.739 | 58.187 | â | -1.36 | -0.82 | -42.4 |
| Li et al. | 2025 | 12.741 | 58.188 | 0.166 | -1.358 | -0.824 | â |
| Hunt & Reffert | 2024 | 12.739 | 58.187 | 0.162 | -1.419 | -0.844 | -101.762 |
| Cavallo et al. | 2024 | 12.743 | 58.192 | 0.154 | â | â | â |
| Hunt & Reffert | 2023 | 12.739 | 58.187 | 0.162 | -1.419 | -0.844 | -101.762 |
| Just et al. | 2023 | 12.722 | 58.198 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 12.741 | 58.188 | â | â | â | â |
| Jaehnig et al. | 2021 | 12.736 | 58.194 | 0.156 | -1.381 | -0.816 | â |
| Netopil et al. | 2022 | 12.75 | 58.184 | â | â | â | -145.06 |
| Rain et al. | 2021 | 12.741 | 58.188 | 0.166 | -1.358 | -0.824 | â |
| Spina et al. | 2021 | 12.741 | 58.188 | 0.15 | -1.351 | -0.828 | â |
| Cantat-Gaudin et al. | 2020 | 12.741 | 58.188 | 0.166 | -1.358 | -0.824 | â |
| Donor et al. | 2020 | 12.732 | 58.201 | â | -1.49 | -0.92 | -135.5 |
| Cantat-Gaudin & Anders | 2020 | 12.741 | 58.188 | 0.166 | -1.358 | -0.824 | â |
| Bica et al. | 2019 | 12.723 | 58.202 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 12.741 | 58.188 | 0.166 | -1.358 | -0.824 | â |
| Loktin & Popova | 2017 | 12.75 | 58.201 | â | -0.223 | -1.271 | -144.2 |
| Sampedro et al. | 2017 | 12.75 | 58.183 | â | â | â | â |
| Kharchenko et al. | 2016 | 12.722 | 58.198 | â | â | â | â |
| Netopil et al. | 2016 | 12.75 | 58.183 | â | â | â | â |
| Dias et al. | 2014 | 12.75 | 58.183 | â | -2.0 | -2.6 | â |
| Kharchenko et al. | 2013 | 12.732 | 58.201 | â | -1.71 | -0.08 | -144.2 |
| Gozha et al. | 2012 | 12.75 | 58.184 | â | â | â | â |
| Kharchenko et al. | 2012 | 12.732 | 58.201 | â | -1.71 | -0.08 | -144.25 |
| Bukowiecki et al. | 2011 | 12.738 | 58.196 | â | â | â | â |
| Ahumada & Lapasset | 2007 | 12.75 | 58.183 | â | â | â | â |
| van den Bergh | 2006 | 12.75 | 58.183 | â | â | â | â |
| Dias et al. | 2002 | 12.75 | 58.183 | â | -2.0 | -2.6 | -144.25 |
| Lynga | 1987 | 12.761 | 58.202 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 5.5 | 0.98 | 2.16 | 4376 | -0.360 | 1949 | â | 26 |
| Otto et al. | 2026 | â | â | â | 4074 | -0.180(15) | â | â | â |
| Li et al. | 2025 | 5.15 | 1.69 | â | 1366 | -0.360 | â | â | â |
| Hunt & Reffert | 2024 | 5.07 | 1.22 | 2.16 | 1096 | â | 1949(1) | â | â |
| Cavallo et al. | 2024 | 4.09 | 1.13 | â | 2291 | -0.290 | â | â | â |
| Hunt & Reffert | 2023 | 5.07 | 1.22 | 2.16 | 1096 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 4677 | â | 305 | â | â |
| Spina et al. | 2022 | â | â | â | â | -0.360 | â | â | â |
| Jadhav & Subramaniam | 2021 | 6.76 | 0.97 | â | 4074 | â | 9995 | â | 14(1) |
| Jaehnig et al. | 2021 | 6.35(1) | â | â | â | â | â | â | â |
| Netopil et al. | 2022 | 6.61(1) | â | â | 5012 | -0.360(1) | â | â | â |
| Rain et al. | 2021 | 5.14 | 0.98 | â | 6026 | â | â | â | 26 |
| Spina et al. | 2021 | 4.65 | â | â | 4074 | -0.359(20) | â | â | â |
| Cantat-Gaudin et al. | 2020 | 6.76 | 0.97 | â | 4074 | â | â | â | â |
| Kounkel et al. | 2020 | 4.36 | 1.14 | â | 1698 | â | â | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.360 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 5.14 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 5.14 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.78 | 1.73 | â | 2818 | â | â | â | â |
| Kharchenko et al. | 2016 | 5.50 | 0.95 | â | 4677 | â | â | â | â |
| Netopil et al. | 2016 | 12.39 | â | â | 4920 | â | â | â | â |
| Kharchenko et al. | 2013 | 5.50 | 0.95 | â | 4677 | -0.420 | â | â | â |
| Gozha et al. | 2012 | 5.75 | â | â | 6026 | -0.420 | â | â | â |
| Kharchenko et al. | 2012 | 5.50 | 0.95 | â | 4677 | -0.420 | â | â | â |
| Bukowiecki et al. | 2011 | 7.01(1) | 1.17 | â | 1778 | â | â | â | â |
| Paunzen et al. | 2010 | â | â | â | â | -0.320 | â | â | â |
| Ahumada & Lapasset | 2007 | â | 0.98 | â | 6026 | â | â | â | 30 |
| van den Bergh | 2006 | 5.75 | 0.98 | â | 6026 | â | â | â | â |
| Dias et al. | 2002 | 5.75 | 0.98 | â | 6026 | -0.420 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Silver sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.09 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.09 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.2019, e_all=0.0876.
Rain et al. (2021)
The isochrone was move in 0.05 to the red and a distance modulus of m-M=13.8 was used to fit it.
Ahumada & Lapasset (2007)
Only candidates inside r/R=1 were considered. Adopted cluster centre: star 419 of (1990A&A...240..262A).