King 2
(MWSC 79; OCL 311)
0.93
UTI
0.89
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
2.1 [arcmin]
- CN 0.89 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 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.
(*): The parallax distance estimate (~7.40 kpc) differs significantly from the median photometric distance (~5.50 kpc).
Note: This object contains blue stragglers according to at least one source.
Very distant
Low extinction
Massive
Near-solar metallicity
Old
Contains BSS
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 12.739 | 58.192 | 0.135 | -1.399 | -0.869 | -137.646 |
| 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 |
| Jaehnig et al. | 2021 | 12.736 | 58.194 | 0.156 | -1.381 | -0.816 | â |
| Rain et al. | 2021 | 12.741 | 58.188 | 0.166 | -1.358 | -0.824 | 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 |
| Kharchenko et al. | 2016 | 12.722 | 58.198 | 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 |
| 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 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 5.15 | 1.69 | â | 1366 | -0.360 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1949* | 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 |
| Jaehnig et al. | 2021 | 6.35* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 5.14 | 0.96 | â | 6026 | â | â | â | 26 |
| Cantat-Gaudin et al. | 2020 | 6.76 | 0.97 | â | 4074 | 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 | 1.70 | â | 2818 | â | â | â | â |
| Kharchenko et al. | 2016 | 5.50 | 0.93 | â | 4677 | â | â | â | â |
| Kharchenko et al. | 2013 | 5.50 | 0.93 | 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 | 0.93 | â | 4677 | -0.420 | â | â | â |
| van den Bergh | 2006 | 5.75 | 0.96 | â | 6026 | â | â | â | â |
| Dias et al. | 2002 | 5.75 | 0.96 | â | 6026 | -0.420 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.