Markarian 50
(MWSC 3712; Mrk 50)
0.83
UTI
0.52
CN
1.0
Cdens
1.0
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad)
18.3 [N/pc2]
- CN 0.52 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
Markarian 50 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~3.11 kpc) differs significantly from the median photometric distance (~2.36 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 348.809 | 60.448 | 0.322 | -3.414 | -2.628 | â |
| Almeida et al. | 2025 | 348.812 | 60.451 | â | â | â | â |
| Hunt & Reffert | 2024 | 348.809 | 60.44 | 0.328 | -3.398 | -2.648 | â |
| Celli et al. | 2024 | 348.806 | 60.448 | â | â | â | â |
| Cavallo et al. | 2024 | 348.811 | 60.448 | 0.326 | â | â | â |
| Hunt & Reffert | 2023 | 348.809 | 60.44 | 0.328 | -3.398 | -2.648 | â |
| Just et al. | 2023 | 348.806 | 60.43 | â | â | â | â |
| Jaehnig et al. | 2021 | 348.806 | 60.439 | 0.346 | -3.438 | -2.562 | â |
| Rain et al. | 2021 | 348.806 | 60.448 | 0.323 | -3.465 | -2.56 | â |
| Dias et al. | 2021 | 348.812 | 60.451 | 0.317 | -3.495 | -2.568 | â |
| Cantat-Gaudin et al. | 2020 | 348.806 | 60.448 | 0.323 | -3.465 | -2.56 | â |
| Cantat-Gaudin & Anders | 2020 | 348.806 | 60.448 | 0.323 | -3.465 | -2.56 | â |
| Cantat-Gaudin et al. | 2018 | 348.806 | 60.448 | 0.323 | -3.465 | -2.56 | â |
| Dias et al. | 2018 | â | â | â | -3.99 | -2.51 | â |
| Loktin & Popova | 2017 | 348.78 | 60.436 | â | -0.464 | -1.643 | -81.0 |
| Sampedro et al. | 2017 | 348.825 | 60.467 | -2.95 | 0.91 | â | â |
| Kharchenko et al. | 2016 | 348.806 | 60.43 | â | â | â | â |
| Kharchenko et al. | 2013 | 348.813 | 60.434 | â | -0.31 | -1.54 | -81.0 |
| Kharchenko et al. | 2012 | 348.813 | 60.434 | â | -0.31 | -1.54 | -81.0 |
| Bukowiecki et al. | 2011 | 348.792 | 60.438 | â | â | â | â |
| Kharchenko et al. | 2007 | 348.82 | 60.47 | â | 0.02 | â | â |
| Ahumada & Lapasset | 2007 | 348.825 | 60.467 | â | â | â | â |
| van den Bergh | 2006 | 348.809 | 60.448 | â | â | â | â |
| Dias et al. | 2002 | 348.825 | 60.467 | â | -0.96 | -6.43 | â |
| Dambis | 1999 | 348.807 | 60.45 | â | â | â | â |
| Lynga | 1987 | 348.825 | 60.494 | â | â | â | -81.0 |
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 | 2.36 | 2.47 | 1.14 | 13 | -0.077 | 309 | â | 0 |
| Almeida et al. | 2025 | 2.68 | 2.24 | â | 13 | â | 331 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 583(1) | â | â |
| Celli et al. | 2024 | â | â | â | 12 | â | 307 | â | â |
| Cavallo et al. | 2024 | 2.36 | 2.24 | â | 25 | -0.100 | â | â | â |
| Hunt & Reffert | 2023 | 2.78 | 2.41 | 1.14 | 12 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 13 | â | 78 | â | â |
| Jaehnig et al. | 2021 | 2.86(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 2.84 | 2.56 | â | 12 | â | â | â | 0 |
| Dias et al. | 2021 | 2.68 | 2.24 | â | 13 | -0.054 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.21 | 2.35 | â | 11 | â | â | â | â |
| Kounkel et al. | 2020 | 2.89 | 2.25 | â | 21 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.84 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.84 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.11 | 2.47 | â | 15 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.30 | 2.56 | â | 13 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.30 | 2.56 | â | 13 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 309 | â | â |
| Kharchenko et al. | 2012 | 2.30 | 2.56 | â | 13 | â | â | â | â |
| Bukowiecki et al. | 2011 | 1.70(1) | 1.64 | â | 126 | â | â | â | â |
| Ahumada & Lapasset | 2007 | â | 2.56 | â | 13 | â | â | â | 0 |
| van den Bergh | 2006 | 2.11 | 2.56 | â | 13 | â | â | â | â |
| Dias et al. | 2002 | 2.11 | 2.56 | â | 12 | â | â | â | â |
| Dambis | 1999 | 1.78 | 2.28 | â | 13 | â | â | â | â |
| Lynga | 1987 | 2.25 | 2.62 | â | 10 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Part of multiple system G198, along with HSC_880, CWNU_2651 and CWNU_2203.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (50th percentile).