Ruprecht 120
(MWSC 2426)
0.76
UTI
0.68
CN
1.0
Cdens
0.5
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
3.8 [arcmin]
- CN 0.68 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 120 is a moderately populated, very dense object of intermediate 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, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 248.791 | -48.285 | 0.465 | -0.851 | -2.159 | β |
| Li et al. | 2025 | 248.789 | -48.282 | 0.415 | -0.88 | -2.2 | β |
| Almeida et al. | 2025 | 248.789 | -48.282 | β | β | β | β |
| Hunt & Reffert | 2024 | 248.807 | -48.277 | 0.488 | -0.862 | -2.148 | β |
| Cavallo et al. | 2024 | 248.795 | -48.278 | 0.485 | β | β | β |
| He et al. | 2023 | 248.785 | -48.268 | 0.514 | -0.884 | -2.184 | β |
| Hunt & Reffert | 2023 | 248.807 | -48.277 | 0.488 | -0.862 | -2.148 | β |
| Almeida et al. | 2023 | 248.792 | -48.286 | β | β | β | β |
| Just et al. | 2023 | 248.779 | -48.299 | β | β | β | β |
| Dias et al. | 2021 | 248.789 | -48.282 | 0.415 | -0.88 | -2.2 | β |
| SΓ‘nchez et al. | 2020 | 248.792 | -48.283 | β | -1.405 | -3.757 | β |
| Kharchenko et al. | 2016 | 248.779 | -48.299 | β | β | β | β |
| Dias et al. | 2014 | 248.792 | -48.283 | β | -0.67 | -2.77 | β |
| Kharchenko et al. | 2013 | 248.79 | -48.3 | β | -2.43 | -0.39 | β |
| van den Bergh | 2006 | 248.85 | -48.3 | β | β | β | β |
| Dias et al. | 2002 | 248.792 | -48.283 | β | -1.24 | -3.44 | β |
π‘ 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 | 1.08 | 1.75 | β | 954 | -0.027 | β | β | β |
| Almeida et al. | 2025 | 2.10 | 2.51 | β | 18 | β | 366 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 407* | β | β |
| Cavallo et al. | 2024 | 1.51 | 2.76 | β | 151 | -0.370 | β | β | β |
| He et al. | 2023 | 1.91 | 3.20 | β | 50 | β | β | β | β |
| Hunt & Reffert | 2023 | 1.91 | 2.56 | 1.53 | 66 | β | β | β | β |
| Almeida et al. | 2023 | 1.75 | 2.41 | β | 25 | 0.177 | 221* | 0.60 | β |
| Just et al. | 2023 | β | β | β | 282 | β | 105 | β | β |
| Dias et al. | 2021 | 2.10 | 2.51 | β | 18 | 0.266 | β | β | β |
| Kharchenko et al. | 2016 | 1.48 | 2.45 | β | 282 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.48 | 2.45 | β | 282 | β | β | β | β |
| van den Bergh | 2006 | 2.00 | 2.17 | β | 151 | β | β | β | β |
| Dias et al. | 2002 | 2.00 | 2.17 | β | 151 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.