Ruprecht 144
(MWSC 2950; OCL 63)
0.83
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
4.9 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 144 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 278.423 | -11.43 | 0.565 | 0.207 | -0.891 | -2.618 |
| Li et al. | 2025 | 278.437 | -11.425 | 0.555 | 0.142 | -0.876 | â |
| Almeida et al. | 2025 | 278.465 | -11.46 | â | â | â | â |
| Hunt & Reffert | 2024 | 278.411 | -11.421 | 0.568 | 0.236 | -0.886 | -54.134 |
| Cavallo et al. | 2024 | 278.44 | -11.431 | 0.568 | â | â | â |
| Hunt & Reffert | 2023 | 278.411 | -11.421 | 0.568 | 0.236 | -0.886 | -54.134 |
| Just et al. | 2023 | 278.37 | -11.411 | â | â | â | â |
| Dias et al. | 2021 | 278.465 | -11.46 | 0.555 | 0.134 | -0.866 | â |
| Cantat-Gaudin et al. | 2020 | 278.437 | -11.425 | 0.555 | 0.142 | -0.876 | â |
| Cantat-Gaudin & Anders | 2020 | 278.437 | -11.425 | 0.555 | 0.142 | -0.876 | â |
| Bica et al. | 2019 | 278.38 | -11.421 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 278.437 | -11.425 | 0.555 | 0.142 | -0.876 | â |
| Kharchenko et al. | 2016 | 278.37 | -11.411 | â | â | â | â |
| Dias et al. | 2014 | 278.392 | -11.417 | â | -2.7 | 1.46 | â |
| Kharchenko et al. | 2013 | 278.377 | -11.41 | â | -0.29 | -7.34 | â |
| Dias et al. | 2002 | 278.392 | -11.417 | â | -2.7 | 1.46 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.17 | 2.22 | â | 42 | -0.242 | â | â | â |
| Almeida et al. | 2025 | 1.51 | 2.17 | â | 17 | â | 341 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 500* | â | â |
| Cavallo et al. | 2024 | 1.53 | 2.59 | â | 71 | -0.150 | â | â | â |
| Hunt & Reffert | 2023 | 1.61 | 2.31 | 1.62 | 21 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 624 | â | 161 | â | â |
| Dias et al. | 2021 | 1.51 | 2.17 | â | 17 | 0.233 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.59 | 1.90 | â | 30 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.71 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.71 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.65 | 2.06 | â | 624 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.65 | 2.06 | â | 624 | â | â | â | â |
| Dias et al. | 2002 | 1.60 | 2.39 | â | 447 | â | â | â | â |
(*): 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.