Ruprecht 148
(Basel 9; OCL 408; MWSC 421)
0.83
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
4.5 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 148 is a rich, very dense object of 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, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.
Distant
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 | β | 71.641 | 44.711 | 0.261 | -0.178 | -1.138 | -1.19 |
| Almeida et al. | 2025 | 71.641 | 44.716 | β | β | β | β |
| Hunt & Reffert | 2024 | 71.628 | 44.715 | 0.276 | -0.165 | -1.122 | -23.232 |
| Cavallo et al. | 2024 | 71.696 | 44.74 | 0.278 | β | β | β |
| Hunt & Reffert | 2023 | 71.628 | 44.715 | 0.276 | -0.165 | -1.122 | -23.232 |
| Almeida et al. | 2023 | 71.657 | 44.716 | β | β | β | β |
| Dias et al. | 2021 | 71.641 | 44.716 | 0.251 | -0.143 | -1.081 | β |
| Cantat-Gaudin et al. | 2020 | 71.638 | 44.711 | 0.26 | -0.153 | -1.076 | β |
| SΓ‘nchez et al. | 2020 | 71.625 | 44.733 | β | -0.273 | -1.098 | β |
| Cantat-Gaudin & Anders | 2020 | 71.638 | 44.711 | 0.26 | -0.153 | -1.076 | β |
| Bica et al. | 2019 | 71.625 | 44.728 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 71.638 | 44.711 | 0.26 | -0.153 | -1.076 | β |
| Loktin & Popova | 2017 | 71.625 | 44.734 | β | -1.88 | 0.57 | β |
| Dias et al. | 2014 | 71.625 | 44.733 | β | -1.88 | 0.57 | β |
| van den Bergh | 2006 | 71.645 | 44.71 | β | β | β | β |
| Dias et al. | 2002 | 71.625 | 44.733 | β | -1.88 | 0.57 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.80 | 2.05 | β | 80 | β | 262 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 871* | β | β |
| Cavallo et al. | 2024 | 3.24 | 2.18 | β | 93 | 0.480 | β | β | β |
| Hunt & Reffert | 2023 | 3.16 | 2.10 | 1.75 | 96 | β | β | β | β |
| Almeida et al. | 2023 | 3.01 | 2.29 | β | 27 | -0.140 | 388* | 0.64 | β |
| Dias et al. | 2021 | 2.80 | 2.05 | β | 80 | 0.188 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.40 | 1.84 | β | 44 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.46 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.46 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 2.37 | 1.40 | β | 245 | β | β | β | β |
| van den Bergh | 2006 | 3.03 | 2.17 | β | 52 | β | β | β | β |
| Dias et al. | 2002 | 3.03 | 2.18 | β | 53 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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