Ruprecht 1
(MWSC 929; OCL 563; FoF 655)
0.95
UTI
0.77
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
7.8 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 1 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Relatively close
Low 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 | 99.075 | -14.166 | 0.641 | -0.299 | -0.902 | 11.208 |
| Li et al. | 2025 | 99.084 | -14.157 | 0.631 | -0.316 | -0.9 | β |
| Hu & Soubiran | 2025 | 99.058 | -14.169 | β | β | β | β |
| Almeida et al. | 2025 | 99.082 | -14.151 | β | β | β | β |
| Hunt & Reffert | 2024 | 99.099 | -14.167 | 0.641 | -0.293 | -0.901 | 9.39 |
| Cavallo et al. | 2024 | 99.058 | -14.169 | 0.642 | β | β | β |
| Hunt & Reffert | 2023 | 99.099 | -14.167 | 0.641 | -0.293 | -0.901 | 9.39 |
| Almeida et al. | 2023 | 99.078 | -14.163 | β | β | β | β |
| Just et al. | 2023 | 99.129 | -14.192 | β | β | β | β |
| Tarricq et al. | 2022 | 99.094 | -14.178 | 0.651 | -0.304 | -0.908 | β |
| Dias et al. | 2021 | 99.082 | -14.151 | 0.633 | -0.322 | -0.899 | 11.459 |
| Cantat-Gaudin et al. | 2020 | 99.084 | -14.157 | 0.631 | -0.316 | -0.9 | β |
| SΓ‘nchez et al. | 2020 | 99.088 | -14.147 | β | -0.262 | -1.023 | β |
| Cantat-Gaudin & Anders | 2020 | 99.084 | -14.157 | 0.631 | -0.316 | -0.9 | β |
| Liu & Pang | 2019 | 99.056 | -14.158 | 0.64 | -0.305 | -0.867 | β |
| Bossini et al. | 2019 | 99.084 | -14.157 | β | β | β | β |
| Soubiran et al. | 2018 | 99.084 | -14.157 | β | β | β | 12.52 |
| Bica et al. | 2019 | 99.104 | -14.148 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 99.084 | -14.157 | 0.631 | -0.316 | -0.9 | β |
| Loktin & Popova | 2017 | 99.09 | -14.146 | β | 0.064 | 0.884 | β |
| Kharchenko et al. | 2016 | 99.129 | -14.192 | β | β | β | β |
| Dias et al. | 2014 | 99.087 | -14.147 | β | 0.49 | -0.66 | β |
| Kharchenko et al. | 2013 | 99.135 | -14.193 | β | 0.48 | 0.44 | β |
| Piskunov et al. | 2008 | 99.099 | -14.183 | β | β | β | β |
| Piskunov et al. | 2007 | 99.099 | -14.183 | β | β | β | β |
| Kharchenko et al. | 2005 | 99.1 | -14.18 | β | 2.2 | 0.1 | β |
| Kharchenko et al. | 2003 | 99.07 | -14.17 | β | -0.75 | -0.74 | β |
| Dias et al. | 2002 | 99.088 | -14.147 | β | 0.49 | -0.66 | 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 | 1.45 | 0.61 | β | 535 | -0.062 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.230* | β | β | β |
| Almeida et al. | 2025 | 1.43 | 0.74 | β | 432 | β | 345 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 739* | β | β |
| Cavallo et al. | 2024 | 1.50 | 0.28 | β | 813 | 0.390 | β | β | β |
| Hunt & Reffert | 2023 | 1.45 | 0.26 | 0.54 | 486 | β | β | β | β |
| Almeida et al. | 2023 | 1.46 | 0.74 | β | 484 | -0.065 | 403* | 0.53 | β |
| Just et al. | 2023 | β | β | β | 617 | β | 30 | β | β |
| Tarricq et al. | 2022 | 1.48 | β | β | 309 | β | β | β | β |
| Dias et al. | 2021 | 1.43 | 0.74 | β | 432 | -0.077 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.53 | 0.61 | β | 288 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.51 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 576 | 0.500 | β | β | β |
| Bossini et al. | 2019 | 1.44 | 0.70 | β | 318 | -0.250 | β | β | β |
| Soubiran et al. | 2018 | 1.51 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.51 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 2.41 | 0.27 | β | 631 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.20 | 0.45 | β | 617 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.20 | 0.45 | β | 617 | β | β | β | β |
| Piskunov et al. | 2008 | 1.10 | 0.46 | β | 575 | β | 133* | β | β |
| Piskunov et al. | 2007 | 1.10 | 0.46 | β | 575 | β | 29 | β | β |
| Kharchenko et al. | 2005 | 1.10 | 0.46 | β | 575 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.00 | 0.62 | β | β | β | β | β | β |
| Dias et al. | 2002 | 1.48 | 0.53 | β | 479 | -0.250 | 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: good fit.
Cavallo et al. (2024)
Gold sample.