Ruprecht 23
(FSR 1286; MWSC 1248; OCL 632; ESO 492 17; FoF 90)
0.82
UTI
0.8
CN
1.0
Cdens
0.75
CC3
0.77
Clit
1.0
Cdup
Nm (P>50%)
240
Core radius and density
1.5 [pc], 6.6 [pc-2]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.77 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 23 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below 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 metallicity parameter (see Parameters). It is well-studied in the literature.
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 112.663 | -23.375 | 0.342 | -2.065 | 1.61 | 59.894 |
| Li et al. | 2025 | 112.665 | -23.383 | 0.341 | -2.078 | 1.56 | â |
| Almeida et al. | 2025 | 112.669 | -23.387 | â | â | â | â |
| Hunt & Reffert | 2024 | 112.658 | -23.38 | 0.344 | -2.058 | 1.624 | 55.244 |
| Cavallo et al. | 2024 | 112.654 | -23.368 | 0.346 | â | â | â |
| Hunt & Reffert | 2023 | 112.658 | -23.38 | 0.344 | -2.058 | 1.624 | 55.244 |
| Just et al. | 2023 | 112.644 | -23.381 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 112.665 | -23.383 | â | â | â | â |
| Dias et al. | 2021 | 112.669 | -23.387 | 0.34 | -2.081 | 1.553 | 54.405 |
| Cantat-Gaudin et al. | 2020 | 112.665 | -23.383 | 0.341 | -2.078 | 1.56 | â |
| Cantat-Gaudin & Anders | 2020 | 112.665 | -23.383 | 0.341 | -2.078 | 1.56 | â |
| Liu & Pang | 2019 | 112.65 | -23.378 | 0.349 | -2.032 | 1.549 | â |
| Soubiran et al. | 2018 | 112.665 | -23.383 | â | â | â | 56.31 |
| Bica et al. | 2019 | 112.671 | -23.375 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 112.665 | -23.383 | 0.341 | -2.078 | 1.56 | â |
| Dias et al. | 2018 | â | â | â | -2.43 | 2.06 | â |
| Loktin & Popova | 2017 | 112.65 | -23.395 | â | -2.537 | 2.82 | â |
| Sampedro et al. | 2017 | 112.662 | -23.393 | â | -2.21 | 1.98 | â |
| Kharchenko et al. | 2016 | 112.644 | -23.381 | â | â | â | â |
| Dias et al. | 2014 | 112.662 | -23.393 | â | -2.75 | 2.68 | â |
| Kharchenko et al. | 2013 | 112.65 | -23.383 | â | -1.89 | 3.53 | â |
| Bukowiecki et al. | 2011 | 112.662 | -23.385 | â | â | â | â |
| Froebrich et al. | 2007 | 112.667 | -23.394 | â | â | â | â |
| Dias et al. | 2002 | 112.662 | -23.393 | â | -2.75 | 2.68 | â |
| Lynga | 1987 | 112.601 | -23.342 | â | â | â | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.7 | 1.725 | 1.48 | 603 | -0.090 | 877 | â | 0 |
| Li et al. | 2025 | 2.50 | 2.00 | â | 407 | -0.090 | â | â | â |
| Almeida et al. | 2025 | 1.89 | 1.18 | â | 902 | â | 538 | â | â |
| Hunt & Reffert | 2024 | 2.61 | 1.75 | 1.48 | 479 | â | 892(1) | â | â |
| Cavallo et al. | 2024 | 2.54 | 2.10 | â | 479 | -0.090 | â | â | â |
| Hunt & Reffert | 2023 | 2.61 | 1.75 | 1.48 | 479 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 603 | â | 499 | â | â |
| Jadhav & Subramaniam | 2021 | 2.73 | 1.49 | â | 407 | â | 877 | â | 0(1) |
| Dias et al. | 2021 | 1.89 | 1.18 | â | 902 | 0.245 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.73 | 1.49 | â | 407 | â | â | â | â |
| Kounkel et al. | 2020 | 2.85 | 2.08 | â | 513 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.70 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 851 | -1.000 | â | â | â |
| Soubiran et al. | 2018 | 2.70 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.70 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.85 | 1.31 | â | 1622 | â | â | â | â |
| Kharchenko et al. | 2016 | 3.02 | 1.97 | â | 603 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.02 | 1.97 | â | 603 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 1557 | â | â |
| Bukowiecki et al. | 2011 | 2.15(1) | 1.36 | â | 891 | â | â | â | â |
| Dias et al. | 2002 | 3.06 | 1.70 | â | 603 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.4226, e_all=0.1099.