Ruprecht 55
(MWSC 1451; OCL 713; ESO 430 25)
0.58
UTI
0.52
CN
0.13
Cdens
0.25
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
5.1 [arcmin]
- CN 0.52 Moderately populated
- Cdens 0.13 Very loose
- CC3 0.25 Low quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 55 is a moderately populated, very loose object of low C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It is very well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 123.113 | -32.573 | 0.165 | -2.345 | 2.913 | 53.509 |
| Almeida et al. | 2025 | 123.113 | -32.581 | â | â | â | â |
| He et al. | 2023 | 123.049 | -32.499 | 0.145 | -2.42 | 3.223 | 102.2 |
| Just et al. | 2023 | 123.137 | -32.602 | â | â | â | â |
| Jaehnig et al. | 2021 | 123.072 | -32.576 | 0.144 | -2.429 | 3.165 | â |
| Dias et al. | 2021 | 123.113 | -32.581 | 0.187 | -2.316 | 2.921 | 64.253 |
| Bica et al. | 2019 | 123.078 | -32.565 | â | â | â | â |
| Loktin & Popova | 2017 | 123.12 | -32.582 | â | -5.777 | 3.16 | 95.3 |
| Kharchenko et al. | 2016 | 123.137 | -32.602 | â | â | â | â |
| Dias et al. | 2014 | 123.112 | -32.583 | â | -2.37 | 0.83 | â |
| Kharchenko et al. | 2013 | 123.142 | -32.605 | â | -2.43 | 2.52 | 95.3 |
| Gozha et al. | 2012 | 123.112 | -32.583 | â | â | â | â |
| Piskunov et al. | 2008 | 123.118 | -32.579 | â | â | â | â |
| Kharchenko et al. | 2007 | 123.12 | -32.58 | â | 0.2 | â | 95.33 |
| Piskunov et al. | 2007 | 123.118 | -32.579 | â | â | â | â |
| van den Bergh | 2006 | 123.125 | -32.583 | â | â | â | â |
| Kharchenko et al. | 2005 | 123.12 | -32.58 | â | -5.06 | 1.32 | 95.33 |
| Kharchenko et al. | 2003 | 123.09 | -32.59 | â | -2.7 | 4.15 | â |
| Dias et al. | 2002 | 123.112 | -32.583 | â | -2.37 | 0.83 | 94.2 |
| Dambis | 1999 | 123.112 | -32.583 | 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 | 4.85 | 1.71 | â | 9 | -0.226 | 1910 | â | â |
| Almeida et al. | 2025 | 4.24 | 1.64 | â | 21 | â | 1067 | â | â |
| He et al. | 2023 | 5.01 | 1.55 | â | 25 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 9 | â | 796 | â | â |
| Jaehnig et al. | 2021 | 6.82(1) | â | â | â | â | â | â | â |
| Dias et al. | 2021 | 4.24 | 1.64 | â | 21 | -0.226 | â | â | â |
| Loktin & Popova | 2017 | 4.85 | 1.71 | â | 8 | â | â | â | â |
| Kharchenko et al. | 2016 | 3.64 | 1.87 | â | 9 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.64 | 1.87 | â | 9 | â | â | â | â |
| Gozha et al. | 2012 | 4.60 | â | â | 10 | â | 37154 | â | â |
| Piskunov et al. | 2008 | 4.89 | 1.74 | â | 9 | â | 13740(1) | â | â |
| Piskunov et al. | 2007 | 4.89 | 1.74 | â | 9 | â | 1910 | â | â |
| van den Bergh | 2006 | 4.89 | 1.74 | â | 7 | â | â | â | â |
| Kharchenko et al. | 2005 | 4.89 | 1.74 | â | 9 | â | â | â | â |
| Kharchenko et al. | 2003 | 4.76 | 1.46 | â | â | â | â | â | â |
| Dias et al. | 2002 | 4.60 | 1.40 | â | 10 | â | â | â | â |
| Dambis | 1999 | 6.79 | 1.71 | â | 8 | â | â | â | â |
(N): Indicates that are N extra values assigned to this parameter in the corresponding reference.

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.