Ruprecht 53
(MWSC 1442; OCL 682; ESO 494 32)
0.72
UTI
0.54
CN
0.89
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
11.9 [arcmin]
- CN 0.54 Moderately populated
- Cdens 0.89 Dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
Ruprecht 53 is a moderately populated, dense object of high C3 quality. Its parallax locates it at a relatively close* distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~1.03 kpc) differs significantly from the median photometric distance (~1.52 kpc).
Note: This object shares a large 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 | â | 122.737 | -27.027 | 0.968 | -2.864 | 1.004 | 11.48 |
| Hunt & Reffert | 2024 | 122.741 | -27.003 | 0.956 | -2.877 | 0.99 | 11.802 |
| Cavallo et al. | 2024 | 122.728 | -27.037 | 0.957 | â | â | â |
| Hunt & Reffert | 2023 | 122.741 | -27.003 | 0.956 | -2.877 | 0.99 | 11.802 |
| Just et al. | 2023 | 122.674 | -26.937 | â | â | â | â |
| Bica et al. | 2019 | 122.717 | -26.991 | â | â | â | â |
| Kharchenko et al. | 2016 | 122.674 | -26.937 | â | â | â | â |
| Dias et al. | 2014 | 122.725 | -27.0 | â | -2.0 | 4.52 | â |
| Kharchenko et al. | 2013 | 122.68 | -26.94 | â | -0.34 | 5.63 | â |
| Piskunov et al. | 2008 | 122.692 | -26.993 | â | â | â | â |
| Kharchenko et al. | 2005 | 122.7 | -27.0 | â | -1.11 | 0.32 | â |
| Kharchenko et al. | 2003 | 122.64 | -27.0 | â | -0.58 | 0.46 | â |
| Dias et al. | 2002 | 122.725 | -26.0 | â | -2.0 | 4.52 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 126* | â | â |
| Cavallo et al. | 2024 | 1.00 | 0.19 | â | 309 | -0.070 | â | â | â |
| Hunt & Reffert | 2023 | 0.97 | 0.09 | 0.54 | 343 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 724 | â | 97 | â | â |
| Kharchenko et al. | 2016 | 1.52 | 0.84 | â | 724 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.52 | 0.84 | â | 724 | â | â | â | â |
| Piskunov et al. | 2008 | 1.70 | 0.34 | â | 389 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.70 | 0.34 | â | 389 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.00 | 0.46 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.70 | 0.34 | â | 389 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.