Ruprecht 72
(MWSC 1591; OCL 737; ESO 371 22)
0.16
UTI
0.0
CN
0.01
Cdens
0.38
CC3
0.19
Clit
1.0
Cdup
Nm (P>50%)
16
Core radius and density
6.5 [pc], 0.07 [pc-2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.38 Low quality
- Clit 0.19 Rarely studied
- Cdup 1.0 Unique
Overview
Ruprecht 72 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature.
(*): The parallax distance estimate (~3.91 kpc) differs significantly from the median photometric distance (~2.42 kpc).
โ ๏ธ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999โ | 132.981 | -37.639 | 0.256 | -4.188 | 3.102 | โ |
| Just et al. | 2023 | 133.007 | -37.607 | โ | โ | โ | โ |
| Bica et al. | 2019 | 133.011 | -37.61 | โ | โ | โ | โ |
| Kharchenko et al. | 2016 | 133.007 | -37.607 | โ | โ | โ | โ |
| Kharchenko et al. | 2013 | 133.012 | -37.61 | โ | -3.89 | 3.89 | โ |
| Bukowiecki et al. | 2011 | 133.0 | -37.562 | โ | โ | โ | โ |
| van den Bergh | 2006 | 133.025 | -37.6 | โ | โ | โ | โ |
| Lynga | 1987 | 133.038 | -37.605 | โ | โ | โ | โ |
๐ก 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 | 99999โ | 2.415 | 0.5 | โ | 2512 | โ | 238 | โ | โ |
| Just et al. | 2023 | โ | โ | โ | 2512 | โ | 101 | โ | โ |
| Kharchenko et al. | 2016 | 2.24 | 0.46 | โ | 2512 | โ | โ | โ | โ |
| Kharchenko et al. | 2013 | 2.24 | 0.46 | โ | 2512 | โ | โ | โ | โ |
| Bukowiecki et al. | 2012 | โ | โ | โ | โ | โ | 376 | โ | โ |
| Bukowiecki et al. | 2011 | 2.59(1) | 0.54 | โ | 1413 | โ | โ | โ | โ |
| van den Bergh | 2006 | 3.02 | 0.76 | โ | 1259 | โ | โ | โ | โ |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA

Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010).
Dias et al. (2002)
Field fluctuation (Vรกzquez, R. A. et al. 2010, A&A 511, 38); cat V3.5 (Jan 2016)