Ruprecht 36
(MWSC 1344)
0.81
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.77
Clit
1.0
Cdup
Nm (P>50%)
126
Core radius and density
1.2 [pc], 6.9 [pc-2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.77 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 36 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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 age and metallicity parameters (see Parameters). It is 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 | 117.093 | -26.291 | 0.363 | -2.694 | 0.93 | â |
| Li et al. | 2025 | 117.096 | -26.287 | 0.34 | -2.768 | 0.903 | â |
| Almeida et al. | 2025 | 117.095 | -26.281 | â | â | â | â |
| Hunt & Reffert | 2024 | 117.09 | -26.29 | 0.354 | -2.691 | 0.931 | 68.601 |
| Cavallo et al. | 2024 | 117.096 | -26.278 | 0.361 | â | â | â |
| Hunt & Reffert | 2023 | 117.09 | -26.29 | 0.354 | -2.691 | 0.931 | 68.601 |
| Just et al. | 2023 | 117.092 | -26.287 | â | â | â | â |
| Jaehnig et al. | 2021 | 117.099 | -26.29 | 0.372 | -2.725 | 0.902 | â |
| Rain et al. | 2021 | 117.096 | -26.287 | 0.34 | -2.768 | 0.903 | â |
| Dias et al. | 2021 | 117.095 | -26.281 | 0.348 | -2.779 | 0.9 | â |
| Cantat-Gaudin et al. | 2020 | 117.096 | -26.287 | 0.34 | -2.768 | 0.903 | â |
| Cantat-Gaudin & Anders | 2020 | 117.096 | -26.287 | 0.34 | -2.768 | 0.903 | â |
| Soubiran et al. | 2018 | 117.096 | -26.287 | â | â | â | 41.9 |
| Cantat-Gaudin et al. | 2018 | 117.096 | -26.287 | 0.34 | -2.768 | 0.903 | â |
| Dib et al. | 2018 | 117.097 | -26.29 | â | â | â | â |
| Loktin & Popova | 2017 | 117.09 | -26.299 | â | -4.843 | 1.422 | â |
| Sampedro et al. | 2017 | 117.096 | -26.3 | â | -4.03 | 1.26 | â |
| Kharchenko et al. | 2016 | 117.092 | -26.287 | â | â | â | â |
| Dias et al. | 2014 | 117.096 | -26.3 | â | -3.67 | 2.29 | â |
| Kharchenko et al. | 2013 | 117.097 | -26.29 | â | -5.15 | 3.04 | â |
| Bukowiecki et al. | 2011 | 117.1 | -26.278 | â | â | â | â |
| Ahumada & Lapasset | 2007 | 117.1 | -26.3 | â | â | â | â |
| van den Bergh | 2006 | 117.092 | -26.303 | â | â | â | â |
| Dias et al. | 2002 | 117.096 | -26.3 | â | -3.67 | 2.29 | â |
| Lynga | 1987 | 117.123 | -26.294 | 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 | 2.46 | 0.53 | 0.98 | 174 | -0.130 | 262 | â | 0 |
| Li et al. | 2025 | 2.47 | 0.51 | â | 364 | -0.032 | â | â | â |
| Almeida et al. | 2025 | 2.48 | 0.86 | â | 104 | â | 370 | â | â |
| Hunt & Reffert | 2024 | 2.45 | 0.32 | 0.98 | 192 | â | 294(1) | â | â |
| Cavallo et al. | 2024 | 2.18 | 0.74 | â | 275 | -0.370 | â | â | â |
| Hunt & Reffert | 2023 | 2.45 | 0.32 | 0.98 | 192 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 191 | â | 64 | â | â |
| Jaehnig et al. | 2021 | 2.77(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 2.71 | 0.50 | â | 40 | â | â | â | 0 |
| Dias et al. | 2021 | 2.48 | 0.86 | â | 104 | -0.130 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.70 | 0.63 | â | 56 | â | â | â | â |
| Kounkel et al. | 2020 | 2.83 | 0.78 | â | 174 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.71 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.71 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.71 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.82 | â | â | 191 | â | â | â | â |
| Loktin & Popova | 2017 | 1.71 | 0.52 | â | 44 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.82 | 0.47 | â | 191 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.82 | 0.47 | â | 191 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 231 | â | â |
| Bukowiecki et al. | 2011 | 2.06(1) | 0.66 | â | 45 | â | â | â | â |
| Ahumada & Lapasset | 2007 | â | 0.54 | â | 41 | â | â | â | 0 |
| van den Bergh | 2006 | 1.68 | 0.54 | â | 41 | â | â | â | â |
| Dias et al. | 2002 | 1.68 | 0.52 | â | 40 | â | â | â | â |
| Lynga | 1987 | â | â | â | 200 | 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: good fit. Silver sample.
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=0.2682, e_all=0.4529.
Ahumada & Lapasset (2007)
Star 1=CD-26 5011 appears as a straggler in (1972A&AS....7..133V), but it is a non-member according to that reference.