Ruprecht 78
(MWSC 1675)
0.91
UTI
0.8
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
1.3 [arcmin]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 78 is a rich, very dense object of high C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is very well-studied in the literature.
(*): The parallax distance estimate (~8.96 kpc) differs significantly from the median photometric distance (~1.71 kpc).
Relatively close
Moderate extinction
Massive
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 142.284 | -53.699 | 0.112 | -3.872 | 3.287 | 52.866 |
| Hunt & Reffert | 2024 | 142.28 | -53.699 | 0.118 | -3.838 | 3.333 | 77.819 |
| Celli et al. | 2024 | 142.282 | -53.696 | â | â | â | â |
| Cavallo et al. | 2024 | 142.123 | -53.672 | 0.118 | â | â | â |
| Hunt & Reffert | 2023 | 142.28 | -53.699 | 0.118 | -3.838 | 3.333 | 77.819 |
| Just et al. | 2023 | 142.256 | -53.707 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 142.282 | -53.696 | 0.097 | -3.892 | 3.252 | â |
| Cantat-Gaudin & Anders | 2020 | 142.282 | -53.696 | 0.097 | -3.892 | 3.252 | â |
| Soubiran et al. | 2018 | 142.282 | -53.696 | â | â | â | 51.32 |
| Cantat-Gaudin et al. | 2018 | 142.282 | -53.696 | 0.097 | -3.892 | 3.252 | â |
| Loktin & Popova | 2017 | 142.29 | -53.699 | â | -9.771 | -1.719 | â |
| Kharchenko et al. | 2016 | 142.256 | -53.707 | â | â | â | â |
| Dias et al. | 2014 | 142.292 | -53.7 | â | -2.47 | -0.79 | â |
| Kharchenko et al. | 2013 | 142.26 | -53.71 | â | -10.0 | 5.4 | â |
| Piskunov et al. | 2008 | 142.286 | -53.695 | â | â | â | â |
| van den Bergh | 2006 | 142.3 | -53.7 | â | â | â | â |
| Kharchenko et al. | 2005 | 142.29 | -53.7 | â | -9.23 | 5.51 | â |
| Kharchenko et al. | 2003 | 142.3 | -53.58 | â | -9.07 | 3.57 | â |
| Dias et al. | 2002 | 142.292 | -53.7 | â | -2.14 | -1.32 | 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 | 1760* | â | â |
| Celli et al. | 2024 | â | â | â | 18 | â | 1250 | â | â |
| Cavallo et al. | 2024 | 6.19 | 3.08 | â | 110 | 0.450 | â | â | â |
| Hunt & Reffert | 2023 | 7.97 | 3.39 | 2.83 | 21 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 18 | â | 44 | â | â |
| Cantat-Gaudin & Anders | 2020 | 7.96 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 7.96 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 7.96 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.73 | 1.10 | â | 113 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.71 | 1.35 | â | 18 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.71 | 1.35 | â | 18 | â | â | â | â |
| Piskunov et al. | 2008 | 1.64 | 1.08 | â | 14 | â | â | â | â |
| van den Bergh | 2006 | 1.64 | 1.08 | â | 98 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.64 | 1.08 | â | 14 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.64 | 1.08 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.64 | 1.08 | â | 97 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.