Ruprecht 3
- CN 0.0 Sparse
- Cdens 0.02 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
(*): The parallax distance estimate (~6.63 kpc) differs significantly from the median photometric distance (~1.56 kpc).
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
â ī¸ 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 | 99999â | 100.479 | -29.466 | 0.151 | -0.874 | 1.535 | â |
| Angelo et al. | 2019 | 100.533 | -29.452 | â | â | â | â |
| Bukowiecki et al. | 2011 | 100.529 | -29.452 | 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 | 1.56 | 0.0 | â | 1449 | â | 24 | â | â |
| Angelo et al. | 2019 | 2.29 | â | â | 1120 | â | 24 | â | â |
| Bukowiecki et al. | 2011 | 0.83(1) | 0.00 | â | 1778 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA

Cantat-Gaudin & Anders (2020)
Appears as a tight group of bright stars, but Gaia DR1 and DR2 parallaxes and proper motions show it is an asterism. More details in Appendix A of the article.