RSG2
(TRSG 2; Alessi 84)
0.43
UTI
0.57
CN
0.33
Cdens
1.0
CC3
0.13
Clit
1.0
Cdup
Nm (P>50%)
65
Core radius and density
1.8 [pc], 1.7 [pc-2]
- CN 0.57 Moderately populated
- Cdens 0.33 Loose
- CC3 1.0 Very high quality
- Clit 0.13 Rarely studied
- Cdup 1.0 Unique
Overview
RSG2 is a moderately populated, loose object of very high C3 quality. Its parallax locates it at a very close distance, above 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 metallicity parameter (see Parameters). It is rarely studied in the literature.
Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 110.724 | 55.284 | 5.043 | -2.844 | -31.209 | 10.89 |
| Yang et al. | 2025 | 110.51 | 55.385 | â | â | â | â |
| Zhang et al. | 2024 | 110.51 | 55.384 | â | â | â | â |
| Cavallo et al. | 2024 | 111.316 | 54.892 | 5.044 | â | â | â |
| Hunt & Reffert | 2023 | 110.51 | 55.384 | 5.037 | -3.12 | -31.447 | 8.742 |
| Bica et al. | 2019 | 110.725 | 55.282 | â | â | â | â |
| Roser et al. | 2016 | 110.58 | 54.7 | â | -3.02 | -28.8 | 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 | 0.2 | 0.13 | 0.31 | 120 | 0.112 | â | â | â |
| Yang et al. | 2025 | â | â | â | 118 | -0.040(3) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.112(1) | â | â | â |
| Cavallo et al. | 2024 | 0.20 | 0.46 | â | 123 | 0.280 | â | â | â |
| Hunt & Reffert | 2023 | 0.20 | 0.07 | 0.31 | 117 | â | â | â | â |
| Roser et al. | 2016 | 0.20 | 0.13 | â | 126 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as moving group. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Bica et al. (2019)
List of clusters and alike reported by B. Alessi.