ESO 092 05
(MWSC 1752)
0.87
UTI
1.0
CN
1.0
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
2.0 [arcmin]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
ESO 092 05 is a very rich, very dense object of high C3 quality. Its parallax locates it at a very large distance, well below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
Extremely distant
Low extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 150.802 | -64.752 | 0.075 | -3.039 | 2.44 | 70.537 |
| Hu & Soubiran | 2025 | 150.787 | -64.762 | β | β | β | β |
| Hunt & Reffert | 2024 | 150.79 | -64.754 | 0.059 | -3.024 | 2.462 | 27.465 |
| Cavallo et al. | 2024 | 150.787 | -64.762 | 0.057 | β | β | β |
| Hunt & Reffert | 2023 | 150.79 | -64.754 | 0.059 | -3.024 | 2.462 | 27.465 |
| Just et al. | 2023 | 150.797 | -64.791 | β | β | β | β |
| Perren et al. | 2022 | 150.808 | -64.753 | β | β | β | β |
| Cantat-Gaudin et al. | 2020 | 150.801 | -64.755 | 0.061 | -2.919 | 2.397 | β |
| SΓ‘nchez et al. | 2020 | 150.808 | -64.753 | β | -2.767 | 2.43 | β |
| Cantat-Gaudin & Anders | 2020 | 150.801 | -64.755 | 0.061 | -2.919 | 2.397 | β |
| Bica et al. | 2019 | 150.802 | -64.749 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 150.801 | -64.755 | 0.061 | -2.919 | 2.397 | β |
| Kharchenko et al. | 2016 | 150.797 | -64.791 | β | β | β | β |
| Dias et al. | 2014 | 150.808 | -64.753 | β | -6.56 | 3.79 | β |
| Kharchenko et al. | 2013 | 150.802 | -64.795 | β | -13.39 | 4.57 | β |
π‘ 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | β | β | β | β | -0.300* | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 693* | β | β |
| Cavallo et al. | 2024 | 8.09 | 0.62 | β | 7413 | -0.280 | β | β | β |
| Hunt & Reffert | 2023 | 12.23 | 0.69 | 1.51 | 1585 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 1995 | β | 845 | β | β |
| Perren et al. | 2022 | 12.71 | 0.34 | β | 6026 | -0.120 | 33000 | 0.74 | β |
| Cantat-Gaudin et al. | 2020 | 12.42 | 0.17 | β | 4467 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 11.15 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 11.15 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 5.17 | 0.32 | β | 1995 | β | β | β | β |
| Kharchenko et al. | 2013 | 5.17 | 0.32 | β | 1995 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.