SAI 86
(MWSC 1435)
0.90
UTI
0.77
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
2.1 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
SAI 86 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is very well-studied in the literature.
Distant
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 122.052 | -36.61 | 0.249 | -3.102 | 2.974 | 62.825 |
| Li et al. | 2025 | 122.055 | -36.606 | 0.219 | -3.111 | 2.931 | â |
| Hu & Soubiran | 2025 | 122.061 | -36.622 | â | â | â | â |
| Almeida et al. | 2025 | 122.053 | -36.609 | â | â | â | â |
| Hunt & Reffert | 2024 | 122.051 | -36.609 | 0.249 | -3.084 | 2.984 | 60.985 |
| Cavallo et al. | 2024 | 122.061 | -36.622 | 0.249 | â | â | â |
| Hunt & Reffert | 2023 | 122.051 | -36.609 | 0.249 | -3.084 | 2.984 | 60.985 |
| Almeida et al. | 2023 | 122.06 | -36.606 | â | â | â | â |
| Just et al. | 2023 | 122.058 | -36.588 | â | â | â | â |
| Dias et al. | 2021 | 122.053 | -36.609 | 0.211 | -3.124 | 2.949 | â |
| Cantat-Gaudin et al. | 2020 | 122.055 | -36.606 | 0.219 | -3.111 | 2.931 | â |
| Cantat-Gaudin & Anders | 2020 | 122.055 | -36.606 | 0.219 | -3.111 | 2.931 | â |
| Soubiran et al. | 2018 | 122.055 | -36.606 | â | â | â | 60.97 |
| Bica et al. | 2019 | 122.058 | -36.608 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 122.055 | -36.606 | 0.219 | -3.111 | 2.931 | â |
| Kharchenko et al. | 2016 | 122.058 | -36.588 | â | â | â | â |
| Dias et al. | 2014 | 122.062 | -36.609 | â | -1.24 | 1.43 | â |
| Kharchenko et al. | 2013 | 122.062 | -36.59 | â | -3.74 | 0.42 | â |
| Glushkova et al. | 2010 | 122.062 | -36.609 | â | â | â | â |
| Dias et al. | 2002 | 122.062 | -36.609 | â | -1.24 | 1.43 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 4.46 | 2.21 | â | 398 | 0.122 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.240* | â | â | â |
| Almeida et al. | 2025 | 3.28 | 1.99 | â | 701 | â | 717 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 887* | â | â |
| Cavallo et al. | 2024 | 2.92 | 1.72 | â | 1023 | -0.030 | â | â | â |
| Hunt & Reffert | 2023 | 3.63 | 1.81 | 1.57 | 354 | â | â | â | â |
| Almeida et al. | 2023 | 3.29 | 2.06 | â | 652 | -0.130 | 628* | 0.56 | â |
| Just et al. | 2023 | â | â | â | 447 | â | 140 | â | â |
| Dias et al. | 2021 | 3.28 | 1.99 | â | 701 | -0.113 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.63 | 1.72 | â | 562 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.03 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.03 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.03 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 3.02 | 2.19 | â | 447 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.02 | 2.19 | â | 447 | â | â | â | â |
| Glushkova et al. | 2010 | 3.03 | 2.14 | â | 398 | â | â | â | â |
| Dias et al. | 2002 | 3.03 | 2.14 | â | 398 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.