Alessi 31
(ASCC 92; MWSC 2723; FoF 2356)
0.88
UTI
0.78
CN
1.0
Cdens
1.0
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad)
18.5 [N/pc2]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
Alessi 31 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, above 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 distance, age, metallicity, and mass parameters (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 267.715 | -11.837 | 1.476 | -1.147 | -4.172 | 2.939 |
| Li et al. | 2025 | 267.698 | -11.853 | 1.477 | -1.164 | -4.122 | â |
| Wei et al. | 2025 | 267.725 | -11.842 | 1.475 | -1.136 | -4.179 | â |
| Almeida et al. | 2025 | 267.665 | -11.882 | â | â | â | â |
| Alfonso et al. | 2024 | 267.719 | -11.85 | 1.442 | -1.139 | -4.178 | â |
| Hunt & Reffert | 2024 | 267.748 | -11.857 | 1.473 | -1.13 | -4.167 | 3.514 |
| Cavallo et al. | 2024 | 267.715 | -11.845 | 1.474 | â | â | â |
| Hunt & Reffert | 2023 | 267.748 | -11.857 | 1.473 | -1.13 | -4.167 | 3.514 |
| Just et al. | 2023 | 267.772 | -11.881 | â | â | â | â |
| He et al. | 2022 | 267.741 | -11.859 | 1.481 | -1.136 | -4.208 | â |
| Tarricq et al. | 2022 | 267.747 | -11.87 | 1.503 | -1.137 | -4.177 | â |
| Dias et al. | 2021 | 267.665 | -11.882 | 1.483 | -1.189 | -4.091 | â |
| Cantat-Gaudin et al. | 2020 | 267.698 | -11.853 | 1.477 | -1.164 | -4.122 | â |
| Cantat-Gaudin & Anders | 2020 | 267.698 | -11.853 | 1.477 | -1.164 | -4.122 | â |
| Liu & Pang | 2019 | 267.752 | -11.835 | 1.474 | -1.157 | -4.115 | â |
| Soubiran et al. | 2018 | 267.698 | -11.853 | â | â | â | 5.36 |
| Bica et al. | 2019 | 267.68 | -12.002 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 267.698 | -11.853 | 1.477 | -1.164 | -4.122 | â |
| Dib et al. | 2018 | 267.78 | -11.88 | â | â | â | â |
| Sampedro et al. | 2017 | 267.675 | -12.002 | -5.25 | -2.2 | â | â |
| Joshi et al. | 2016 | 267.78 | -11.88 | â | â | â | â |
| Kharchenko et al. | 2016 | 267.772 | -11.881 | â | â | â | â |
| Dias et al. | 2014 | 267.675 | -12.002 | â | -5.29 | -2.16 | â |
| Kharchenko et al. | 2013 | 267.78 | -11.88 | â | -6.63 | -5.53 | â |
| Piskunov et al. | 2008 | 267.774 | -11.883 | â | â | â | â |
| Kharchenko et al. | 2005 | 267.78 | -11.88 | â | -7.68 | -4.91 | â |
| Dias et al. | 2002 | 267.675 | -12.002 | â | -5.29 | -2.16 | 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 | 0.65 | 1.75 | 2.5 | 351 | 0.285 | 371 | 0.47 | â |
| Li et al. | 2025 | 0.55 | 1.75 | â | 601 | 0.147 | â | â | â |
| Wei et al. | 2025 | 2.10 | 3.31 | â | 28 | -0.750 | 371 | 0.47 | â |
| Almeida et al. | 2025 | 0.65 | 2.15 | â | 113 | â | 557 | â | â |
| Alfonso et al. | 2024 | 0.71 | 1.75 | â | 79 | 0.359 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 668(1) | â | â |
| Cavallo et al. | 2024 | 0.70 | 2.37 | â | 126 | 0.320 | â | â | â |
| Hunt & Reffert | 2023 | 0.64 | 2.23 | 2.50 | 150 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1202 | â | 25 | â | â |
| He et al. | 2022 | â | 2.70 | â | 40 | â | â | â | â |
| Tarricq et al. | 2022 | 0.70 | â | â | 251 | â | â | â | â |
| Dias et al. | 2021 | 0.65 | 2.15 | â | 113 | 0.359 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.71 | 1.75 | â | 240 | â | â | â | â |
| Kounkel et al. | 2020 | 0.65 | 1.79 | â | 355 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.66 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 347 | 0.250 | â | â | â |
| Soubiran et al. | 2018 | 0.66 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.66 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 0.64 | â | â | 1202 | â | â | â | â |
| Joshi et al. | 2016 | 0.64 | 0.98 | â | 1202 | â | 234 | â | â |
| Kharchenko et al. | 2016 | 0.64 | 0.98 | â | 1202 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.64 | 0.98 | â | 1202 | â | â | â | â |
| Piskunov et al. | 2008 | 0.65 | 0.79 | â | 1023 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.65 | 0.79 | â | 1023 | â | â | â | â |
| Dias et al. | 2002 | 0.65 | 0.79 | â | 1023 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.83 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.83 (50th percentile).
Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010). List of clusters and alike reported by B. Alessi. The Preliminary Amateur Open Cluster Catalog, Version 08/03/2003.