Alessi 2
(MWSC 419; LeDrew 4)
0.93
UTI
0.82
CN
0.85
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Nm (P>50%)
287
Core radius and density
2.1 [pc], 4.2 [pc-2]
- CN 0.82 Rich
- Cdens 0.85 Dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Alessi 2 is a rich, dense object of very high C3 quality. Its parallax locates it at a 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 and mass parameters (see Parameters). It is very 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 | 71.607 | 55.181 | 1.615 | -0.915 | -1.095 | -10.442 |
| Otto et al. | 2026 | 71.557 | 55.184 | â | -0.9 | -1.05 | -10.1 |
| Li et al. | 2025 | 71.602 | 55.199 | 1.589 | -0.904 | -1.046 | â |
| Yang et al. | 2025 | 71.557 | 55.184 | â | â | â | â |
| Almeida et al. | 2025 | 71.627 | 55.234 | â | â | â | â |
| Alfonso et al. | 2024 | 71.619 | 55.181 | 1.583 | -0.925 | -1.099 | â |
| Zhang et al. | 2024 | 71.557 | 55.184 | â | â | â | â |
| Hunt & Reffert | 2024 | 71.557 | 55.184 | 1.618 | -0.928 | -1.095 | -10.275 |
| Cavallo et al. | 2024 | 71.648 | 55.186 | 1.623 | â | â | â |
| Hunt & Reffert | 2023 | 71.557 | 55.184 | 1.618 | -0.928 | -1.095 | -10.275 |
| Almeida et al. | 2023 | 71.511 | 55.213 | â | â | â | â |
| Just et al. | 2023 | 71.552 | 55.255 | â | â | â | â |
| He et al. | 2022 | 71.606 | 55.2 | 1.624 | -0.944 | -1.091 | â |
| Jadhav & Subramaniam | 2021 | 71.602 | 55.199 | â | â | â | â |
| Dias et al. | 2021 | 71.627 | 55.234 | 1.582 | -0.896 | -1.055 | -10.466 |
| Cantat-Gaudin et al. | 2020 | 71.602 | 55.199 | 1.589 | -0.904 | -1.046 | â |
| Zhong et al. | 2020 | 71.602 | 55.199 | â | -0.904 | -1.046 | -20.564 |
| Cantat-Gaudin & Anders | 2020 | 71.602 | 55.199 | 1.589 | -0.904 | -1.046 | â |
| Bossini et al. | 2019 | 71.602 | 55.199 | â | â | â | â |
| Soubiran et al. | 2018 | 71.602 | 55.199 | â | â | â | -11.0 |
| Bica et al. | 2019 | 71.561 | 55.234 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 71.602 | 55.199 | 1.589 | -0.904 | -1.046 | â |
| Dias et al. | 2018 | â | â | â | 0.56 | -2.7 | â |
| Dib et al. | 2018 | 71.565 | 55.255 | â | â | â | â |
| Loktin & Popova | 2017 | 71.505 | 55.207 | â | 1.62 | -3.654 | â |
| Sampedro et al. | 2017 | 71.508 | 55.207 | â | 2.31 | 0.86 | â |
| Joshi et al. | 2016 | 71.565 | 55.255 | â | â | â | â |
| Kharchenko et al. | 2016 | 71.552 | 55.255 | â | â | â | â |
| Dias et al. | 2014 | 71.508 | 55.207 | â | 1.75 | 0.14 | â |
| Kharchenko et al. | 2013 | 71.565 | 55.255 | â | -0.91 | -0.75 | â |
| Kharchenko et al. | 2012 | 71.565 | 55.255 | â | -0.91 | -0.75 | â |
| Piskunov et al. | 2008 | 71.548 | 55.228 | â | â | â | â |
| Piskunov et al. | 2007 | 71.548 | 55.228 | â | â | â | â |
| van den Bergh | 2006 | 71.6 | 55.25 | â | â | â | â |
| Kharchenko et al. | 2005 | 71.56 | 55.23 | â | -0.08 | 0.31 | â |
| Alessi et al. | 2003 | 71.6 | 55.25 | â | 0.2 | -1.1 | â |
| Dias et al. | 2002 | 71.508 | 55.207 | â | 0.25 | -1.09 | 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 | 0.59 | 0.57 | 0.75 | 388 | -0.015 | 173 | 0.54 | 0 |
| Otto et al. | 2026 | â | â | â | 355 | 0.050(15) | â | â | â |
| Li et al. | 2025 | 0.58 | 0.68 | â | 538 | -0.029 | â | â | â |
| Yang et al. | 2025 | â | â | â | 263 | -0.110(3) | â | â | â |
| Almeida et al. | 2025 | 0.61 | 0.81 | â | 396 | â | 391 | â | â |
| Alfonso et al. | 2024 | 0.66 | 0.52 | â | 701 | 0.058 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.046(1) | â | â | â |
| Hunt & Reffert | 2024 | 0.59 | 0.57 | 0.75 | 264 | â | 289(1) | â | â |
| Cavallo et al. | 2024 | 0.62 | 0.89 | â | 251 | 0.270 | â | â | â |
| Hunt & Reffert | 2023 | 0.59 | 0.57 | 0.75 | 264 | â | â | â | â |
| Almeida et al. | 2023 | 0.60 | 0.92 | â | 318 | -0.086 | 317(1) | 0.54 | â |
| Just et al. | 2023 | â | â | â | 499 | â | 28 | â | â |
| He et al. | 2022 | â | 0.85 | â | 282 | â | â | â | â |
| Tarricq et al. | 2022 | 0.65 | â | â | 380 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 0.66 | 0.52 | â | 355 | â | 515 | â | 0(1) |
| Dias et al. | 2021 | 0.61 | 0.81 | â | 396 | 0.057 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.66 | 0.52 | â | 355 | â | â | â | â |
| Kounkel et al. | 2020 | 0.62 | 0.78 | â | 195 | â | â | â | â |
| Zhong et al. | 2020 | 0.62(1) | 0.49 | â | 8759 | -0.045 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.62 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 0.59 | 0.48 | â | 574 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.62 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.62 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 0.52 | â | â | 499 | â | â | â | â |
| Loktin & Popova | 2017 | 0.57 | 0.97 | â | 34 | â | â | â | â |
| Joshi et al. | 2016 | 0.52 | 0.47 | â | 499 | â | 45 | â | â |
| Kharchenko et al. | 2016 | 0.52 | 0.47 | â | 499 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.52 | 0.47 | â | 499 | â | â | â | â |
| Kharchenko et al. | 2012 | 0.52 | 0.47 | â | 499 | â | â | â | â |
| Piskunov et al. | 2008 | 0.50 | 0.57 | â | 398 | â | 57(1) | â | â |
| Piskunov et al. | 2007 | 0.50 | 0.57 | â | 398 | â | 10 | â | â |
| van den Bergh | 2006 | 0.50 | 0.57 | â | 316 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.50 | 0.57 | â | 398 | â | â | â | â |
| Alessi et al. | 2003 | 0.50 | 0.57 | â | 316 | â | â | â | â |
| Dias et al. | 2002 | 0.50 | 0.57 | â | 316 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P258, along with Theia_1040.
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.2799, e_all=0.4225.
Piecka & Paunzen (2021)
Belongs to cluster aggregate 'Agg04' along with UPK 312.
Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010). List of clusters and alike reported by B. Alessi.