Alessi 5
(MWSC 1844; FoF 2407; OCSN 138)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
83.7 [N/pc2]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Alessi 5 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, young cluster, but with a large variance across recent sources for the mass parameter (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 | 160.833 | -61.089 | 2.508 | -15.386 | 2.526 | 10.065 |
| Li et al. | 2025 | 160.819 | -61.081 | 2.501 | -15.411 | 2.503 | â |
| Wei et al. | 2025 | 160.83 | -61.039 | 2.514 | -15.351 | 2.469 | â |
| Almeida et al. | 2025 | 160.621 | -61.118 | â | â | â | â |
| Alfonso et al. | 2024 | 160.904 | -61.086 | 2.484 | -15.376 | 2.542 | â |
| Hunt & Reffert | 2024 | 160.902 | -61.111 | 2.497 | -15.4 | 2.544 | 13.41 |
| Cavallo et al. | 2024 | 160.827 | -61.086 | 2.509 | â | â | â |
| Hunt & Reffert | 2023 | 160.902 | -61.111 | 2.497 | -15.4 | 2.544 | 13.41 |
| Qin et al. | 2023 | 160.87 | -61.09 | 2.5 | -15.36 | 2.52 | 9.65 |
| Just et al. | 2023 | 160.824 | -61.166 | â | â | â | â |
| He et al. | 2022 | 160.7 | -61.029 | 2.502 | -15.453 | 2.556 | â |
| Dias et al. | 2021 | 160.621 | -61.118 | 2.492 | -15.363 | 2.537 | 11.504 |
| Cantat-Gaudin et al. | 2020 | 160.819 | -61.081 | 2.501 | -15.411 | 2.503 | â |
| Cantat-Gaudin & Anders | 2020 | 160.819 | -61.081 | 2.501 | -15.411 | 2.503 | â |
| Liu & Pang | 2019 | 160.691 | -61.076 | 2.494 | -15.354 | 2.569 | â |
| Bossini et al. | 2019 | 160.819 | -61.081 | â | â | â | â |
| Soubiran et al. | 2018 | 160.819 | -61.081 | â | â | â | 12.49 |
| Bica et al. | 2019 | 160.777 | -61.165 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 160.819 | -61.081 | 2.501 | -15.411 | 2.503 | â |
| Loktin & Popova | 2017 | 160.785 | -61.167 | â | -14.33 | 4.4 | 8.2 |
| Kharchenko et al. | 2016 | 160.824 | -61.166 | â | â | â | â |
| Dias et al. | 2014 | 160.783 | -61.167 | â | -2.62 | -1.91 | â |
| Kharchenko et al. | 2013 | 160.83 | -61.17 | â | -12.5 | 2.42 | 8.2 |
| Gozha et al. | 2012 | 160.783 | -61.167 | â | â | â | â |
| Piskunov et al. | 2008 | 160.777 | -61.165 | â | â | â | â |
| Kharchenko et al. | 2007 | 160.78 | -61.17 | â | 0.3 | â | 12.8 |
| Piskunov et al. | 2007 | 160.777 | -61.165 | â | â | â | â |
| van den Bergh | 2006 | 160.725 | -61.2 | â | â | â | â |
| Kharchenko et al. | 2005 | 160.78 | -61.17 | â | -14.56 | 3.77 | 12.8 |
| Alessi et al. | 2003 | 160.725 | -61.2 | â | -14.3 | 4.4 | â |
| Dias et al. | 2002 | 160.783 | -61.167 | â | -14.33 | 4.4 | 18.0 |
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 | 0.4 | 0.48 | 0.73 | 51 | 0.000 | 37 | 0.17 | â |
| Li et al. | 2025 | 0.44 | 0.57 | â | 54 | 0.048 | â | â | â |
| Wei et al. | 2025 | 0.51 | 0.76 | â | 41 | 0.000 | 492 | 0.17 | â |
| Almeida et al. | 2025 | 0.40 | 0.40 | â | 61 | â | 408 | â | â |
| Alfonso et al. | 2024 | 0.42 | 0.62 | â | 49 | 0.063 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 684(1) | â | â |
| Cavallo et al. | 2024 | 0.41 | 0.85 | â | 26 | 0.130 | â | â | â |
| Hunt & Reffert | 2023 | 0.38 | 0.40 | 0.73 | 56 | â | â | â | â |
| Qin et al. | 2023 | 0.48 | 0.59 | â | 56 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 58 | â | 18 | â | â |
| He et al. | 2022 | â | 0.50 | â | 40 | â | â | â | â |
| Tarricq et al. | 2022 | 0.42 | â | â | 68 | â | â | â | â |
| Dias et al. | 2021 | 0.40 | 0.40 | â | 61 | 0.064 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.42 | 0.62 | â | 68 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.40 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 34 | -0.250 | â | â | â |
| Bossini et al. | 2019 | 0.35 | 0.59 | â | 53 | -0.133 | â | â | â |
| Soubiran et al. | 2018 | 0.40 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.40 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.42 | 0.46 | â | 40 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.38 | 0.64 | â | 58 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.38 | 0.64 | â | 58 | -0.382 | â | â | â |
| Gozha et al. | 2012 | 0.40 | â | â | 40 | â | 37 | â | â |
| Piskunov et al. | 2008 | 0.40 | 0.46 | â | 51 | â | 18(1) | â | â |
| Piskunov et al. | 2007 | 0.40 | 0.46 | â | 51 | â | 9 | â | â |
| van den Bergh | 2006 | 0.40 | 0.46 | â | 40 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.40 | 0.46 | â | 51 | â | â | â | â |
| Alessi et al. | 2003 | 0.40 | 0.46 | â | 40 | â | â | â | â |
| Dias et al. | 2002 | 0.40 | 0.46 | â | 40 | -0.382 | 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: good fit. Isochrone match: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.