Alessi Teutsch 5
(ASCC 118; AT 5; Alessi 27; MWSC 3589)
0.83
UTI
0.79
CN
1.0
Cdens
0.75
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad)
23.8 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
Alessi Teutsch 5 is a rich, very dense object of 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, very young cluster, but with a large variance across recent sources for the absorption and age parameters (see Parameters). It is well-studied in the literature.
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 332.152 | 61.103 | 1.115 | -1.901 | -3.272 | -22.755 |
| Almeida et al. | 2025 | 332.274 | 61.096 | â | â | â | â |
| Alfonso et al. | 2024 | 333.452 | 61.239 | 1.091 | -1.391 | -3.114 | â |
| Hunt & Reffert | 2024 | 332.043 | 61.052 | 1.126 | -1.88 | -3.329 | -22.773 |
| Celli et al. | 2024 | 332.218 | 61.103 | â | â | â | â |
| Cavallo et al. | 2024 | 332.085 | 61.065 | 1.123 | â | â | â |
| Hunt & Reffert | 2023 | 332.043 | 61.052 | 1.126 | -1.88 | -3.329 | -22.773 |
| He et al. | 2022 | 333.275 | 61.36 | 1.114 | -1.43 | -3.086 | â |
| Dias et al. | 2021 | 332.274 | 61.096 | 1.127 | -1.943 | -3.205 | â |
| Cantat-Gaudin et al. | 2020 | 332.218 | 61.103 | 1.111 | -1.895 | -3.207 | â |
| Cantat-Gaudin & Anders | 2020 | 332.218 | 61.103 | 1.111 | -1.895 | -3.207 | â |
| Dias et al. | 2019 | 332.217 | 61.103 | 1.111 | -1.895 | -3.207 | -5.04 |
| Soubiran et al. | 2018 | 332.218 | 61.103 | â | â | â | -21.04 |
| Bica et al. | 2019 | 332.108 | 61.03 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 332.218 | 61.103 | 1.111 | -1.895 | -3.207 | â |
| Dias et al. | 2018 | â | â | â | -2.36 | -2.0 | â |
| Dib et al. | 2018 | 332.115 | 61.095 | â | â | â | â |
| Loktin & Popova | 2017 | 332.115 | 61.028 | â | -1.017 | -0.935 | -42.0 |
| Sampedro et al. | 2017 | 332.113 | 61.028 | -0.76 | -2.51 | â | â |
| Dias et al. | 2014 | 332.112 | 61.028 | â | -0.96 | -2.81 | â |
| Gozha et al. | 2012 | 332.112 | 61.028 | â | â | â | â |
| Piskunov et al. | 2008 | 332.087 | 61.096 | â | â | â | â |
| Kharchenko et al. | 2007 | 332.1 | 61.1 | â | 0.21 | â | -42.0 |
| Kharchenko et al. | 2005 | 332.1 | 61.1 | â | -2.19 | -4.03 | -42.0 |
| Dias et al. | 2002 | 332.113 | 61.028 | â | -0.96 | -2.81 | -42.0 |
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 | 0.885 | 1.055 | 1.29 | 12 | -0.141 | 269 | â | â |
| Liu et al. | 2025 | 1.31 | 0.40 | â | 13 | â | â | â | â |
| Almeida et al. | 2025 | 0.87 | 1.25 | â | 12 | â | 453 | â | â |
| Alfonso et al. | 2024 | 0.86 | 1.02 | â | 14 | -0.050 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 222(1) | â | â |
| Celli et al. | 2024 | â | â | â | 19 | â | 316 | â | â |
| Cavallo et al. | 2024 | 0.89 | 1.41 | â | 5 | -0.230 | â | â | â |
| Hunt & Reffert | 2023 | 0.87 | 0.91 | 1.29 | 6 | â | â | â | â |
| He et al. | 2022 | â | 1.10 | â | 2 | â | â | â | â |
| Dias et al. | 2021 | 0.87 | 1.25 | â | 12 | -0.053 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.91 | 1.02 | â | 19 | â | â | â | â |
| Kounkel et al. | 2020 | 0.85 | 1.19 | â | 14 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.88 | â | â | â | â | â | â | â |
| Dias et al. | 2019 | 0.80 | 1.26 | â | 13 | -0.404 | â | â | â |
| Soubiran et al. | 2018 | 0.88 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.88 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.03 | â | â | 74 | â | â | â | â |
| Loktin & Popova | 2017 | 1.08 | 1.09 | â | 26 | â | â | â | â |
| Gozha et al. | 2012 | 0.90 | â | â | 10 | â | 95 | â | â |
| Piskunov et al. | 2008 | 0.90 | 0.95 | â | 10 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.90 | 0.95 | â | 10 | â | â | â | â |
| Dias et al. | 2002 | 0.90 | 0.95 | â | 10 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 26 along with FSR_0369.
Palma et al. (2025)
Part of multiple system G81, along with HSC_816, FSR_0369, UBC_168 and HSC_789.
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: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Piecka & Paunzen (2021)
Belongs cluster aggregate 'to' Agg08 along with BDSB30.
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.