HSC 2142
Summary
HSC 2142 is a sparse, loose object of low C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.
This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.8) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 127.691 | -48.717 | 0.639 | -4.379 | 4.256 | 32.838 |
| Cavallo et al. (2024) | 127.692 | -48.686 | 0.647 | – | – | – |
| Hunt & Reffert (2024) | 127.691 | -48.717 | 0.639 | -4.379 | 4.256 | 32.838 |
| UCC | 127.691 | -48.72 | 0.658 | -4.389 | 4.216 | 32.975 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.725, diffAV50=0.578, MOD50=10.767, logAge50=8.324 |
| Cavallo et al. (2024) | AV50=1.17, dMod50=10.95, logAge50=7.83, [Fe/H]50=-0.11 |
| Hunt & Reffert (2024) | MassJ=67.9199, MassTot=107.763 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 2328 | 20.0 | 128.08 | -49.41 | 0.6 | -4.34 | 4.15 | – | 0.21 |
