HSC 1117
Summary
HSC 1117 is a poorly populated, moderately dense object of high C3 quality. It is located at a large distance from the Sun, well above the mid-plane. It was recently reported in the literature.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 50.107 | 65.055 | 0.155 | -0.317 | 0.171 | – |
| Cavallo et al. (2024) | 50.056 | 65.089 | 0.165 | – | – | – |
| Hunt & Reffert (2024) | 50.107 | 65.055 | 0.155 | -0.317 | 0.171 | – |
| UCC | 50.097 | 65.067 | 0.161 | -0.312 | 0.164 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=2.604, diffAV50=1.601, MOD50=13.749, logAge50=8.294 |
| Cavallo et al. (2024) | AV50=2.85, dMod50=13.39, logAge50=7.76, [Fe/H]50=0.05 |
| Hunt & Reffert (2024) | MassJ=525.440, MassTot=811.460 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3672 | 100.0 | 50.09 | 65.07 | 0.16 | -0.31 | 0.16 | -72.19 | 0.09 |
