Gulliver 52
Summary
Gulliver 52 is a moderately populated, very dense object of high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is well-studied in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Cantat-Gaudin et al. (2018) | 161.669 | -59.508 | 0.396 | -4.755 | 1.47 | – |
| Soubiran et al. (2018) | 161.669 | -59.508 | – | – | – | -11.33 |
| Cantat-Gaudin et al. (2020) | 161.669 | -59.508 | 0.396 | -4.755 | 1.47 | – |
| Dias et al. (2021) | 161.832 | -59.519 | 0.396 | -4.753 | 1.466 | – |
| Rain et al. (2021) | 161.669 | -59.508 | 0.396 | -4.755 | 1.47 | – |
| Hunt & Reffert (2023) | 161.607 | -59.485 | 0.408 | -4.749 | 1.506 | -17.609 |
| Cavallo et al. (2024) | 161.737 | -59.523 | 0.409 | – | – | – |
| Hunt & Reffert (2024) | 161.607 | -59.485 | 0.408 | -4.749 | 1.506 | -17.609 |
| Almeida et al. (2025) | 161.832 | -59.519 | – | – | – | – |
| UCC | 161.646 | -59.507 | 0.403 | -4.748 | 1.498 | -16.807 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Cantat-Gaudin et al. (2018) | dmode=2350.8 |
| Soubiran et al. (2018) | dmode=2350.8 |
| Cantat-Gaudin et al. (2020) | AVNN=1.04, DistPc=2482.0, AgeNN=8.68 |
| Dias et al. (2021) | Av=1.544, Dist=2087, logage=8.373, [Fe/H]=0.103 |
| Rain et al. (2021) | E(B-V)=0.5, Dist=2350.8, log(Age)=8.33, NBSS=0 |
| Hunt & Reffert (2023) | AV50=1.381, diffAV50=0.914, MOD50=11.734, logAge50=8.011 |
| Cavallo et al. (2024) | AV50=1.37, dMod50=11.8, logAge50=8.53, [Fe/H]50=0.2 |
| Hunt & Reffert (2024) | MassJ=369.401, MassTot=475.352 |
| Almeida et al. (2025) | AV=1.544, Dist=2087, logAge=8.373, MassRk=293.7 |
Search coordinates in Bayestar19