Gulliver 53
0.69
UTI
0.57
CN
0.95
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Stellar density (N50/rad)
4.8 [N/pc2]
- CN 0.57 Moderately populated
- Cdens 0.95 Very dense
- CC3 0.75 High quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
Gulliver 53 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 80.986 | 34.008 | 0.381 | 0.395 | -2.869 | 1.114 |
| Almeida et al. | 2025 | 81.004 | 34.017 | â | â | â | â |
| Zhang et al. | 2024 | 81.009 | 34.05 | â | â | â | â |
| Hunt & Reffert | 2024 | 81.009 | 34.05 | 0.371 | 0.393 | -2.873 | 1.095 |
| Cavallo et al. | 2024 | 80.973 | 34.015 | 0.372 | â | â | â |
| Hunt & Reffert | 2023 | 81.009 | 34.05 | 0.371 | 0.393 | -2.873 | 1.095 |
| Dias et al. | 2021 | 81.004 | 34.017 | 0.375 | 0.388 | -2.872 | â |
| Cantat-Gaudin et al. | 2020 | 80.975 | 34.012 | 0.384 | 0.401 | -2.837 | â |
| Zhong et al. | 2020 | 80.975 | 34.012 | â | 0.401 | -2.837 | 30.031 |
| Cantat-Gaudin & Anders | 2020 | 80.975 | 34.012 | 0.384 | 0.401 | -2.837 | â |
| Monteiro & Dias | 2019 | 80.975 | 34.012 | â | â | â | 2.59 |
| Cantat-Gaudin et al. | 2018 | 80.975 | 34.012 | 0.384 | 0.401 | -2.837 | â |
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 | 2.27 | 1.46 | 0.87 | 144 | 0.000 | 267 | â | â |
| Almeida et al. | 2025 | 2.19 | 1.46 | â | 213 | â | 124 | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.056(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 410(1) | â | â |
| Cavallo et al. | 2024 | 2.25 | 1.56 | â | 195 | -0.020 | â | â | â |
| Hunt & Reffert | 2023 | 2.37 | 1.35 | 0.87 | 144 | â | â | â | â |
| Dias et al. | 2021 | 2.19 | 1.46 | â | 213 | -0.072 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.43 | 0.96 | â | 129 | â | â | â | â |
| Zhong et al. | 2020 | 0.00 | 0.00 | â | 0 | 0.000 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.42 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 2.27 | 1.60 | â | 115 | 0.004 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.42 | â | â | â | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Piecka & Paunzen (2021)
Belongs to cluster aggregate 'Agg17' along with COIN-Gaia 40, Kronberger 1, NGC 1893 and Stock 8.
Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.