NGC 6800
(MWSC 3124; OCL 123; FoF 2340)
0.93
UTI
0.67
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
10.2 [arcmin]
- CN 0.67 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 6800 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is very well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 291.699 | 25.079 | 0.951 | 0.444 | -0.87 | -16.456 |
| Li et al. | 2025 | 291.664 | 25.008 | 0.953 | 0.438 | -0.876 | â |
| Almeida et al. | 2025 | 291.677 | 25.034 | â | â | â | â |
| Hunt & Reffert | 2024 | 291.761 | 25.163 | 0.934 | 0.42 | -0.878 | -18.339 |
| Cavallo et al. | 2024 | 291.707 | 25.05 | 0.942 | â | â | â |
| Hunt & Reffert | 2023 | 291.761 | 25.163 | 0.934 | 0.42 | -0.878 | -18.339 |
| Just et al. | 2023 | 291.76 | 25.122 | â | â | â | â |
| He et al. | 2022 | 291.719 | 25.111 | 0.953 | 0.445 | -0.855 | â |
| Tarricq et al. | 2022 | 291.692 | 25.065 | 0.953 | 0.429 | -0.865 | â |
| Dias et al. | 2021 | 291.677 | 25.034 | 0.953 | 0.425 | -0.879 | â |
| Cantat-Gaudin et al. | 2020 | 291.664 | 25.008 | 0.953 | 0.438 | -0.876 | â |
| Cantat-Gaudin & Anders | 2020 | 291.664 | 25.008 | 0.953 | 0.438 | -0.876 | â |
| Liu & Pang | 2019 | 291.699 | 25.111 | 0.951 | 0.47 | -0.828 | â |
| Bossini et al. | 2019 | 291.664 | 25.008 | â | â | â | â |
| Soubiran et al. | 2018 | 291.664 | 25.008 | â | â | â | -13.29 |
| Bica et al. | 2019 | 291.756 | 25.155 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 291.664 | 25.008 | 0.953 | 0.438 | -0.876 | â |
| Loktin & Popova | 2017 | 291.765 | 25.125 | â | -2.341 | -5.235 | â |
| Kharchenko et al. | 2016 | 291.76 | 25.122 | â | â | â | â |
| Dias et al. | 2014 | 291.779 | 25.14 | â | -0.53 | -3.27 | â |
| Kharchenko et al. | 2013 | 291.765 | 25.125 | â | 1.05 | 0.86 | â |
| Piskunov et al. | 2008 | 291.771 | 25.137 | â | â | â | â |
| Kharchenko et al. | 2005 | 291.78 | 25.14 | â | 1.65 | 4.27 | â |
| Kharchenko et al. | 2003 | 291.78 | 25.14 | â | 1.88 | 4.12 | â |
| Dias et al. | 2002 | 291.779 | 25.14 | â | -0.53 | -3.27 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.00 | 0.99 | â | 459 | 0.257 | â | â | â |
| Almeida et al. | 2025 | 1.06 | 1.15 | â | 313 | â | 117 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 486* | â | â |
| Cavallo et al. | 2024 | 1.03 | 1.24 | â | 372 | 0.280 | â | â | â |
| Hunt & Reffert | 2023 | 1.01 | 1.07 | 0.88 | 284 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 363 | â | 83 | â | â |
| He et al. | 2022 | â | 1.40 | â | 282 | â | â | â | â |
| Tarricq et al. | 2022 | 0.98 | â | â | 437 | â | â | â | â |
| Dias et al. | 2021 | 1.06 | 1.15 | â | 313 | 0.387 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.01 | 0.83 | â | 407 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.02 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 437 | 0.000 | â | â | â |
| Bossini et al. | 2019 | 1.12 | 1.08 | â | 346 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 1.02 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.02 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.35 | 0.88 | â | 224 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.08 | 1.24 | â | 363 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.08 | 1.24 | â | 363 | â | â | â | â |
| Piskunov et al. | 2008 | 1.00 | 1.24 | â | 389 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.00 | 1.24 | â | 389 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.00 | 0.31 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.00 | 1.24 | â | 389 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.