NGC 5999
(Melotte 137; Collinder 293; VDBH 178; MWSC 2326; OCL 946; vdBergh-Hagen 178; ESO 178 01; FSR 1706)
0.95
UTI
0.9
CN
1.0
Cdens
1.0
CC3
0.94
Clit
1.0
Cdup
Stellar density (N50/rad)
72.6 [N/pc2]
- CN 0.9 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.94 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 5999 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 238.045 | -56.483 | 0.345 | -3.411 | -4.22 | -31.119 |
| Li et al. | 2025 | 238.046 | -56.482 | 0.326 | -3.389 | -4.216 | â |
| Almeida et al. | 2025 | 238.047 | -56.482 | â | â | â | â |
| Hunt & Reffert | 2024 | 238.044 | -56.479 | 0.349 | -3.421 | -4.211 | -33.152 |
| Cavallo et al. | 2024 | 238.049 | -56.486 | 0.348 | â | â | â |
| Hunt & Reffert | 2023 | 238.044 | -56.479 | 0.349 | -3.421 | -4.211 | -33.152 |
| Almeida et al. | 2023 | 238.048 | -56.484 | â | â | â | â |
| Just et al. | 2023 | 238.031 | -56.466 | â | â | â | â |
| Jaehnig et al. | 2021 | 238.054 | -56.481 | 0.36 | -3.372 | -4.226 | â |
| Rain et al. | 2021 | 238.046 | -56.482 | 0.326 | -3.389 | -4.216 | â |
| Dias et al. | 2021 | 238.047 | -56.482 | 0.329 | -3.389 | -4.21 | -30.883 |
| Cantat-Gaudin et al. | 2020 | 238.046 | -56.482 | 0.326 | -3.389 | -4.216 | â |
| Cantat-Gaudin & Anders | 2020 | 238.046 | -56.482 | 0.326 | -3.389 | -4.216 | â |
| Soubiran et al. | 2018 | 238.046 | -56.482 | â | â | â | -30.78 |
| Bica et al. | 2019 | 238.03 | -56.468 | â | â | â | â |
| Ferreira et al. | 2019 | 238.047 | -56.488 | â | -3.374 | -4.216 | â |
| Cantat-Gaudin et al. | 2018 | 238.046 | -56.482 | 0.326 | -3.389 | -4.216 | â |
| Dias et al. | 2018 | â | â | â | -3.15 | -4.08 | â |
| Dib et al. | 2018 | 238.042 | -56.467 | â | â | â | â |
| Sampedro et al. | 2017 | 238.033 | -56.473 | -1.47 | -3.25 | â | â |
| Joshi et al. | 2016 | 238.042 | -56.467 | â | â | â | â |
| Kharchenko et al. | 2016 | 238.031 | -56.466 | â | â | â | â |
| Netopil et al. | 2016 | 238.043 | -56.467 | â | â | â | â |
| Dias et al. | 2014 | 238.033 | -56.473 | â | -0.72 | -2.79 | â |
| Kharchenko et al. | 2013 | 238.042 | -56.467 | â | 0.8 | 0.25 | â |
| Ahumada & Lapasset | 2007 | 238.05 | -56.483 | â | â | â | â |
| van den Bergh | 2006 | 238.05 | -56.467 | â | â | â | â |
| Dias et al. | 2002 | 238.033 | -56.473 | â | -0.72 | -2.74 | â |
| Lynga | 1987 | 238.056 | -56.47 | â | â | â | â |
| van den Bergh & Hagen | 1975 | 237.05 | -56.317 | â | â | â | â |
| Sulentic et al. | 1973 | 238.048 | -56.491 | â | â | â | 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 | 2.29 | 1.545 | 1.39 | 398 | 0.070 | 1144 | 0.6 | 2 |
| Li et al. | 2025 | 2.24 | 1.59 | â | 468 | 0.061 | â | â | â |
| Almeida et al. | 2025 | 2.19 | 1.87 | â | 196 | â | 1086 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 4448(1) | â | â |
| Cavallo et al. | 2024 | 2.42 | 2.12 | â | 219 | 0.140 | â | â | â |
| Hunt & Reffert | 2023 | 2.56 | 1.78 | 1.39 | 137 | â | â | â | â |
| Almeida et al. | 2023 | 2.29 | 1.94 | â | 163 | 0.135 | 1203(1) | 0.60 | â |
| Just et al. | 2023 | â | â | â | 398 | â | 102 | â | â |
| Jaehnig et al. | 2021 | 2.80(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 2.81 | 1.42 | â | 398 | â | â | â | 0 |
| Dias et al. | 2021 | 2.19 | 1.87 | â | 196 | 0.079 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.75 | 1.40 | â | 200 | â | â | â | â |
| Kounkel et al. | 2020 | 2.81 | 1.50 | â | 347 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.81 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.81 | â | â | â | â | â | â | â |
| Ferreira et al. | 2019 | 1.82 | 2.02 | â | 316 | -0.200 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.81 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.63 | â | â | 398 | â | â | â | â |
| Joshi et al. | 2016 | 1.63 | 1.38 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.63 | 1.38 | â | 398 | â | â | â | â |
| Netopil et al. | 2016 | 6.39 | â | â | 400 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.63 | 1.38 | â | 398 | â | â | â | â |
| Ahumada & Lapasset | 2007 | â | 1.96 | â | 251 | â | â | â | 4 |
| van den Bergh | 2006 | 2.05 | 1.42 | â | 398 | â | â | â | â |
| Dias et al. | 2002 | 2.05 | 1.42 | â | 398 | 0.000 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Ahumada & Lapasset (2007)
All the cluster parameters except the apparent diameter are from (2005, unpublished data). The diagram up to 2.5' from the cluster centre was examined.