NGC 6530
0.95
UTI
1.0
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
4.0 [arcmin]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 6530 is a very rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 271.102 | -24.37 | 0.762 | 1.286 | -2.052 | 0.143 |
| Wei et al. | 2025 | 271.098 | -24.351 | 0.775 | 1.409 | -2.005 | β |
| Almeida et al. | 2025 | 271.109 | -24.357 | β | β | β | β |
| Hunt & Reffert | 2024 | 271.102 | -24.37 | 0.764 | 1.333 | -2.058 | 5.957 |
| Cavallo et al. | 2024 | 271.053 | -24.351 | 0.764 | β | β | β |
| Hunt & Reffert | 2023 | 271.102 | -24.37 | 0.764 | 1.333 | -2.058 | 5.957 |
| Jaehnig et al. | 2021 | 271.091 | -24.372 | 0.788 | 1.321 | -2.038 | β |
| Dias et al. | 2021 | 271.109 | -24.357 | 0.762 | 1.375 | -1.992 | β |
| SΓ‘nchez et al. | 2020 | 271.129 | -24.358 | β | 1.48 | -1.938 | β |
| Loktin & Popova | 2017 | 271.125 | -24.359 | β | 0.988 | -1.915 | -6.5 |
| Dias et al. | 2014 | 271.129 | -24.358 | β | 0.35 | -2.11 | β |
| Gozha et al. | 2012 | 271.129 | -24.358 | β | β | β | β |
| Piskunov et al. | 2008 | 271.111 | -24.364 | β | β | β | β |
| Kharchenko et al. | 2007 | 271.12 | -24.36 | β | 0.25 | β | -6.49 |
| van den Bergh | 2006 | 271.125 | -24.367 | β | β | β | β |
| Kharchenko et al. | 2005 | 271.12 | -24.36 | β | 2.01 | -1.81 | -13.32 |
| Kharchenko et al. | 2003 | 271.09 | -24.36 | β | 2.11 | -3.68 | β |
| Chen et al. | 2003 | 271.204 | -24.377 | β | 0.58 | -2.09 | -30.0 |
| Dias et al. | 2002 | 271.129 | -24.358 | β | 0.58 | -2.09 | -4.21 |
| Dambis | 1999 | 271.129 | -24.358 | β | β | β | β |
π‘ 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 | 99999β | 1.32 | 1.04 | 2.36 | 5 | 0.000 | 1148 | 0.62 | β |
| Wei et al. | 2025 | 1.70 | 1.66 | β | 7 | 0.000 | 1620 | 0.62 | β |
| Almeida et al. | 2025 | 1.21 | 1.16 | β | 5 | β | 328 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 2336(1) | β | β |
| Cavallo et al. | 2024 | 1.30 | 1.50 | β | 7 | -0.050 | β | β | β |
| Hunt & Reffert | 2023 | 1.24 | 1.48 | 2.36 | 4 | β | β | β | β |
| Jaehnig et al. | 2021 | 1.27(1) | β | β | β | β | β | β | β |
| Dias et al. | 2021 | 1.21 | 1.16 | β | 5 | 0.373 | β | β | β |
| Loktin & Popova | 2017 | 1.32 | 1.00 | β | 8 | β | β | β | β |
| Gozha et al. | 2012 | 1.33 | β | β | 7 | β | 676 | β | β |
| Piskunov et al. | 2008 | 1.32 | 0.93 | β | 5 | β | β | β | β |
| van den Bergh | 2006 | 1.33 | 1.02 | β | 7 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.32 | 0.93 | β | 5 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.33 | 0.87 | β | β | β | β | β | β |
| Chen et al. | 2003 | 1.33 | β | β | 0 | β | β | β | β |
| Dias et al. | 2002 | 1.33 | 1.03 | β | 7 | β | β | β | β |
| Dambis | 1999 | 1.27 | 1.05 | β | 3 | β | β | β | β |
(N): Indicates that are N extra values assigned to this parameter in the corresponding reference.


Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Bronze sample.