NGC 6530
(M8)
0.95
UTI
1.0
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
264.0 [N/pc2]
- 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 2 later reported entries. 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 |
| Richer et al. | 2021 | 271.111 | -24.373 | 0.753 | 1.282 | -2.028 | 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 |
| Morales et al. | 2013 | 271.129 | -24.358 | β | β | β | 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 |
| Lada & Lada | 2003 | 271.966 | -24.326 | β | β | β | β |
| 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 | 1.03 | 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 |
| Richer et al. | 2021 | β | 0.93 | 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 |
| Morales et al. | 2013 | 1.30 | β | β | 2 | 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 |
| Lada & Lada | 2003 | 1.80 | β | β | β | 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 there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Part of multiple system G203, along with ESO_521-38, UBC_94, HSC_94 and Collinder_367.
Morales et al. (2013)
Classified as morphological type 'OC0' (emerging exposed cluster). Morphological flag: one or a few submm emission within the cluster area, but the submm emission is likely associated to the cluster, presence of emission related to PAH or warm dust.
Cavallo et al. (2024)
Bronze sample.
Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: intermediate fit.
Lada & Lada (2003)
Embedded cluster within βΌ2 Kpc of the Sun.