NGC 6910
(MWSC 3327)
0.91
UTI
0.82
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
5.3 [arcmin]
- CN 0.82 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 6910 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a 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 very small percentage of members with a later reported entry. See table with shared members information.
Relatively close
High extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 305.79 | 40.769 | 0.567 | -3.37 | -5.397 | -37.885 |
| Almeida et al. | 2025 | 305.789 | 40.767 | â | â | â | â |
| Hunt & Reffert | 2024 | 305.802 | 40.774 | 0.569 | -3.296 | -5.423 | -30.639 |
| Celli et al. | 2024 | 305.797 | 40.771 | â | â | â | â |
| Cavallo et al. | 2024 | 305.74 | 40.734 | 0.57 | â | â | â |
| Hunt & Reffert | 2023 | 305.802 | 40.774 | 0.569 | -3.296 | -5.423 | -30.639 |
| Almeida et al. | 2023 | 305.781 | 40.749 | â | â | â | â |
| Just et al. | 2023 | 305.807 | 40.792 | â | â | â | â |
| Jaehnig et al. | 2021 | 305.799 | 40.771 | 0.581 | -3.387 | -5.389 | â |
| Rain et al. | 2021 | 305.797 | 40.771 | 0.545 | -3.415 | -5.359 | â |
| Dias et al. | 2021 | 305.789 | 40.767 | 0.539 | -3.431 | -5.373 | â |
| Cantat-Gaudin et al. | 2020 | 305.797 | 40.771 | 0.545 | -3.415 | -5.359 | â |
| Cantat-Gaudin & Anders | 2020 | 305.797 | 40.771 | 0.545 | -3.415 | -5.359 | â |
| Soubiran et al. | 2018 | 305.797 | 40.771 | â | â | â | 14.97 |
| Cantat-Gaudin et al. | 2018 | 305.797 | 40.771 | 0.545 | -3.415 | -5.359 | â |
| Loktin & Popova | 2017 | 305.805 | 40.778 | â | -1.333 | -1.557 | -32.8 |
| Kharchenko et al. | 2016 | 305.807 | 40.792 | â | â | â | â |
| Dias et al. | 2014 | 305.8 | 40.778 | â | -2.46 | -6.02 | â |
| Kharchenko et al. | 2013 | 305.812 | 40.795 | â | -4.27 | -5.72 | -32.8 |
| Gozha et al. | 2012 | 305.8 | 40.778 | â | â | â | â |
| Piskunov et al. | 2008 | 305.802 | 40.774 | â | â | â | â |
| Kharchenko et al. | 2007 | 305.8 | 40.78 | â | 0.17 | â | -32.76 |
| van den Bergh | 2006 | 305.783 | 40.775 | â | â | â | â |
| Kharchenko et al. | 2005 | 305.8 | 40.78 | â | -3.89 | -4.93 | -32.76 |
| Kharchenko et al. | 2003 | 305.77 | 40.77 | â | -3.94 | -4.86 | â |
| Chen et al. | 2003 | 305.828 | 40.785 | â | -3.66 | -5.33 | -30.0 |
| Dias et al. | 2002 | 305.8 | 40.778 | â | -2.46 | -6.02 | -31.57 |
| Dambis | 1999 | 305.783 | 40.775 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 1.72 | 3.15 | â | 9 | â | 734 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2155* | â | â |
| Celli et al. | 2024 | â | â | â | 14 | â | 1194 | â | â |
| Cavallo et al. | 2024 | 1.68 | 3.40 | â | 19 | 0.900 | â | â | â |
| Hunt & Reffert | 2023 | 1.69 | 3.83 | 2.89 | 15 | â | â | â | â |
| Almeida et al. | 2023 | 1.64 | 3.31 | â | 10 | -0.030 | 1528* | 0.74 | â |
| Just et al. | 2023 | â | â | â | 34 | â | 26 | â | â |
| Jaehnig et al. | 2021 | 1.73* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.74 | 3.01 | â | 13 | â | â | â | 0 |
| Dias et al. | 2021 | 1.72 | 3.15 | â | 9 | 0.035 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.73 | 2.83 | â | 13 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.74 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 1.74 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.74 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.21 | 3.06 | â | 12 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.13 | 3.23 | â | 34 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.13 | 3.23 | â | 34 | â | â | â | â |
| Gozha et al. | 2012 | 1.14 | â | â | 13 | â | 209 | â | â |
| Piskunov et al. | 2008 | 1.14 | 3.01 | â | 21 | â | â | â | â |
| van den Bergh | 2006 | 1.14 | 3.01 | â | 13 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.14 | 3.01 | â | 21 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.14 | 3.01 | â | â | â | â | â | â |
| Chen et al. | 2003 | 1.14 | â | â | 10 | â | â | â | â |
| Dias et al. | 2002 | 1.14 | 3.01 | â | 13 | â | â | â | â |
| Dambis | 1999 | 1.43 | 3.25 | â | 3 | 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: intermediate fit. Silver sample.
Cavallo et al. (2024)
Silver sample.