Collinder 417
(NGC 6885; MWSC 3282; 20 Vul; OCL 132)
0.58
UTI
0.0
CN
1.0
Cdens
0.5
CC3
0.69
Clit
1.0
Cdup
Stellar density (N50/rad)
8.8 [N/pc2]
- CN 0.0 Sparse
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.69 Moderately studied
- Cdup 1.0 Unique
Overview
Collinder 417 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~1.79 kpc) differs significantly from the median photometric distance (~1.02 kpc).
Note: This object shares a large 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 | 302.92 | 26.501 | 0.559 | -3.155 | -5.54 | 85.771 |
| Almeida et al. | 2025 | 302.983 | 26.494 | β | β | β | β |
| Just et al. | 2023 | 303.002 | 26.512 | β | β | β | β |
| Dias et al. | 2021 | 302.983 | 26.494 | 0.439 | -3.127 | -5.471 | 2.378 |
| SΓ‘nchez et al. | 2020 | 303.004 | 26.478 | β | -3.145 | -5.666 | β |
| Bica et al. | 2019 | 303.001 | 26.481 | β | β | β | β |
| Loktin & Popova | 2017 | 303.0 | 26.478 | β | -3.3 | -5.14 | -1.5 |
| Kharchenko et al. | 2016 | 303.002 | 26.512 | β | β | β | β |
| Dias et al. | 2014 | 303.004 | 26.478 | β | -3.3 | -5.14 | β |
| Kharchenko et al. | 2013 | 303.007 | 26.515 | β | -1.0 | -3.79 | -1.5 |
| Gozha et al. | 2012 | 303.004 | 26.478 | β | β | β | β |
| van den Bergh | 2006 | 303.0 | 26.483 | β | β | β | β |
| Dias et al. | 2002 | 303.004 | 26.478 | β | -3.3 | -5.14 | -1.5 |
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 | 1.025 | 1.93 | β | 1109 | 0.055 | 1848 | β | β |
| Almeida et al. | 2025 | 1.45 | 1.93 | β | 124 | β | 866 | β | β |
| Just et al. | 2023 | β | β | β | 1109 | β | 2831 | β | β |
| Dias et al. | 2021 | 1.45 | 1.93 | β | 124 | 0.055 | β | β | β |
| Loktin & Popova | 2017 | 0.44 | 0.46 | β | 462 | β | β | β | β |
| Kharchenko et al. | 2016 | 3.78 | 3.03 | β | 1109 | β | β | β | β |
| Kharchenko et al. | 2013 | 3.78 | 3.03 | β | 1109 | β | β | β | β |
| Gozha et al. | 2012 | 0.60 | β | β | 1445 | β | β | β | β |
| van den Bergh | 2006 | 0.60 | 0.25 | β | 1445 | β | β | β | β |
| Dias et al. | 2002 | 0.60 | 0.25 | β | 1445 | β | β | β | β |
MOCA

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.