FSR 0336
(SAI 145; MWSC 3567)
0.86
UTI
0.83
CN
1.0
Cdens
1.0
CC3
0.74
Clit
1.0
Cdup
Nm (P>50%)
319
Core radius and density
2.4 [pc], 5.3 [pc-2]
- CN 0.83 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.74 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0336 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above 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 distance, age, metallicity, and mass parameters (see Parameters). It is moderately 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 327.711 | 55.239 | 0.38 | -3.036 | -2.893 | -15.516 |
| Li et al. | 2025 | 327.711 | 55.243 | 0.369 | -3.066 | -2.855 | â |
| Almeida et al. | 2025 | 327.713 | 55.24 | â | â | â | â |
| Hunt & Reffert | 2024 | 327.707 | 55.24 | 0.373 | -3.029 | -2.904 | 12.42 |
| Cavallo et al. | 2024 | 327.717 | 55.236 | 0.377 | â | â | â |
| Hunt & Reffert | 2023 | 327.707 | 55.24 | 0.373 | -3.029 | -2.904 | 12.42 |
| Just et al. | 2023 | 327.72 | 55.212 | â | â | â | â |
| Dias et al. | 2021 | 327.713 | 55.24 | 0.369 | -3.07 | -2.847 | -26.583 |
| Cantat-Gaudin et al. | 2020 | 327.711 | 55.243 | 0.369 | -3.066 | -2.855 | â |
| Cantat-Gaudin & Anders | 2020 | 327.711 | 55.243 | 0.369 | -3.066 | -2.855 | â |
| Soubiran et al. | 2018 | 327.711 | 55.243 | â | â | â | -27.32 |
| Bica et al. | 2019 | 327.713 | 55.242 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 327.711 | 55.243 | 0.369 | -3.066 | -2.855 | â |
| Dias et al. | 2018 | â | â | â | -5.63 | -2.91 | â |
| Dib et al. | 2018 | 327.726 | 55.215 | â | â | â | â |
| Loktin & Popova | 2017 | 327.705 | 55.246 | â | -4.511 | -3.377 | â |
| Sampedro et al. | 2017 | 327.712 | 55.246 | â | -1.72 | -6.26 | â |
| Joshi et al. | 2016 | 327.726 | 55.215 | â | â | â | â |
| Kharchenko et al. | 2016 | 327.72 | 55.212 | â | â | â | â |
| Kharchenko et al. | 2013 | 327.726 | 55.215 | â | -4.49 | -3.24 | â |
| Kharchenko et al. | 2012 | 327.726 | 55.215 | â | -4.49 | -3.24 | â |
| Glushkova et al. | 2010 | 327.698 | 55.275 | â | â | â | â |
| Froebrich et al. | 2007 | 327.712 | 55.246 | â | â | â | â |
| Dias et al. | 2002 | 327.712 | 55.246 | â | -5.74 | -7.21 | 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 | 2.31 | 2.21 | 2.34 | 596 | 0.038 | 1533 | â | â |
| Liu et al. | 2025 | 7.87 | 1.11 | â | 69 | â | â | â | â |
| Li et al. | 2025 | 0.94 | 1.04 | â | 7085 | -0.034 | â | â | â |
| Almeida et al. | 2025 | 2.31 | 3.00 | â | 12 | â | 1533 | â | â |
| Hunt & Reffert | 2024 | 2.45 | 3.29 | 2.34 | 47 | â | 2617(1) | â | â |
| Cavallo et al. | 2024 | 2.74 | 3.41 | â | 54 | 0.340 | â | â | â |
| Hunt & Reffert | 2023 | 2.45 | 3.29 | 2.34 | 47 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1259 | â | 46 | â | â |
| Dias et al. | 2021 | 2.31 | 3.00 | â | 12 | 0.038 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.67 | 2.74 | â | 48 | â | â | â | â |
| Kounkel et al. | 2020 | 2.83 | 3.49 | â | 155 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.51 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.51 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.51 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.12 | â | â | 1259 | â | â | â | â |
| Loktin & Popova | 2017 | 1.39 | 2.68 | â | 398 | â | â | â | â |
| Joshi et al. | 2016 | 1.12 | 1.58 | â | 1259 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.12 | 1.58 | â | 1259 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.12 | 1.58 | â | 1259 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.12 | 1.58 | â | 1259 | â | â | â | â |
| Glushkova et al. | 2010 | 2.16 | 1.74 | â | 794 | â | â | â | â |
| Dias et al. | 2002 | 1.12 | 1.58 | â | 1259 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 140 along with UBC_1147.
Palma et al. (2025)
Classified as genetic pair P214, along with UBC_1147.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.98 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.98 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.0442, e_all=0.0095.