FSR 0850

(MWSC 662; FoF 77; LISC 0122)

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0.78 UTI
0.79
CN
0.81
Cdens
0.75
CC3
0.77
Clit
1.0
Cdup
Core radius and density 2.5 [pc], 4.1 [pc-2]
  • CN 0.79 Rich
  • Cdens 0.81 Dense
  • CC3 0.75 High quality
  • Clit 0.77 Well-studied
  • Cdup 1.0 Unique

Overview

â„šī¸
FSR 0850 is a rich, dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is well-studied in the literature.

Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.

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

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.91 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.91 (50th percentile).

Hu et al. (2021)
Ellipticities (core, all): e_core=0.1287, e_all=0.2437.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 86.261 24.744 0.444 1.263 -2.528 18.599
Hu & Soubiran 2025 86.273 24.761 – – – –
Almeida et al. 2025 86.266 24.744 – – – –
Zhang et al. 2024 86.241 24.745 – – – –
Hunt & Reffert 2024 86.241 24.745 0.447 1.248 -2.524 15.209
Cavallo et al. 2024 86.274 24.761 0.446 – – –
Hunt & Reffert 2023 86.241 24.745 0.447 1.248 -2.524 15.209
Almeida et al. 2023 86.278 24.753 – – – –
Just et al. 2023 86.271 24.739 – – – –
Jadhav & Subramaniam 2021 86.257 24.74 – – – –
Dias et al. 2021 86.266 24.744 0.441 1.296 -2.57 16.987
Cantat-Gaudin et al. 2020 86.257 24.74 0.438 1.301 -2.555 –
Zhong et al. 2020 86.257 24.74 – 1.301 -2.555 17.289
Cantat-Gaudin & Anders 2020 86.257 24.74 0.438 1.301 -2.555 –
Liu & Pang 2019 86.269 24.76 0.461 1.237 -2.491 –
Dias et al. 2019 86.312 24.754 0.456 1.286 -2.518 19.37
Soubiran et al. 2018 86.257 24.74 – – – 19.24
Cantat-Gaudin et al. 2018 86.257 24.74 0.438 1.301 -2.555 –
Dib et al. 2018 86.28 24.738 – – – –
Sampedro et al. 2017 86.312 24.754 – -1.07 0.58 –
Kharchenko et al. 2016 86.271 24.739 – – – –
Kharchenko et al. 2013 86.28 24.738 – 0.07 -3.88 -17.0
Camargo et al. 2012 86.312 24.754 – – – –
Froebrich et al. 2007 86.312 24.754 – – – –
Dias et al. 2002 86.312 24.754 – 0.07 -3.88 –

💡 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 99999– 2.04 1.74 2.28 263 -0.160 513 0.62 0
Hu & Soubiran 2025 – – – – -0.160(5) – – –
Almeida et al. 2025 1.92 1.78 – 219 – 470 – –
Zhang et al. 2024 – – – – -0.278(1) – – –
Hunt & Reffert 2024 2.04 1.57 2.28 376 – 1172(1) – –
Cavallo et al. 2024 2.07 1.72 – 537 0.080 – – –
Hunt & Reffert 2023 2.04 1.57 2.28 377 – – – –
Almeida et al. 2023 1.89 1.71 – 377 -0.099 513(1) 0.62 –
Deng & Li 2023 1.91 1.76 – 500 -0.136 – – –
Just et al. 2023 – – – 20 – 139 – –
Jadhav & Subramaniam 2021 2.23 1.29 – 468 – 881 – 0(1)
Dias et al. 2021 1.92 1.78 – 219 -0.086 – – –
Cantat-Gaudin et al. 2020 2.23 1.29 – 468 – – – –
Kounkel et al. 2020 2.25 1.80 – 263 – – – –
Zhong et al. 2020 2.14(1) 1.51 – 9000 -0.185 – – –
Cantat-Gaudin & Anders 2020 2.14 – – – – – – –
Liu & Pang 2019 – – – 1150 -0.500 – – –
Dias et al. 2019 1.86 1.51 – 37 -0.881 – – –
Soubiran et al. 2018 2.14 – – – – – – –
Cantat-Gaudin et al. 2018 2.14 – – – – – – –
Dib et al. 2018 1.84 – – 20 – – – –
Kharchenko et al. 2016 1.84 1.77 – 20 – – – –
Kharchenko et al. 2013 1.84 1.77 – 20 – – – –
Camargo et al. 2012 2.75 2.18 – 10 – – – –
Dias et al. 2002 1.84 1.77 – 20 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0299 15.6 86.26 24.75 0.47 1.25 -2.53 18.65 0.0

💡 Note: The % column shows the percentage of members that FSR 0850 shares with each listed object.

Visualization

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