FSR 0282

(SAI 140; MWSC 3453)

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0.91 UTI
0.81
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
C3 classification AB
Number of members (P>50%) 255
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.81 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique
πŸ“₯ Members πŸ“Š Colab πŸ”¬ Bayestar19 πŸ” CDS πŸ” Simbad πŸ” CDS (Ξ±, Ξ΄) πŸ” Simbad (Ξ±, Ξ΄)

Overview
ℹ️
FSR 0282 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is very well-studied in the literature.
Distant High extinction Massive Near-solar metallicity Intermediate age

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

Cavallo et al. (2024)
Silver sample.

Data
πŸ” Search references for FSR 0282 in: SciX Simbad
ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 315.579 48.099 0.239 -3.65 -4.679 -44.761
Almeida et al. 2025 315.562 48.095 – – – –
Hunt & Reffert 2024 315.581 48.105 0.239 -3.653 -4.679 -44.773
Cavallo et al. 2024 315.562 48.101 0.244 – – –
Hunt & Reffert 2023 315.581 48.105 0.239 -3.653 -4.679 -44.773
Just et al. 2023 315.55 48.102 – – – –
Dias et al. 2021 315.562 48.095 0.222 -3.634 -4.644 –
Cantat-Gaudin et al. 2020 315.572 48.096 0.243 -3.64 -4.67 –
SΓ‘nchez et al. 2020 315.575 48.117 – -3.721 -4.492 –
Cantat-Gaudin & Anders 2020 315.572 48.096 0.243 -3.64 -4.67 –
Soubiran et al. 2018 315.572 48.096 – – – -43.99
Bica et al. 2019 315.575 48.115 – – – –
Cantat-Gaudin et al. 2018 315.572 48.096 0.243 -3.64 -4.67 –
Kharchenko et al. 2016 315.55 48.102 – – – –
Dias et al. 2014 315.575 48.117 – -4.85 -4.43 –
Kharchenko et al. 2013 315.555 48.105 – -2.23 1.44 –
Glushkova et al. 2010 315.584 48.107 – – – –
Froebrich et al. 2007 315.575 48.117 – – – –
Dias et al. 2002 315.575 48.117 – -4.85 -4.43 –

πŸ’‘ 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 3.08 3.91 – 458 – 1329 – –
Hunt & Reffert 2024 – – – – – 3355* – –
Cavallo et al. 2024 4.90 4.71 – 71 -0.080 – – –
Hunt & Reffert 2023 3.50 5.00 2.66 156 – – – –
Just et al. 2023 – – – 1738 – 288 – –
Dias et al. 2021 3.08 3.91 – 458 0.165 – – –
Cantat-Gaudin et al. 2020 4.13 3.61 – 347 – – – –
Cantat-Gaudin & Anders 2020 3.68 – – – – – – –
Soubiran et al. 2018 3.68 – – – – – – –
Cantat-Gaudin et al. 2018 3.68 – – – – – – –
Kharchenko et al. 2016 2.53 2.71 – 1738 – – – –
Kharchenko et al. 2013 2.53 2.71 – 1738 – – – –
Glushkova et al. 2010 2.28 2.42 – 1122 – – – –
Dias et al. 2002 2.53 2.71 – 1738 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization
ℹ️
FSR 0282 UCC
FSR 0282 HUNT23
FSR 0282 CANTAT20
Galactocentric position diagram