Melotte 93

(Collinder 200; VDBH 50; NGC 2670; MWSC 1554; OCL 764; vdBergh-Hagen 50; ESO 210 05; FoF 694)

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0.92 UTI
0.83
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad) 35.3 [N/pc2]
  • CN 0.83 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

ℹ️
Melotte 93 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close 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 very well-studied in the literature.

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

Cavallo et al. (2024)
Gold sample.

Data

ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 131.388 -48.797 0.666 -5.356 3.667 19.38
Li et al. 2025 131.386 -48.801 0.647 -5.379 3.621 –
Wei et al. 2025 131.401 -48.803 0.657 -5.37 3.723 –
Almeida et al. 2025 131.375 -48.81 – – – –
Hunt & Reffert 2024 131.369 -48.791 0.666 -5.36 3.678 14.814
Cavallo et al. 2024 131.374 -48.812 0.668 – – –
Hunt & Reffert 2023 131.369 -48.791 0.666 -5.36 3.678 14.814
Almeida et al. 2023 131.395 -48.783 – – – –
Just et al. 2023 131.388 -48.817 – – – –
Tarricq et al. 2022 131.404 -48.801 0.661 -5.349 3.692 –
Jaehnig et al. 2021 131.386 -48.796 0.681 -5.379 3.599 –
Rain et al. 2021 131.386 -48.801 0.647 -5.379 3.621 –
Dias et al. 2021 131.375 -48.81 0.651 -5.381 3.606 –
Cantat-Gaudin et al. 2020 131.386 -48.801 0.647 -5.379 3.621 –
SΓ‘nchez et al. 2020 131.375 -48.8 – -5.356 3.635 –
Cantat-Gaudin & Anders 2020 131.386 -48.801 0.647 -5.379 3.621 –
Liu & Pang 2019 131.375 -48.795 0.653 -5.392 3.606 –
Soubiran et al. 2018 131.386 -48.801 – – – 5.15
Bica et al. 2019 131.385 -48.8 – – – –
Cantat-Gaudin et al. 2018 131.386 -48.801 0.647 -5.379 3.621 –
Loktin & Popova 2017 131.37 -48.8 – -6.15 5.74 17.2
Kharchenko et al. 2016 131.388 -48.817 – – – –
Dias et al. 2014 131.375 -48.8 – -6.15 5.74 –
Kharchenko et al. 2013 131.392 -48.82 – -11.95 6.2 17.2
Gozha et al. 2012 131.375 -48.8 – – – –
Piskunov et al. 2008 131.364 -48.799 – – – –
van den Bergh 2006 131.375 -48.8 – – – –
Kharchenko et al. 2005 131.37 -48.8 – -11.97 4.86 –
Kharchenko et al. 2003 131.38 -48.78 – -11.05 3.98 –
Dias et al. 2002 131.375 -48.8 – -6.15 5.74 17.2

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] Bfrac BSS
UCC 99999– 1.41 1.33 1.81 114 0.277 682 0.435 0.0
Li et al. 2025 1.21 1.16 – 253 -0.254 – – –
Wei et al. 2025 2.44 1.46 – 407 0.250 1054 0.34 –
Almeida et al. 2025 1.47 1.31 – 93 – 802 – –
Hunt & Reffert 2024 – – – – – 1147(1) – –
Cavallo et al. 2024 1.56 1.25 – 191 0.620 – – –
Hunt & Reffert 2023 1.41 1.50 1.81 105 – – – –
Almeida et al. 2023 1.39 1.42 – 125 0.148 562(1) 0.53 –
Just et al. 2023 – – – 138 – 28 – –
Tarricq et al. 2022 1.46 – – 123 – – – –
Jaehnig et al. 2021 1.47(1) – – – – – – –
Rain et al. 2021 1.48 1.33 – 49 – – – 0
Dias et al. 2021 1.47 1.31 – 93 0.304 – – –
Cantat-Gaudin et al. 2020 1.51 1.08 – 102 – – – –
Cantat-Gaudin & Anders 2020 1.48 – – – – – – –
Liu & Pang 2019 – – – 63 0.500 – – –
Soubiran et al. 2018 1.48 – – – – – – –
Cantat-Gaudin et al. 2018 1.48 – – – – – – –
Loktin & Popova 2017 1.19 1.33 – 49 – – – –
Kharchenko et al. 2016 1.29 1.35 – 138 – – – –
Kharchenko et al. 2013 1.29 1.35 – 138 – – – –
Gozha et al. 2012 1.19 – – 49 – 44 – –
Piskunov et al. 2008 1.19 1.33 – 126 – – – –
van den Bergh 2006 1.19 1.33 – 49 – – – –
Kharchenko et al. 2005 1.19 1.33 – 126 – – – –
Kharchenko et al. 2003 1.12 1.05 – – – – – –
Dias et al. 2002 1.19 1.33 – 49 – – – –

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

Visualization

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