Melotte 48

(Collinder 108; NGC 2259; MWSC 940; OCL 492; FoF 370)

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0.90 UTI
0.77
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad) 56.7 [N/pc2]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Melotte 48 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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 metallicity parameter (see Parameters). It is very well-studied in the literature.

Note: This object contains blue stragglers according to at least one source.

Note: This object shares a small percentage of members with 2 later reported entries. See table with shared members information.

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

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 99.637 10.884 0.328 -0.231 -1.097 64.761
Li et al. 2025 99.633 10.885 0.326 -0.273 -1.032 –
Hu & Soubiran 2025 99.633 10.884 – – – –
Almeida et al. 2025 99.621 10.886 – – – –
Zhang et al. 2024 99.639 10.881 – – – –
Hunt & Reffert 2024 99.639 10.881 0.31 -0.237 -1.086 80.409
Cavallo et al. 2024 99.633 10.884 0.309 – – –
Hunt & Reffert 2023 99.639 10.881 0.31 -0.237 -1.086 80.409
Almeida et al. 2023 99.623 10.881 – – – –
Just et al. 2023 99.625 10.876 – – – –
Jaehnig et al. 2021 99.638 10.876 0.376 -0.245 -1.128 –
Rain et al. 2021 99.633 10.885 0.326 -0.273 -1.032 –
Dias et al. 2021 99.621 10.886 0.308 -0.266 -1.062 –
Cantat-Gaudin et al. 2020 99.633 10.885 0.326 -0.273 -1.032 –
Cantat-Gaudin & Anders 2020 99.633 10.885 0.326 -0.273 -1.032 –
Liu & Pang 2019 99.632 10.889 0.328 -0.257 -1.045 –
Soubiran et al. 2018 99.633 10.885 – – – 65.86
Bica et al. 2019 99.637 10.888 – – – –
Cantat-Gaudin et al. 2018 99.633 10.885 0.326 -0.273 -1.032 –
Loktin & Popova 2017 99.63 10.884 – 0.877 -0.715 –
Kharchenko et al. 2016 99.625 10.876 – – – –
Dias et al. 2014 99.587 10.883 – 2.79 -0.96 –
Kharchenko et al. 2013 99.633 10.875 – 2.66 -2.38 –
Gozha et al. 2012 99.588 10.883 – – – –
van den Bergh 2006 99.643 10.89 – – – –
Chen et al. 2003 99.582 10.883 – – – –
Dias et al. 2002 99.588 10.883 – 2.79 -0.96 –

💡 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– 2.82 1.83 1.18 337 0.070 880 0.55 4.0
Li et al. 2025 2.63 1.64 – 742 -0.152 – – –
Hu & Soubiran 2025 – – – – -0.240(5) – – –
Almeida et al. 2025 2.34 1.85 – 337 – 645 – –
Zhang et al. 2024 – – – – 0.237(1) – – –
Hunt & Reffert 2024 – – – – – 1114(1) – –
Cavallo et al. 2024 2.58 1.60 – 603 0.350 – – –
Hunt & Reffert 2023 2.78 1.66 1.18 350 – – – –
Almeida et al. 2023 2.62 2.00 – 316 -0.160 406(1) 0.55 –
Just et al. 2023 – – – 422 – 1197 – –
Jaehnig et al. 2021 2.68(1) – – – – – – –
Rain et al. 2021 2.82 1.83 – 316 – – – 4
Dias et al. 2021 2.34 1.85 – 337 -0.152 – – –
Cantat-Gaudin et al. 2020 3.01 1.52 – 275 – – – –
Cantat-Gaudin & Anders 2020 2.82 – – – – – – –
Liu & Pang 2019 – – – 603 0.500 – – –
Soubiran et al. 2018 2.82 – – – – – – –
Cantat-Gaudin et al. 2018 2.82 – – – – – – –
Loktin & Popova 2017 2.19 1.47 – 166 – – – –
Kharchenko et al. 2016 3.06 2.13 – 422 – – – –
Kharchenko et al. 2013 3.06 2.13 – 422 0.070 – – –
Gozha et al. 2012 3.31 – – 316 0.070 – – –
van den Bergh 2006 3.31 1.83 – 316 – – – –
Chen et al. 2003 3.31 1.83 – 320 0.070(1) – – –
Dias et al. 2002 3.31 1.83 – 316 0.070 – – –

(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 0334 15.5 99.64 10.88 0.34 -0.2 -1.09 – 0.0
OC 0335 14.9 99.65 10.88 0.41 -0.2 -0.98 64.76 0.01

💡 Note: The % column shows the percentage of members that Melotte 48 shares with each listed object.

Visualization

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