NGC 2483

(MWSC 1383; OCL 677.1; ESO 430 02)

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0.35 UTI
0.0
CN
0.03
Cdens
0.5
CC3
0.61
Clit
1.0
Cdup
Nm (P>50%) 21
Core radius and density 4.3 [pc], 0.1 [pc-2]
C3 classification BB
  • CN 0.0 Sparse
  • Cdens 0.03 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.61 Moderately studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 MOCAMOCA 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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NGC 2483 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~4.08 kpc) differs significantly from the median photometric distance (~1.66 kpc).

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

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).

Data
🔍 Search references for NGC 2483 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 118.888 -28.001 0.245 -2.3 3.272 –
Hunt & Reffert 2024 118.879 -27.945 0.237 -2.285 3.255 –
Cavallo et al. 2024 118.907 -28.042 0.238 – – –
Hunt & Reffert 2023 118.879 -27.945 0.237 -2.285 3.255 –
Just et al. 2023 118.915 -27.902 – – – –
Bica et al. 2019 118.928 -27.897 – – – –
Dias et al. 2018 – – – -2.24 1.81 –
Dib et al. 2018 118.92 -27.905 – – – –
Loktin & Popova 2017 118.92 -27.894 – -2.714 0.133 121.51
Sampedro et al. 2017 118.912 -27.895 – -2.15 0.53 –
Joshi et al. 2016 118.92 -27.905 – – – –
Kharchenko et al. 2016 118.915 -27.902 – – – –
Dias et al. 2014 118.912 -27.895 – -2.01 0.55 121.51
Kharchenko et al. 2013 118.92 -27.905 – -1.0 2.45 –
Piskunov et al. 2008 118.903 -27.899 – – – –
van den Bergh 2006 118.9 -27.9 – – – –
Kharchenko et al. 2005 118.9 -27.9 – -2.24 1.55 –
Kharchenko et al. 2003 118.96 -27.91 – -2.18 1.64 –
Dias et al. 2002 118.912 -27.895 – -2.01 0.55 121.51
Dambis 1999 118.9 -27.9 – – – –
Lynga 1987 118.993 -27.933 – – – –
Sulentic et al. 1973 119.006 -27.934 – – – –

💡 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– 1.66 0.95 1.71 40 0.230 142 – –
Hunt & Reffert 2024 3.82 0.70 1.71 107 – 142(1) – –
Cavallo et al. 2024 3.37 0.64 – 186 0.230 – – –
Hunt & Reffert 2023 3.82 0.70 1.71 107 – – – –
Just et al. 2023 – – – 40 – 123 – –
Dib et al. 2018 1.65 – – 40 – – – –
Loktin & Popova 2017 1.73 0.88 – 19 – – – –
Joshi et al. 2016 1.65 1.12 – 40 – 380 – –
Kharchenko et al. 2016 1.65 1.12 – 40 – – – –
Kharchenko et al. 2013 1.65 1.12 – 40 – – – –
Piskunov et al. 2008 1.66 0.95 – 31 – – – –
van den Bergh 2006 1.66 0.95 – 12 – – – –
Kharchenko et al. 2005 1.66 0.95 – 31 – – – –
Kharchenko et al. 2003 1.67 0.95 – – – – – –
Dias et al. 2002 1.66 0.96 – 12 – – – –
Dambis 1999 2.01 1.43 – 3 – – – –
Lynga 1987 2.90 1.26 – 10 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1401 88.0 118.92 -28.06 0.24 -2.27 3.25 – 0.16

💡 Note: The % column shows the percentage of members that NGC 2483 shares with each listed object.

Visualization
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NGC 2483 UCC
NGC 2483 HUNT23
Galactocentric position diagram