NGC 1802

(MWSC 478)

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0.30 UTI
0.0
CN
0.02
Cdens
0.38
CC3
0.56
Clit
1.0
Cdup
Stellar density (N50/rad) 0.1 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.38 Low quality
  • Clit 0.56 Moderately studied
  • Cdup 1.0 Unique

Overview

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NGC 1802 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~6.04 kpc) differs significantly from the median photometric distance (~2.10 kpc).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 77.53 24.169 0.166 0.489 -0.661 –
Just et al. 2023 77.518 24.18 – – – –
Donor et al. 2020 77.528 24.18 – 2.01 -0.62 35.0
Bica et al. 2019 77.563 24.104 – – – –
Loktin & Popova 2017 77.52 24.18 – 0.24 -1.299 –
Kharchenko et al. 2016 77.518 24.18 – – – –
Dias et al. 2014 77.558 24.108 – 1.99 -0.82 –
Kharchenko et al. 2013 77.527 24.18 – 1.17 -4.37 –
Kharchenko et al. 2012 77.527 24.18 – 1.17 -4.37 –
Piskunov et al. 2008 77.562 24.14 – – – –
Kharchenko et al. 2005 77.56 24.14 – -0.48 -8.23 –

💡 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– 2.1 1.65 – 1413 -0.300 286 – –
Just et al. 2023 – – – 1413 – 286 – –
Donor et al. 2020 – – – – -0.300 – – –
Loktin & Popova 2017 3.10 1.50 – 2042 – – – –
Kharchenko et al. 2016 2.10 1.80 – 1413 – – – –
Kharchenko et al. 2013 2.10 1.80 – 1413 – – – –
Kharchenko et al. 2012 2.10 1.80 – 1413 – – – –
Piskunov et al. 2008 0.40 0.78 – 457 – – – –
Kharchenko et al. 2005 0.40 0.78 – 457 – – – –

Visualization

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