NGC 1802
(MWSC 478)
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
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
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 77.53 | 24.169 | 0.166 | 0.489 | -0.661 | â |
| Just et al. | 2023 | 77.518 | 24.18 | â | â | â | â |
| Donor et al. | 2020 | 77.528 | 24.18 | â | 2.01 | -0.62 | 35.0 |
| Bica et al. | 2019 | 77.563 | 24.104 | â | â | â | â |
| Loktin & Popova | 2017 | 77.52 | 24.18 | â | 0.24 | -1.299 | â |
| Kharchenko et al. | 2016 | 77.518 | 24.18 | â | â | â | â |
| Dias et al. | 2014 | 77.558 | 24.108 | â | 1.99 | -0.82 | â |
| Kharchenko et al. | 2013 | 77.527 | 24.18 | â | 1.17 | -4.37 | â |
| Kharchenko et al. | 2012 | 77.527 | 24.18 | â | 1.17 | -4.37 | â |
| Piskunov et al. | 2008 | 77.562 | 24.14 | â | â | â | â |
| Kharchenko et al. | 2005 | 77.56 | 24.14 | â | -0.48 | -8.23 | â |
đĄ 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 | 99999â | 2.1 | 1.65 | â | 1413 | -0.300 | 286 | â | â |
| Just et al. | 2023 | â | â | â | 1413 | â | 286 | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.300 | â | â | â |
| Loktin & Popova | 2017 | 3.10 | 1.50 | â | 2042 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.10 | 1.80 | â | 1413 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.10 | 1.80 | â | 1413 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.10 | 1.80 | â | 1413 | â | â | â | â |
| Piskunov et al. | 2008 | 0.40 | 0.78 | â | 457 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.40 | 0.78 | â | 457 | â | â | â | â |
MOCA
