NGC 2430

(MWSC 1298)

Click to load Aladin Lite
0.19 UTI
0.0
CN
0.04
Cdens
0.12
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad) 0.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.4 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
NGC 2430 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.84 kpc) differs significantly from the median photometric distance (~0.71 kpc).

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 114.9 -16.412 0.261 -2.496 2.273 –
Just et al. 2023 114.911 -16.378 – – – –
Loktin & Popova 2017 114.915 -16.375 – -0.818 1.064 2.8
Kharchenko et al. 2016 114.911 -16.378 – – – –
Dias et al. 2014 114.921 -16.297 – -2.35 1.35 34.14
Kharchenko et al. 2013 114.916 -16.38 – -2.74 2.09 2.8
Piskunov et al. 2008 114.894 -16.348 – – – –
Kharchenko et al. 2005 114.9 -16.35 – -4.07 1.28 –

💡 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– 0.71 0.52 – 264 0.130 9 – –
Just et al. 2023 – – – 50 – 9 – –
Loktin & Popova 2017 1.91 0.00 – 813 – – – –
Kharchenko et al. 2016 0.71 0.52 – 50 – – – –
Kharchenko et al. 2013 0.71 0.52 – 50 0.130 – – –
Piskunov et al. 2008 0.65 0.53 – 479 – – – –
Kharchenko et al. 2005 0.65 0.53 – 479 – – – –

Visualization

â„šī¸