Loden 480
(MWSC 1986; OCL 865.3)
0.40
UTI
0.41
CN
0.12
Cdens
0.62
CC3
0.42
Clit
1.0
Cdup
Nm (P>50%)
41
Core radius and density
1.5 [pc], 0.6 [pc-2]
- CN 0.41 Poorly populated
- Cdens 0.12 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.42 Poorly studied
- Cdup 1.0 Unique
Overview
Loden 480 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a close* distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~0.74 kpc) differs significantly from the median photometric distance (~1.30 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 179.266 | -58.324 | 1.342 | -9.835 | -0.707 | -5.539 |
| Cavallo et al. | 2024 | 179.686 | -58.345 | 1.369 | â | â | â |
| Hunt & Reffert | 2023 | 179.317 | -58.3 | 1.363 | -9.848 | -0.687 | -7.488 |
| Just et al. | 2023 | 178.896 | -58.387 | â | â | â | â |
| Bica et al. | 2019 | 179.165 | -58.349 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -7.86 | 0.39 | â |
| Dib et al. | 2018 | 178.905 | -58.39 | â | â | â | â |
| Sampedro et al. | 2017 | 179.0 | -58.433 | â | â | â | â |
| Joshi et al. | 2016 | 178.905 | -58.39 | â | â | â | â |
| Kharchenko et al. | 2016 | 178.896 | -58.387 | â | â | â | â |
| Dias et al. | 2014 | 179.0 | -58.433 | â | -7.78 | 2.47 | â |
| Kharchenko et al. | 2013 | 178.905 | -58.39 | â | -9.03 | 4.4 | â |
| Piskunov et al. | 2008 | 178.988 | -58.401 | â | â | â | â |
| Kharchenko et al. | 2005 | 178.99 | -58.4 | â | -10.56 | 2.94 | â |
| Kharchenko et al. | 2003 | 178.99 | -58.4 | â | -8.55 | 5.73 | â |
| Lynga | 1987 | 179.013 | -58.434 | â | â | â | 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 | 1.3 | 0.665 | 0.49 | 501 | -0.010 | 101 | â | â |
| Cavallo et al. | 2024 | 0.73 | 0.67 | â | 347 | -0.010 | â | â | â |
| Hunt & Reffert | 2023 | 0.69 | 0.27 | 0.49 | 220 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 501 | â | 54 | â | â |
| Dib et al. | 2018 | 1.30 | â | â | 501 | â | â | â | â |
| Joshi et al. | 2016 | 1.30 | 0.66 | â | 501 | â | 148 | â | â |
| Kharchenko et al. | 2016 | 1.30 | 0.66 | â | 501 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.30 | 0.66 | â | 501 | â | â | â | â |
| Piskunov et al. | 2008 | 1.20 | 0.95 | â | 513 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.20 | 0.95 | â | 513 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.43 | 1.26 | â | â | â | â | â | â |
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as moving group. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).