NGC 103
(Collinder 1; MWSC 40; OCL 291; FSR 0491)
0.97
UTI
0.84
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Nm (P>50%)
343
Core radius and density
1.9 [pc], 8.3 [pc-2]
- CN 0.84 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 103 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is very well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 6.309 | 61.327 | 0.283 | -2.81 | -1.059 | -77.089 |
| Li et al. | 2025 | 6.312 | 61.326 | 0.288 | -2.823 | -0.988 | β |
| Almeida et al. | 2025 | 6.321 | 61.327 | β | β | β | β |
| Hunt & Reffert | 2024 | 6.311 | 61.326 | 0.286 | -2.815 | -1.066 | -75.123 |
| Cavallo et al. | 2024 | 6.336 | 61.325 | 0.284 | β | β | β |
| Hunt & Reffert | 2023 | 6.311 | 61.326 | 0.286 | -2.815 | -1.066 | -75.123 |
| Almeida et al. | 2023 | 6.319 | 61.325 | β | β | β | β |
| Just et al. | 2023 | 6.26 | 61.337 | β | β | β | β |
| Jaehnig et al. | 2021 | 6.312 | 61.325 | 0.325 | -2.827 | -1.001 | β |
| Rain et al. | 2021 | 6.312 | 61.326 | 0.288 | -2.823 | -0.988 | β |
| Dias et al. | 2021 | 6.321 | 61.327 | 0.289 | -2.829 | -0.978 | -78.897 |
| Cantat-Gaudin et al. | 2020 | 6.312 | 61.326 | 0.288 | -2.823 | -0.988 | β |
| SΓ‘nchez et al. | 2020 | 6.317 | 61.323 | β | -3.162 | -1.027 | β |
| Cantat-Gaudin & Anders | 2020 | 6.312 | 61.326 | 0.288 | -2.823 | -0.988 | β |
| Soubiran et al. | 2018 | 6.312 | 61.326 | β | β | β | -78.11 |
| Bica et al. | 2019 | 6.324 | 61.323 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 6.312 | 61.326 | 0.288 | -2.823 | -0.988 | β |
| Dias et al. | 2018 | β | β | β | -2.33 | 0.08 | β |
| Loktin & Popova | 2017 | 6.315 | 61.323 | β | -1.195 | -2.138 | -116.7 |
| Sampedro et al. | 2017 | 6.317 | 61.323 | β | -2.29 | -0.16 | β |
| Kharchenko et al. | 2016 | 6.26 | 61.337 | β | β | β | β |
| Dias et al. | 2014 | 6.317 | 61.323 | β | -3.44 | -0.32 | β |
| Kharchenko et al. | 2013 | 6.27 | 61.34 | β | -2.49 | -3.62 | -116.7 |
| Gozha et al. | 2012 | 6.317 | 61.323 | β | β | β | β |
| Kharchenko et al. | 2012 | 6.27 | 61.34 | β | -2.49 | -3.62 | -116.7 |
| Bukowiecki et al. | 2011 | 6.304 | 61.344 | β | β | β | β |
| Kharchenko et al. | 2007 | 6.31 | 61.32 | β | 0.03 | β | β |
| Ahumada & Lapasset | 2007 | 6.3 | 61.317 | β | β | β | β |
| van den Bergh | 2006 | 6.325 | 61.35 | β | β | β | β |
| Dias et al. | 2002 | 6.317 | 61.323 | β | -3.44 | -0.32 | -116.7 |
| Dambis | 1999 | 6.325 | 61.35 | β | β | β | β |
| Lynga | 1987 | 6.322 | 61.333 | β | β | β | β |
| Sulentic et al. | 1973 | 6.323 | 61.338 | β | β | β | β |
π‘ 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 | 99999β | 3.03 | 1.42 | 1.37 | 134 | -0.131 | 1164 | 0.58 | 0 |
| Li et al. | 2025 | 3.25 | 1.59 | β | 112 | 0.056 | β | β | β |
| Almeida et al. | 2025 | 2.90 | 1.69 | β | 107 | β | 1231 | β | β |
| Hunt & Reffert | 2024 | 3.09 | 1.40 | 1.37 | 195 | β | 2266(1) | β | β |
| Cavallo et al. | 2024 | 2.83 | 1.51 | β | 282 | 0.070 | β | β | β |
| Hunt & Reffert | 2023 | 3.09 | 1.41 | 1.37 | 195 | β | β | β | β |
| Almeida et al. | 2023 | 2.98 | 1.72 | β | 99 | -0.123 | 841(1) | 0.58 | β |
| Just et al. | 2023 | β | β | β | 367 | β | 34 | β | β |
| Jaehnig et al. | 2021 | 3.11(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 3.16 | 1.26 | β | 132 | β | β | β | 0 |
| Dias et al. | 2021 | 2.90 | 1.69 | β | 107 | -0.138 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.16 | 1.08 | β | 102 | β | β | β | β |
| Kounkel et al. | 2020 | 3.10 | 1.61 | β | 166 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.16 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 3.16 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.16 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 3.00 | 1.26 | β | 134 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.50 | 1.42 | β | 367 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.50 | 1.42 | β | 367 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 1164 | β | β |
| Gozha et al. | 2012 | 3.03 | β | β | 134 | -0.850 | β | β | β |
| Kharchenko et al. | 2012 | 2.50 | 1.42 | β | 367 | β | β | β | β |
| Bukowiecki et al. | 2011 | 3.52(1) | 1.77 | β | 112 | β | β | β | β |
| Paunzen et al. | 2010 | β | β | β | β | -0.850 | β | β | β |
| Ahumada & Lapasset | 2007 | β | 1.29 | β | 135 | β | β | β | 0 |
| van den Bergh | 2006 | 3.03 | 1.29 | β | 135 | β | β | β | β |
| Dias et al. | 2002 | 3.03 | 1.28 | β | 134 | β | β | β | β |
| Dambis | 1999 | 2.75 | 1.74 | β | 28 | β | β | β | β |
| Lynga | 1987 | 3.00 | 1.70 | β | 38 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.2479, e_all=0.1302.
Ahumada & Lapasset (2007)
Star 29 appears as a blue straggler in the diagrams of (1960AAHam...5..215H), but it is located at about five cluster radii from the centre to the west.