IC 2488
(Melotte 97; Collinder 208; VDBH 69; MWSC 1671; OCL 789; vdBergh-Hagen 69; ESO 166 14; FoF 675)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
33.1 [N/pc2]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
IC 2488 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity 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 | 99999â | 141.869 | -57.008 | 0.733 | -7.731 | 5.742 | -3.803 |
| Li et al. | 2025 | 141.857 | -57.004 | 0.718 | -7.761 | 5.698 | â |
| Wei et al. | 2025 | 141.843 | -56.998 | 0.728 | -7.718 | 5.732 | â |
| Almeida et al. | 2025 | 141.846 | -57.019 | â | â | â | â |
| Hunt & Reffert | 2024 | 141.887 | -56.988 | 0.734 | -7.742 | 5.748 | -3.403 |
| Cavallo et al. | 2024 | 141.864 | -57.026 | 0.734 | â | â | â |
| Hunt & Reffert | 2023 | 141.887 | -56.988 | 0.734 | -7.742 | 5.748 | -3.403 |
| Almeida et al. | 2023 | 141.793 | -57.036 | â | â | â | â |
| Cordoni et al. | 2023 | 141.846 | -57.019 | 0.724 | -7.764 | 5.689 | â |
| Just et al. | 2023 | 141.91 | -56.996 | â | â | â | â |
| Tarricq et al. | 2022 | 141.902 | -56.992 | 0.731 | -7.736 | 5.747 | â |
| Jaehnig et al. | 2021 | 141.869 | -56.996 | 0.754 | -7.768 | 5.701 | â |
| Rain et al. | 2021 | 141.857 | -57.004 | 0.718 | -7.761 | 5.698 | â |
| Richer et al. | 2021 | 141.873 | -56.996 | 0.73 | -7.75 | 5.68 | â |
| Dias et al. | 2021 | 141.846 | -57.019 | 0.724 | -7.764 | 5.689 | -3.269 |
| Cantat-Gaudin et al. | 2020 | 141.857 | -57.004 | 0.718 | -7.761 | 5.698 | â |
| Cantat-Gaudin & Anders | 2020 | 141.857 | -57.004 | 0.718 | -7.761 | 5.698 | â |
| Liu & Pang | 2019 | 141.843 | -56.996 | 0.729 | -7.758 | 5.689 | â |
| Bossini et al. | 2019 | 141.857 | -57.004 | â | â | â | â |
| Soubiran et al. | 2018 | 141.857 | -57.004 | â | â | â | -1.42 |
| Bica et al. | 2019 | 141.907 | -56.987 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 141.857 | -57.004 | 0.718 | -7.761 | 5.698 | â |
| Loktin & Popova | 2017 | 141.915 | -57.0 | â | -3.11 | 4.55 | -2.6 |
| Kharchenko et al. | 2016 | 141.91 | -56.996 | â | â | â | â |
| Dias et al. | 2014 | 141.908 | -57.0 | â | -3.11 | 4.55 | â |
| Kharchenko et al. | 2013 | 141.915 | -57.0 | â | -6.78 | 6.0 | -2.6 |
| Gozha et al. | 2012 | 141.908 | -57.0 | â | â | â | â |
| Piskunov et al. | 2008 | 141.908 | -57.001 | â | â | â | â |
| Kharchenko et al. | 2007 | 141.91 | -57.0 | â | 0.3 | â | â |
| Piskunov et al. | 2007 | 141.908 | -57.001 | â | â | â | â |
| Ahumada & Lapasset | 2007 | 141.9 | -57.0 | â | â | â | â |
| van den Bergh | 2006 | 141.9 | -57.0 | â | â | â | â |
| Kharchenko et al. | 2005 | 141.91 | -57.0 | â | -7.03 | 5.82 | â |
| Kharchenko et al. | 2003 | 141.91 | -56.98 | â | -6.85 | 7.76 | â |
| Dias et al. | 2002 | 141.908 | -57.0 | â | -3.11 | 4.55 | -1.84 |
| Dambis | 1999 | 141.908 | -57.0 | â | â | â | â |
| Lynga | 1987 | 141.907 | -56.972 | â | â | â | â |
| van den Bergh & Hagen | 1975 | 141.525 | -56.767 | 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 | 1.29 | 0.73 | 0.99 | 166 | 0.100 | 1023 | 0.47 | 0 |
| Li et al. | 2025 | 1.29 | 0.67 | â | 299 | 0.160 | â | â | â |
| Wei et al. | 2025 | 1.68 | 1.12 | â | 204 | -0.250 | 981 | 0.53 | â |
| Almeida et al. | 2025 | 1.27 | 0.89 | â | 179 | â | 1337 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1672(1) | â | â |
| Cavallo et al. | 2024 | 1.32 | 0.88 | â | 166 | 0.260 | â | â | â |
| Hunt & Reffert | 2023 | 1.29 | 0.73 | 0.99 | 181 | â | â | â | â |
| Almeida et al. | 2023 | 1.29 | 0.98 | â | 153 | 0.019 | 1190(1) | 0.47 | â |
| Cordoni et al. | 2023 | 1.27 | 0.89 | â | 179 | 0.094 | 3029 | 0.45 | 0(1) |
| Just et al. | 2023 | â | â | â | 279 | â | 97 | â | â |
| Tarricq et al. | 2022 | 1.29 | â | â | 166 | â | â | â | â |
| Jaehnig et al. | 2021 | 1.33(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.34 | 0.69 | â | 158 | â | â | â | 0 |
| Richer et al. | 2021 | â | 0.84 | â | 162 | â | â | â | â |
| Dias et al. | 2021 | 1.27 | 0.89 | â | 179 | 0.094 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.32 | 0.67 | â | 162 | â | â | â | â |
| Kounkel et al. | 2020 | 1.30 | 0.90 | â | 138 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.34 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 105 | 0.250 | â | â | â |
| Bossini et al. | 2019 | 1.33 | 0.70 | â | 158 | 0.080 | â | â | â |
| Soubiran et al. | 2018 | 1.34 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.34 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.48 | 1.02 | â | 25 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.14 | 0.66 | â | 279 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.14 | 0.66 | â | 279 | 0.100 | â | â | â |
| Gozha et al. | 2012 | 1.13 | â | â | 130 | 0.100 | 1023 | â | â |
| Piskunov et al. | 2008 | 1.13 | 0.73 | â | 339 | â | 410(1) | â | â |
| Piskunov et al. | 2007 | 1.13 | 0.73 | â | 339 | â | 87 | â | â |
| Ahumada & Lapasset | 2007 | â | 0.73 | â | 129 | â | â | â | 3 |
| van den Bergh | 2006 | 1.13 | 0.73 | â | 129 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.13 | 0.73 | â | 339 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.14 | 0.73 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.13 | 0.73 | â | 130 | 0.100 | â | â | â |
| Dambis | 1999 | 1.08 | 0.73 | â | 126 | â | â | â | â |
(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. Gold sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Richer et al. (2021)
The expected number of WDs is 22.8, 0 WD candidates found, and 0 WD candidates found in the wide search.
Rain et al. (2021)
This cluster was include in (Dias et al., 2002A&A...389..871D, Cat. B/ocl) however, parameters log(t)=8.200, Av=0.702, [Fe/H]=0.080 were taken from Bossini et al. (2019A&A...623A.108B, Cat. J/A+A/623/A108). Ahumada & Lapasset (2007A&A...463..789A, Cat. J/A+A/463/789) cite star DR2 5306633687113120000=HD 302225 as a blue straggler, the star is a member according to Cantat-Gaudin et al. (2018A&A...618A..93C, Cat. J/A+A18/A93) however, it is located in the turnoff of the cluster and therefore was not included in our catalogue.
Ahumada & Lapasset (2007)
Diagrams in (1987AJ.....94...92P) were also examined. Adopted cluster centre: star 28 in (1987AJ.....94...92P). Star 99=HD 302225(B8) is cited as a blue straggler in (1987AJ.....94...92P), and is a probable cluster member (2003A&A...399..543C).