Melotte 88
(Collinder 189; NGC 2632; MWSC 1527; Praesepe; M 44; OCL 507; OCSN 234)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
N50 (P>50% members)
1204
Stellar density (N50/rad)
67.8 [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
Melotte 88 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the absorption and age 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 | 130.013 | 19.605 | 5.407 | -35.927 | -12.862 | 34.728 |
| Nizovkina et al. | 2025 | 130.088 | 19.666 | â | â | â | â |
| Li et al. | 2025 | 130.054 | 19.621 | 5.361 | -36.09 | -12.919 | â |
| Wei et al. | 2025 | 130.015 | 19.645 | 5.408 | -35.94 | -12.884 | â |
| Almeida et al. | 2025 | 130.057 | 19.613 | â | â | â | â |
| Alfonso et al. | 2024 | 129.974 | 19.621 | 5.368 | -35.914 | -12.884 | â |
| Zhang et al. | 2024 | 130.088 | 19.666 | â | â | â | â |
| Hunt & Reffert | 2024 | 130.088 | 19.666 | 5.404 | -35.943 | -12.903 | 33.941 |
| Cavallo et al. | 2024 | 129.975 | 19.608 | 5.405 | â | â | â |
| Hunt & Reffert | 2023 | 130.088 | 19.666 | 5.404 | -35.943 | -12.903 | 33.941 |
| Cordoni et al. | 2023 | 130.057 | 19.613 | 5.349 | -36.148 | -12.95 | â |
| Qin et al. | 2023 | 130.06 | 19.66 | 5.41 | -35.89 | -12.9 | 34.9 |
| He et al. | 2022 | 129.993 | 19.612 | 5.41 | -35.902 | -12.879 | â |
| Tarricq et al. | 2022 | 130.059 | 19.621 | 5.416 | -35.911 | -12.896 | â |
| Jaehnig et al. | 2021 | 130.056 | 19.623 | 5.385 | -35.964 | -12.918 | â |
| Rain et al. | 2021 | 130.054 | 19.621 | 5.361 | -36.09 | -12.919 | â |
| Dias et al. | 2021 | 130.057 | 19.613 | 5.349 | -36.148 | -12.95 | 34.892 |
| Cantat-Gaudin et al. | 2020 | 130.054 | 19.621 | 5.361 | -36.09 | -12.919 | â |
| Cantat-Gaudin & Anders | 2020 | 130.054 | 19.621 | 5.361 | -36.09 | -12.919 | â |
| Bossini et al. | 2019 | 130.054 | 19.621 | â | â | â | â |
| Soubiran et al. | 2018 | 130.054 | 19.621 | â | â | â | 34.72 |
| Bica et al. | 2019 | 130.057 | 19.939 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 130.054 | 19.621 | 5.361 | -36.09 | -12.919 | â |
| Yen et al. | 2018 | 129.978 | 19.602 | 5.39 | -36.03 | -12.86 | â |
| Loktin & Popova | 2017 | 130.095 | 19.668 | â | -35.58 | -12.9 | 33.4 |
| Kharchenko et al. | 2016 | 130.087 | 19.693 | â | â | â | â |
| Kharchenko et al. | 2013 | 130.095 | 19.69 | â | -36.54 | -13.36 | 33.4 |
| Gozha et al. | 2012 | 130.1 | 19.667 | â | â | â | â |
| Piskunov et al. | 2008 | 130.087 | 19.689 | â | â | â | â |
| Kharchenko et al. | 2007 | 130.09 | 19.67 | â | 3.0 | â | 33.66 |
| Piskunov et al. | 2007 | 130.087 | 19.689 | â | â | â | â |
| van den Bergh | 2006 | 130.1 | 19.683 | â | â | â | â |
| Kharchenko et al. | 2005 | 130.09 | 19.69 | â | -35.9 | -12.88 | 33.57 |
| Kharchenko et al. | 2003 | 130.09 | 19.69 | â | -35.83 | -13.11 | â |
| Chen et al. | 2003 | 130.053 | 19.659 | â | -35.58 | -12.9 | 34.4 |
| Dias et al. | 2002 | 130.1 | 19.667 | â | -35.58 | -12.9 | 34.76 |
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 | 0.19 | 0.03 | 0.53 | 746 | 0.196 | 652 | 0.365 | 0.0 |
| Nizovkina et al. | 2025 | 0.17(4) | 0.12(4) | â | 780(4) | 0.051(4) | â | â | â |
| Li et al. | 2025 | 0.18 | 0.00 | â | 784 | 0.245 | â | â | â |
| Wei et al. | 2025 | 0.20 | 0.60 | â | 158 | 0.250 | 652 | 0.48 | â |
| Almeida et al. | 2025 | 0.19 | 0.03 | â | 762 | â | 458 | â | â |
| Alfonso et al. | 2024 | 0.18 | 0.00 | â | 946 | 0.198 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.193(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 945(1) | â | â |
| Cavallo et al. | 2024 | 0.19 | 0.60 | â | 155 | 0.240 | â | â | â |
| Hunt & Reffert | 2023 | 0.18 | 0.16 | 0.53 | 346 | â | â | â | â |
| Cordoni et al. | 2023 | 0.19 | 0.03 | â | 762 | 0.196 | 611 | 0.25 | 0.00 |
| Qin et al. | 2023 | 0.18 | 0.03 | â | 708 | â | â | â | â |
| He et al. | 2022 | â | 0.40 | â | 708 | â | â | â | â |
| Tarricq et al. | 2022 | 0.18 | â | â | 692 | â | â | â | â |
| Jaehnig et al. | 2021 | 0.19(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 0.19 | 0.06 | â | 741 | â | â | â | 1 |
| Dias et al. | 2021 | 0.19 | 0.03 | â | 762 | 0.196 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.18 | 0.00 | â | 676 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.19 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 0.19 | 0.08 | â | 750 | 0.070 | â | â | â |
| Soubiran et al. | 2018 | 0.19 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.19 | â | â | â | â | â | â | â |
| Yen et al. | 2018 | 0.18 | 0.03 | â | 794 | â | â | â | â |
| Loktin & Popova | 2017 | 0.19 | 0.03 | â | 731 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.19 | 0.03 | â | 832 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.19 | 0.03 | â | 832 | 0.094 | â | â | â |
| Gozha et al. | 2012 | 0.19 | â | â | 729 | 0.270 | 302 | â | â |
| Piskunov et al. | 2008 | 0.19 | 0.03 | â | 794 | â | 2328(1) | â | â |
| Piskunov et al. | 2007 | 0.19 | 0.03 | â | 794 | â | 1807 | â | â |
| van den Bergh | 2006 | 0.19 | 0.03 | â | 724 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.19 | 0.03 | â | 794 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.18 | 0.03 | â | â | â | â | â | â |
| Chen et al. | 2003 | 0.19 | 0.03 | â | 720 | 0.140(1) | â | â | â |
| Dias et al. | 2002 | 0.19 | 0.03 | â | 729 | 0.270 | 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.
Cavallo et al. (2024)
Gold sample.