Melotte 38
(Collinder 75; NGC 2099; MWSC 689; M 37; OCL 451; FSR 0818)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
N50 (P>50% members)
2002
Stellar density (N50/rad)
147.7 [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 38 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above 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.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 88.075 | 32.543 | 0.671 | 1.883 | -5.621 | 6.916 |
| Li et al. | 2025 | 88.074 | 32.545 | 0.666 | 1.924 | -5.648 | β |
| Wei et al. | 2025 | 88.081 | 32.544 | 0.669 | 1.875 | -5.624 | β |
| Carrasco-Varela et al. | 2025 | 88.336 | 32.522 | β | β | β | β |
| Almeida et al. | 2025 | 88.076 | 32.549 | β | β | β | β |
| Zhang et al. | 2024 | 88.08 | 32.541 | β | β | β | β |
| Hunt & Reffert | 2024 | 88.08 | 32.541 | 0.673 | 1.881 | -5.624 | 6.778 |
| Cavallo et al. | 2024 | 88.075 | 32.536 | 0.673 | β | β | β |
| Hunt & Reffert | 2023 | 88.08 | 32.541 | 0.673 | 1.881 | -5.624 | 6.778 |
| Cordoni et al. | 2023 | 88.076 | 32.549 | 0.665 | 1.933 | -5.639 | β |
| Just et al. | 2023 | 88.079 | 32.571 | β | β | β | β |
| Tarricq et al. | 2022 | 88.062 | 32.544 | 0.674 | 1.879 | -5.617 | β |
| Jaehnig et al. | 2021 | 88.072 | 32.546 | 0.698 | 1.925 | -5.635 | β |
| Rain et al. | 2021 | 88.074 | 32.545 | 0.666 | 1.924 | -5.648 | β |
| Dias et al. | 2021 | 88.076 | 32.549 | 0.665 | 1.933 | -5.639 | 11.634 |
| Cantat-Gaudin et al. | 2020 | 88.074 | 32.545 | 0.666 | 1.924 | -5.648 | β |
| SΓ‘nchez et al. | 2020 | 88.075 | 32.553 | β | 2.1 | -5.507 | β |
| Cantat-Gaudin & Anders | 2020 | 88.074 | 32.545 | 0.666 | 1.924 | -5.648 | β |
| Soubiran et al. | 2018 | 88.074 | 32.545 | β | β | β | 8.03 |
| Bica et al. | 2019 | 88.076 | 32.549 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 88.074 | 32.545 | 0.666 | 1.924 | -5.648 | β |
| Loktin & Popova | 2017 | 88.08 | 32.553 | β | 0.708 | -0.196 | 7.7 |
| Kharchenko et al. | 2016 | 88.079 | 32.571 | β | β | β | β |
| Dias et al. | 2014 | 88.075 | 32.553 | β | 2.08 | -6.4 | β |
| Kharchenko et al. | 2013 | 88.087 | 32.57 | β | 2.92 | -7.09 | 7.7 |
| Gozha et al. | 2012 | 88.075 | 32.553 | β | β | β | β |
| Kharchenko et al. | 2012 | 88.087 | 32.57 | β | 2.92 | -7.09 | 7.7 |
| Piskunov et al. | 2008 | 88.076 | 32.549 | β | β | β | β |
| Kharchenko et al. | 2007 | 88.08 | 32.55 | β | 0.32 | β | β |
| Piskunov et al. | 2007 | 88.076 | 32.549 | β | β | β | β |
| van den Bergh | 2006 | 88.079 | 32.553 | β | β | β | β |
| Kharchenko et al. | 2005 | 88.08 | 32.55 | β | 3.09 | -7.35 | β |
| Kharchenko et al. | 2003 | 88.05 | 32.53 | β | 3.42 | -6.61 | β |
| Chen et al. | 2003 | 88.1 | 32.525 | β | 3.36 | -6.17 | 7.7 |
| Dias et al. | 2002 | 88.075 | 32.553 | β | 2.08 | -6.4 | 8.3 |
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 | 1.39 | 0.93 | 0.39 | 355 | 0.089 | 2661 | 0.41 | 0.01 |
| Li et al. | 2025 | 1.33 | 0.83 | β | 671 | -0.047 | β | β | β |
| Wei et al. | 2025 | 1.76 | 0.77 | β | 576 | 0.250 | 3819 | 0.49 | β |
| Carrasco-Varela et al. | 2025 | 1.30 | 0.92 | β | 608 | 0.000 | β | β | 0.01(1) |
| Almeida et al. | 2025 | 1.30 | 0.92 | β | 608 | β | 5058 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.144(1) | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 8682(1) | β | β |
| Cavallo et al. | 2024 | 1.50 | 0.89 | β | 479 | 0.350 | β | β | β |
| Hunt & Reffert | 2023 | 1.39 | 0.62 | 0.39 | 485 | β | β | β | β |
| Cordoni et al. | 2023 | 1.30 | 0.92 | β | 608 | 0.014 | 4410 | 0.33 | 0.00 |
| Just et al. | 2023 | β | β | β | 355 | β | 873 | β | β |
| Tarricq et al. | 2022 | 1.38 | β | β | 447 | β | β | β | β |
| Jaehnig et al. | 2021 | 1.43(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.44 | 0.93 | β | 347 | β | β | β | 1 |
| Dias et al. | 2021 | 1.30 | 0.92 | β | 608 | 0.014 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.43 | 0.75 | β | 447 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.44 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 1.44 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.44 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.41 | 0.93 | β | 346 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.40 | 1.08 | β | 355 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.40 | 1.08 | β | 355 | 0.089 | β | β | β |
| Gozha et al. | 2012 | 1.38 | β | β | 347 | 0.140 | 724 | β | β |
| Kharchenko et al. | 2012 | 1.40 | 1.08 | β | 355 | 0.089 | β | β | β |
| Piskunov et al. | 2008 | 1.38 | 0.93 | β | 347 | β | 1503(1) | β | β |
| Piskunov et al. | 2007 | 1.38 | 0.93 | β | 347 | β | 382 | β | β |
| van den Bergh | 2006 | 1.38 | 0.93 | β | 347 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.38 | 0.93 | β | 347 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.39 | 0.93 | β | β | β | β | β | β |
| Chen et al. | 2003 | 1.38 | 0.94 | β | 340 | 0.090(1) | β | β | β |
| Dias et al. | 2002 | 1.38 | 0.94 | β | 347 | 0.089 | 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.