NGC 2547
(MWSC 1437; FoF 2395; OCSN 233)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
20.4 [arcmin]
- 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
NGC 2547 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.
Very close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 122.502 | -49.184 | 2.583 | -8.545 | 4.344 | 11.441 |
| Li et al. | 2025 | 122.525 | -49.198 | 2.553 | -8.609 | 4.262 | â |
| Wei et al. | 2025 | 122.492 | -49.179 | 2.585 | -8.472 | 4.415 | â |
| Almeida et al. | 2025 | 122.484 | -49.178 | â | â | â | â |
| Alfonso et al. | 2024 | 122.503 | -49.16 | 2.555 | -8.561 | 4.342 | â |
| Hunt & Reffert | 2024 | 122.533 | -49.195 | 2.574 | -8.568 | 4.331 | 9.707 |
| Cavallo et al. | 2024 | 122.456 | -49.133 | 2.58 | â | â | â |
| Hunt & Reffert | 2023 | 122.533 | -49.195 | 2.574 | -8.568 | 4.331 | 9.707 |
| Almeida et al. | 2023 | 122.489 | -49.148 | â | â | â | â |
| Cordoni et al. | 2023 | 122.484 | -49.178 | 2.546 | -8.597 | 4.24 | â |
| Qin et al. | 2023 | 122.53 | -49.2 | 2.58 | -8.58 | 4.34 | 11.94 |
| Just et al. | 2023 | 122.474 | -49.203 | â | â | â | â |
| Jaehnig et al. | 2021 | 122.538 | -49.217 | 2.588 | -8.559 | 4.314 | â |
| Rain et al. | 2021 | 122.525 | -49.198 | 2.553 | -8.609 | 4.262 | â |
| Dias et al. | 2021 | 122.484 | -49.178 | 2.546 | -8.597 | 4.24 | 13.694 |
| Cantat-Gaudin et al. | 2020 | 122.525 | -49.198 | 2.553 | -8.609 | 4.262 | â |
| Cantat-Gaudin & Anders | 2020 | 122.525 | -49.198 | 2.553 | -8.609 | 4.262 | â |
| Liu & Pang | 2019 | 122.451 | -49.152 | 2.545 | -8.592 | 4.261 | â |
| Dias et al. | 2019 | 122.537 | -49.215 | 2.55 | -8.611 | 4.257 | 12.139 |
| Bossini et al. | 2019 | 122.525 | -49.198 | â | â | â | â |
| Soubiran et al. | 2018 | 122.525 | -49.198 | â | â | â | 14.07 |
| Cantat-Gaudin et al. | 2018 | 122.525 | -49.198 | 2.553 | -8.609 | 4.262 | â |
| Loktin & Popova | 2017 | 122.475 | -49.214 | â | -9.343 | 5.618 | 14.8 |
| Kharchenko et al. | 2016 | 122.474 | -49.203 | â | â | â | â |
| Dias et al. | 2014 | 122.537 | -49.215 | â | -2.39 | 4.44 | â |
| Kharchenko et al. | 2013 | 122.478 | -49.205 | â | -8.37 | 4.4 | 14.8 |
| Gozha et al. | 2012 | 122.537 | -49.215 | â | â | â | â |
| Piskunov et al. | 2008 | 122.53 | -49.212 | â | â | â | â |
| Kharchenko et al. | 2007 | 122.53 | -49.22 | â | 0.3 | â | 14.78 |
| Piskunov et al. | 2007 | 122.53 | -49.212 | â | â | â | â |
| van den Bergh | 2006 | 122.607 | -49.167 | â | â | â | â |
| Kharchenko et al. | 2005 | 122.53 | -49.22 | â | -8.95 | 4.08 | 14.78 |
| Kharchenko et al. | 2003 | 122.58 | -49.19 | â | -9.48 | 3.66 | â |
| Chen et al. | 2003 | 122.628 | -49.248 | â | -9.56 | 4.42 | 14.5 |
| Dias et al. | 2002 | 122.537 | -49.215 | â | -7.71 | 3.8 | 15.65 |
| Dambis | 1999 | 122.607 | -49.167 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 0.38 | 0.24 | â | 37 | 0.052 | â | â | â |
| Wei et al. | 2025 | 0.38 | 0.13 | â | 27 | 0.250 | 445 | 0.33 | â |
| Almeida et al. | 2025 | 0.39 | 0.29 | â | 39 | â | 266 | â | â |
| Alfonso et al. | 2024 | 0.40 | 0.14 | â | 28 | -0.013 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 417* | â | â |
| Cavallo et al. | 2024 | 0.40 | 0.59 | â | 15 | -0.040 | â | â | â |
| Hunt & Reffert | 2023 | 0.38 | 0.12 | 0.57 | 22 | â | â | â | â |
| Almeida et al. | 2023 | 0.38 | 0.35 | â | 36 | -0.032 | 362* | 0.23 | â |
| Cordoni et al. | 2023 | 0.39 | 0.29 | â | 39 | -0.014 | 490 | 0.29 | 0.00 |
| Qin et al. | 2023 | 0.38 | 0.12 | â | 40 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 78 | â | 7 | â | â |
| Jaehnig et al. | 2021 | 0.39* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 0.39 | 0.12 | â | 27 | â | â | â | 0 |
| Dias et al. | 2021 | 0.39 | 0.29 | â | 39 | -0.014 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.40 | 0.14 | â | 32 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.39 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 38 | 0.000 | â | â | â |
| Dias et al. | 2019 | 0.38 | 0.25 | â | 37 | 0.051 | â | â | â |
| Bossini et al. | 2019 | 0.39 | 0.12 | â | 27 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.39 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.39 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.46 | 0.13 | â | 37 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.36 | 0.12 | â | 78 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.36 | 0.12 | â | 78 | -0.160 | â | â | â |
| Gozha et al. | 2012 | 0.36 | â | â | 38 | -0.160 | 43 | â | â |
| Piskunov et al. | 2008 | 0.46 | 0.12 | â | 50 | â | 58* | â | â |
| Piskunov et al. | 2007 | 0.46 | 0.12 | â | 50 | â | 12 | â | â |
| van den Bergh | 2006 | 0.46 | 0.12 | â | 36 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.46 | 0.12 | â | 50 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.43 | 0.12 | â | â | â | â | â | â |
| Chen et al. | 2003 | 0.46 | 0.13 | â | 30 | -0.160* | â | â | â |
| Dias et al. | 2002 | 0.36 | 0.58 | â | 38 | -0.160 | â | â | â |
| Dambis | 1999 | 0.38 | 0.17 | â | 45 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.