IC 348
(OCSN 203)
Summary
IC 348 is a rich, very dense object of very high C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It is very well-studied in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 56.142 | 32.163 | – | 3.38 | -7.37 | 18.1 |
| Piskunov et al. (2008) | 56.136 | 32.157 | – | – | – | – |
| Kharchenko et al. (2012) | 56.153 | 32.15 | – | 4.33 | -10.17 | – |
| Loktin & Popova (2017) | 56.145 | 32.163 | – | 3.866 | -12.586 | 16.0 |
| Cantat-Gaudin et al. (2018) | 56.132 | 32.159 | 3.079 | 4.483 | -6.447 | – |
| Soubiran et al. (2018) | 56.132 | 32.159 | – | – | – | 19.71 |
| Donor et al. (2020) | 56.153 | 32.15 | – | 4.38 | -6.26 | 16.7 |
| Cantat-Gaudin et al. (2020) | 56.132 | 32.159 | 3.079 | 4.483 | -6.447 | – |
| Dias et al. (2021) | 56.135 | 32.184 | 3.08 | 4.43 | -6.508 | 21.013 |
| Rain et al. (2021) | 56.132 | 32.159 | 3.079 | 4.483 | -6.447 | – |
| Jaehnig et al. (2021) | 56.124 | 32.159 | 3.113 | 4.472 | -6.437 | – |
| He et al. (2022) | 55.621 | 32.304 | 3.261 | 4.86 | -6.993 | – |
| Qin et al. (2023) | 56.14 | 32.15 | 3.17 | 4.47 | -6.3 | 11.18 |
| Hunt & Reffert (2023) | 56.137 | 32.177 | 3.164 | 4.423 | -6.343 | 11.679 |
| Cavallo et al. (2024) | 56.004 | 32.199 | 3.166 | – | – | – |
| Celli et al. (2024) | 56.132 | 32.159 | – | – | – | – |
| Hunt & Reffert (2024) | 56.137 | 32.177 | 3.164 | 4.423 | -6.343 | 11.679 |
| Alfonso et al. (2024) | 56.107 | 32.159 | 3.129 | 4.432 | -6.336 | – |
| Almeida et al. (2025) | 56.135 | 32.184 | – | – | – | – |
| UCC | 56.124 | 32.155 | 3.172 | 4.417 | -6.338 | 13.17 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.929, Dist=385.0, Age=7.641 |
| Piskunov et al. (2008) | E(B-V)=0.82, Dist=394, logt=7.79, logMA=0.67 |
| Kharchenko et al. (2012) | e_bv=1.049, distance=480, log_age=6.78 |
| Loktin & Popova (2017) | E(B-V)=0.984, Dist=370, logt=7.742 |
| Cantat-Gaudin et al. (2018) | dmode=321.7 |
| Soubiran et al. (2018) | dmode=321.7 |
| Donor et al. (2020) | Fe/H=-0.11 |
| Cantat-Gaudin et al. (2020) | AVNN=1.91, DistPc=337.0, AgeNN=7.07 |
| Dias et al. (2021) | Av=0.331, Dist=321, logage=6.78, [Fe/H]=0.302 |
| Rain et al. (2021) | E(B-V)=0.92, Dist=321.7, log(Age)=7.64, NBSS=0 |
| Jaehnig et al. (2021) | dmode=0.32 |
| He et al. (2022) | A0=0.2, logAge=6.5 |
| Qin et al. (2023) | E(B-V)=0.11, m-M=7.79, logt=6.25 |
| Hunt & Reffert (2023) | AV50=2.545, diffAV50=2.482, MOD50=7.445, logAge50=6.778 |
| Cavallo et al. (2024) | AV50=2.97, dMod50=7.84, logAge50=6.65, [Fe/H]50=0.06 |
| Celli et al. (2024) | Age=11.7, Mc=101.3 |
| Hunt & Reffert (2024) | MassJ=187.429, MassTot=191.695 |
| Alfonso et al. (2024) | AV=1.90755, MOD=7.61026, logAge=7.04353, Z=0.30205 |
| Almeida et al. (2025) | AV=0.331, Dist=321, logAge=6.78, MassRk=135.1 |
Search coordinates in Bayestar19