NGC 1502
(FoF 2200)
Summary
NGC 1502 is a rich, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It is very well-studied in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dambis (1999) | 61.958 | 62.332 | – | – | – | – |
| Dias et al. (2002) | 61.958 | 62.332 | – | -0.55 | -0.91 | -9.7 |
| Chen et al. (2003) | 61.761 | 62.338 | – | -0.85 | 0.55 | -18.0 |
| Piskunov et al. (2008) | 61.944 | 62.328 | – | – | – | – |
| Kharchenko et al. (2012) | 61.958 | 62.331 | – | 0.01 | -0.54 | – |
| Loktin & Popova (2017) | 61.965 | 62.333 | – | 0.054 | -0.223 | -14.0 |
| Cantat-Gaudin et al. (2018) | 61.954 | 62.332 | 0.916 | -0.571 | -0.848 | – |
| Soubiran et al. (2018) | 61.954 | 62.332 | – | – | – | -14.76 |
| Dias et al. (2019) | 61.954 | 62.332 | 0.916 | -0.571 | -0.848 | -14.76 |
| Liu & Pang (2019) | 61.929 | 62.357 | 0.914 | -0.587 | -0.829 | – |
| Cantat-Gaudin et al. (2020) | 61.954 | 62.332 | 0.916 | -0.571 | -0.848 | – |
| Dias et al. (2021) | 61.951 | 62.337 | 0.91 | -0.571 | -0.835 | – |
| Rain et al. (2021) | 61.954 | 62.332 | 0.916 | -0.571 | -0.848 | – |
| Jaehnig et al. (2021) | 61.953 | 62.34 | 0.954 | -0.592 | -0.859 | – |
| He et al. (2022) | 61.959 | 62.332 | 0.945 | -0.685 | -0.892 | – |
| Hunt & Reffert (2023) | 61.961 | 62.326 | 0.926 | -0.652 | -0.896 | -10.18 |
| Cavallo et al. (2024) | 61.972 | 62.383 | 0.939 | – | – | – |
| Celli et al. (2024) | 61.954 | 62.332 | – | – | – | – |
| Hunt & Reffert (2024) | 61.961 | 62.326 | 0.926 | -0.652 | -0.896 | -10.18 |
| Almeida et al. (2025) | 61.951 | 62.337 | – | – | – | – |
| UCC | 61.957 | 62.334 | 0.939 | -0.651 | -0.908 | -11.337 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.78, DM0=9.27, log_age_=6.5 |
| Dias et al. (2002) | E(B-V)=0.7, Dist=1000.0, Age=7.0 |
| Chen et al. (2003) | HDis=821, Age=0.01 |
| Piskunov et al. (2008) | E(B-V)=0.65, Dist=821, logt=6.8, logMA=1.911 |
| Kharchenko et al. (2012) | e_bv=0.625, distance=1023, log_age=7.08 |
| Loktin & Popova (2017) | E(B-V)=0.759, Dist=816, logt=7.051 |
| Cantat-Gaudin et al. (2018) | dmode=1058.4 |
| Soubiran et al. (2018) | dmode=1058.4 |
| Dias et al. (2019) | E(B-V)=0.73, Dist=1243, logAge=7.01, Z=0.025 |
| Liu & Pang (2019) | Age=0.011, Z=0.0 |
| Cantat-Gaudin et al. (2020) | AVNN=1.92, DistPc=1171.0, AgeNN=7.02 |
| Dias et al. (2021) | Av=2.202, Dist=1056, logage=6.945, [Fe/H]=-0.007 |
| Rain et al. (2021) | E(B-V)=0.7, Dist=1058.4, log(Age)=7.0, NBSS=0 |
| Jaehnig et al. (2021) | dmode=1.052 |
| He et al. (2022) | A0=2.4, logAge=6.75 |
| Hunt & Reffert (2023) | AV50=2.099, diffAV50=2.032, MOD50=10.014, logAge50=6.593 |
| Cavallo et al. (2024) | AV50=2.17, dMod50=10.17, logAge50=6.83, [Fe/H]50=0.11 |
| Celli et al. (2024) | Age=10.5, Mc=887.9 |
| Hunt & Reffert (2024) | MassJ=763.859, MassTot=724.936 |
| Almeida et al. (2025) | AV=2.202, Dist=1056, logAge=6.945, MassRk=559.1 |
Search coordinates in Bayestar19