Gaia DR2 2558649835138475904
All names: Gaia DR3 2558649835138475904, WDJ01370.74+014216.17, SDSS J013700.80+014215.8, Gaia EDR3 2558649835138475904, Gaia DR2 2558649835138475904, WDJ013700.74+014216.18, SDSS J013700.80+014215.7
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Kilic et al. 2025 | MWDD H | MWDD HE | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 01 37 00.85 (0.1) | 01 37 00.85 | 01 37 00.85 | 01 37 00.74 (0.1) | 01 37 00.85 | ||||||
| Declination | 01 42 15.45 (0.07) | 01 42 15.48 | 01 42 15.45 | 01 42 16.18 (0.07) | 01 42 15.48 | ||||||
| Spectral type | DA | DA | DA | ||||||||
| Effective temperature | [K] | 6560.0 (30) | 6504.0 | 6253.0 | 6451.0 (69) | ||||||
| log(g) | [cgs] | 8.18 (0.01) | 8.16 | 8.03 | 8.14 (0.02) | ||||||
| Mass | [M☉] | 0.701 (0.01) | 0.69 | 0.593 | 0.679 (0.02) | ||||||
| log(Luminosity) | [L☉] | ||||||||||
| Cooling age | [Gyr] | 2.5780 | 2.2560 | ||||||||
| log(H/He) | |||||||||||
| log(C/He) | |||||||||||
| log(Ca/He) | |||||||||||
| log(Ca/H) | |||||||||||
| log(C/H) | |||||||||||
| log(N/H) | |||||||||||
| log(O/H) | |||||||||||
| log(Na/H) | |||||||||||
| log(Mg/H) | |||||||||||
| log(Al/H) | |||||||||||
| log(Si/H) | |||||||||||
| log(P/H) | |||||||||||
| log(S/H) | |||||||||||
| log(Sc/H) | |||||||||||
| log(Ti/H) | |||||||||||
| log(Cr/H) | |||||||||||
| log(Mn/H) | |||||||||||
| log(Fe/H) | |||||||||||
| log(Ni/H) | |||||||||||
| Parallax | [mas] | 16.18 (0.1) | 16.21 (0.1) | 16.18 | 16.18 (0.1) | 16.21 (0.1) | |||||
| Distance | [pc] | 61.80 (0.5) | 61.68 (0.6) | 61.80 | 61.80 (0.5) | 61.68 (0.6) | |||||
| Composition | H | ||||||||||
| Proper motion (right ascension) | [mas/yr] | 103.4643443 (0.2) | 103.6896908 (0.3) | 103.464 (0.2) | 103.6896908 | ||||||
| Proper motion (declination) | [mas/yr] | -45.55894109 (0.08) | -45.25331397 (0.2) | -45.559 (0.08) | -45.25331397 | ||||||
| Variability | |||||||||||
| Magnetic | |||||||||||
| Bd | [MG] | ||||||||||
| Infrared excess (disk) | |||||||||||
| Binarity | |||||||||||
| B magnitude | |||||||||||
| V magnitude | |||||||||||
| R magnitude | |||||||||||
| I magnitude | |||||||||||
| J magnitude | |||||||||||
| H magnitude | |||||||||||
| K magnitude | |||||||||||
| u magnitude | 18.80 (0.02) | 18.80 (0.02) | |||||||||
| g magnitude | 18.15 (0.006) | 18.15 (0.006) | |||||||||
| r magnitude | 17.91 (0.007) | 17.91 (0.007) | |||||||||
| i magnitude | 17.82 (0.008) | 17.82 (0.008) | |||||||||
| z magnitude | 17.82 (0.02) | 17.82 (0.02) | |||||||||
| G magnitude | 17.88 (0.01) | 17.90 | 17.88 | 17.88 (0.003) | 17.90 | ||||||
| BP magnitude | 18.13 (0.01) | 18.17 | 18.17 | ||||||||
| RP magnitude | 17.50 (0.01) | 17.50 | 17.50 | ||||||||
| Pan g magnitude | 18.12 (0.005) | ||||||||||
| Pan r magnitude | 17.90 (0.006) | ||||||||||
| Pan i magnitude | 17.82 (0.004) | ||||||||||
| Pan z magnitude | 17.85 (0.005) | ||||||||||
| Pan y magnitude | 17.85 (0.01) | ||||||||||
| E(B-V) | 0.002 | ||||||||||
* Constant surface field
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