Gaia DR2 2781770637386074112
All names: Gaia EDR3 2781770637386074112, WDJ00516.38+165936.56, SDSS J005106.40+165936.1, SDSS J005106.40+165936.2, Gaia DR2 2781770637386074112, Gaia DR3 2781770637386074112, WDJ005106.38+165936.57
| 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 | 00 51 06.42 (0.1) | 00 51 06.42 | 00 51 06.42 | 00 51 06.38 (0.1) | 00 51 06.42 | ||||||
| Declination | 16 59 36.02 (0.07) | 16 59 36.04 | 16 59 36.02 | 16 59 36.57 (0.07) | 16 59 36.04 | ||||||
| Spectral type | DA | DA | DA | ||||||||
| Effective temperature | [K] | 5493.0 (12) | 5533.0 | 5251.0 | 5762.0 (51) | ||||||
| log(g) | [cgs] | 8.06 (0.009) | 8.09 | 7.91 | 8.19 (0.02) | ||||||
| Mass | [M☉] | 0.622 (0.008) | 0.64 | 0.514 | 0.705 (0.02) | ||||||
| log(Luminosity) | [L☉] | ||||||||||
| Cooling age | [Gyr] | 3.8480 | 4.0530 | ||||||||
| 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] | 20.82 (0.1) | 20.95 (0.2) | 20.82 | 20.82 (0.1) | 20.95 (0.2) | |||||
| Distance | [pc] | 48.02 (0.3) | 47.74 (0.3) | 48.02 | 48.02 (0.3) | 47.74 (0.3) | |||||
| Composition | H | ||||||||||
| Proper motion (right ascension) | [mas/yr] | 34.99663032 (0.2) | 35.17101098 (0.3) | 34.997 (0.2) | 35.17101098 | ||||||
| Proper motion (declination) | [mas/yr] | -34.38802513 (0.1) | -34.07458207 (0.2) | -34.388 (0.1) | -34.07458207 | ||||||
| Variability | |||||||||||
| Magnetic | |||||||||||
| Bd | [MG] | ||||||||||
| Infrared excess (disk) | |||||||||||
| Binarity | |||||||||||
| B magnitude | |||||||||||
| V magnitude | |||||||||||
| R magnitude | |||||||||||
| I magnitude | |||||||||||
| J magnitude | |||||||||||
| H magnitude | |||||||||||
| K magnitude | |||||||||||
| u magnitude | 19.64 (0.04) | 19.64 (0.04) | |||||||||
| g magnitude | 18.39 (0.007) | 18.39 (0.007) | |||||||||
| r magnitude | 17.86 (0.007) | 17.86 (0.007) | |||||||||
| i magnitude | 17.70 (0.007) | 17.70 (0.007) | |||||||||
| z magnitude | 17.61 (0.02) | 17.61 (0.02) | |||||||||
| G magnitude | 17.89 (0.01) | 17.91 | 17.89 | 17.89 (0.003) | 17.91 | ||||||
| BP magnitude | 18.24 (0.01) | 18.25 | 18.25 | ||||||||
| RP magnitude | 17.37 (0.009) | 17.33 | 17.33 | ||||||||
| Pan g magnitude | 18.32 (0.003) | ||||||||||
| Pan r magnitude | 17.88 (0.004) | ||||||||||
| Pan i magnitude | 17.70 (0.003) | ||||||||||
| Pan z magnitude | 17.64 (0.006) | ||||||||||
| Pan y magnitude | 17.65 (0.006) | ||||||||||
| E(B-V) | 0.002 | ||||||||||
* Constant surface field
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