Gaia DR2 126017157963829120
All names: Gaia DR2 126017157963829120, Gaia DR3 126017157963829120, J0323+3501, WDJ032331.68+350116.24, WDJ032331.68+350116.23, Gaia EDR3 126017157963829120, LAMOST J032331.70+350115.9
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | Jewett et al. 2024 | MWDD H | MWDD HE | Gaia DR2 | Stilism | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 03 23 31.73 (0.08) | 03 23 31.73 | 03 23 31.73 | 03 23 31.68 (0.08) | 03 23 31.73 | ||||||
| Declination | 35 01 15.79 (0.07) | 35 01 15.80 | 35 01 15.79 | 35 01 16.24 (0.07) | 35 01 15.80 | ||||||
| Spectral type | DA | DA | DA | ||||||||
| Effective temperature | [K] | 13621.0 (246) | 13629.0 | 13819.0 | 13760.0 (432) | ||||||
| log(g) | [cgs] | 8.57 | 8.58 | 8.58 | 8.57 (0.02) | ||||||
| Mass | [M☉] | 0.971 (0.01) | 0.975 | 0.957 | 0.97 (0.02) | ||||||
| log(Luminosity) | [L☉] | ||||||||||
| Cooling age | [Gyr] | 0.6800 (0.04) | 0.6554 | 0.6412 | |||||||
| 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] | 10.47 (0.09) | 10.53 (0.1) | 10.47 | 10.47 (0.09) | 10.53 (0.1) | |||||
| Distance | [pc] | 95.53 (0.8) | 94.99 (1) | 95.53 | 95.53 (0.8) | 94.99 (1) | |||||
| Composition | H | ||||||||||
| Proper motion (right ascension) | [mas/yr] | 39.55530011 (0.1) | 39.70285765 (0.2) | 39.555 (0.1) | 39.70285765 | ||||||
| Proper motion (declination) | [mas/yr] | -28.18418795 (0.09) | -28.17193856 (0.2) | -28.184 (0.09) | -28.17193856 | ||||||
| Variability | |||||||||||
| Magnetic | |||||||||||
| Bd | [MG] | ||||||||||
| Infrared excess (disk) | |||||||||||
| Binarity | |||||||||||
| B magnitude | |||||||||||
| V magnitude | |||||||||||
| R magnitude | |||||||||||
| I magnitude | |||||||||||
| J magnitude | |||||||||||
| H magnitude | |||||||||||
| K magnitude | |||||||||||
| u magnitude | |||||||||||
| g magnitude | |||||||||||
| r magnitude | |||||||||||
| i magnitude | |||||||||||
| z magnitude | |||||||||||
| G magnitude | 17.28 (0.008) | 17.30 | 17.28 | 17.28 (0.003) | 17.30 | ||||||
| BP magnitude | 17.27 (0.008) | 17.27 | 17.27 | ||||||||
| RP magnitude | 17.32 (0.01) | 17.34 | 17.34 | ||||||||
| Pan g magnitude | 17.19 (0.005) | ||||||||||
| Pan r magnitude | 17.41 (0.004) | ||||||||||
| Pan i magnitude | 17.65 (0.006) | ||||||||||
| Pan z magnitude | 17.87 (0.01) | ||||||||||
| Pan y magnitude | 18.03 (0.01) | ||||||||||
| E(B-V) | 0.007 | ||||||||||
* Constant surface field
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