LP 20-214
All names: USNO-B1.0 1683-00054877, PM J12145+7822, Gaia EDR3 1717341818608187648, NLTT 30084, Gaia DR3 1717341818608187648, TIC 427587075, 2MASS J12143183+7822559, LP 20-214, Gaia DR2 1717341818608187648, 12145+7822, PSO J183.6350+78.3812, LSPM J1214+7822, WDJ121431.83+782256.54, J1214+7822
| Parameter | Unit | Gaia EDR3 | Pan-STARRS DR1 | O'Brien et al. 2024 | Caron et al. 2023 | Blouin & Xu 2022 | McCleery et al. 2020 | Coutu et al. 2019 | Blouin et al. 2019 | MWDD H | Gaia DR2 | Stilism | Limoges et al. 2015 | Vincent et al. 2024 | Simbad | Gentile Fusillo et al. 2018 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Right ascension | 12 14 32.47 (0.08) | 12 14 32.45 (0.1) | 12 14 31.83 | 12 14 32.45 (0.1) | 12 14 32.47 | 12 14 31.83 (0.08) | 12 14 32.45 | |||||||||
| Declination | 78 22 52.32 (0.07) | 78 22 52.45 (0.08) | 78 22 56.54 | 78 22 52.45 (0.08) | 78 22 52.32 | 78 22 56.54 (0.07) | 78 22 52.45 | |||||||||
| Spectral type | DZ | DZ | DZ | DZ | DZ | DZ | DZ | DC: | DZ | |||||||
| Effective temperature | [K] | 4835.0 (59) | 4895.0 (31) | 4911.0 (41) | 4804.1 (44) | 4329.0 (61) | 4210.0 (20) | 4890.0 | 5000.0 (656) | 4875.0 (33) | ||||||
| log(g) | [cgs] | 7.86 (0.05) | 7.91 (0.01) | 7.92 (0.03) | 7.85 (0.04) | 7.48 | 7.51 (0.02) | 7.91 | 8.00 (0) | 7.90 (0.02) | ||||||
| Mass | [M☉] | 0.497 (0.03) | 0.514 (0.01) | 0.534 (0.01) | 0.3078 | 0.318 (0.009) | 0.527 | 0.58 (0.1) | 0.517 (0.01) | |||||||
| log(Luminosity) | [L☉] | -4.05 | ||||||||||||||
| Cooling age | [Gyr] | 5.3500 | 5.4800 | 3.2200 | 3.5510 (0.1) | 5.1880 | ||||||||||
| log(H/He) | <-30.0 | |||||||||||||||
| log(C/He) | ||||||||||||||||
| log(Ca/He) | -11.2283 (0.1) | -11.2 | -11.87 | |||||||||||||
| log(Ca/H) | -9.4 | -9.13 (0.07) | ||||||||||||||
| 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] | 30.63 (0.08) | 30.63 (0.08) | 30.60 (0.1) | 30.63 (0.08) | 30.60 (0.1) | 30.60 | 30.60 (0.1) | 30.60 (0.1) | 30.63 | 30.63 (0.08) | 30.60 (0.1) | ||||
| Distance | [pc] | 32.65 (0.09) | 32.65 (0.09) | 32.68 (0.1) | 32.65 (0.09) | 32.68 (0.1) | 32.68 (0.1) | 32.68 (0.1) | 32.68 (0.1) | 32.90 (6) | 32.65 | 32.65 (0.09) | 32.68 (0.1) | |||
| Composition | H | H | He | He | He | H | ||||||||||
| Proper motion (right ascension) | [mas/yr] | 120.8142295 (0.1) | 120.4445682 (0.2) | 135.0 | 120.814 (0.1) | 120.4445682 | ||||||||||
| Proper motion (declination) | [mas/yr] | -263.6341682 (0.1) | -263.5868723 (0.2) | -256.0 | -263.634 (0.1) | -263.5868723 | ||||||||||
| Variability | ||||||||||||||||
| Magnetic | ||||||||||||||||
| Bd | [MG] | |||||||||||||||
| Infrared excess (disk) | ||||||||||||||||
| Binarity | ||||||||||||||||
| B magnitude | 18.00 | |||||||||||||||
| V magnitude | ||||||||||||||||
| R magnitude | 17.20 | |||||||||||||||
| I magnitude | ||||||||||||||||
| J magnitude | 16.18 (0.09) | 16.18 (0.1) | 16.18 | 16.18 (0.1) | ||||||||||||
| H magnitude | 15.65 (0.2) | 15.65 (0.2) | 15.65 | 15.65 (0.2) | ||||||||||||
| K magnitude | 15.64 (0.2) | 15.64 (0.2) | 15.64 | 15.64 (0.2) | ||||||||||||
| u magnitude | ||||||||||||||||
| g magnitude | 18.05 (0.02) | |||||||||||||||
| r magnitude | 17.38 (0.004) | |||||||||||||||
| i magnitude | 17.12 (0.005) | |||||||||||||||
| z magnitude | 17.03 (0.003) | |||||||||||||||
| G magnitude | 17.42 (0.01) | 17.44 | 17.44 | 17.42 | 17.42 (0.003) | 17.44 | ||||||||||
| BP magnitude | 17.94 (0.01) | 17.95 | 17.95 | |||||||||||||
| RP magnitude | 16.76 (0.007) | 16.77 | 16.77 | |||||||||||||
| Pan g magnitude | 18.08 (0.01) | 18.05 (0.02) | 18.05 (0.02) | 18.05 (0.02) | ||||||||||||
| Pan r magnitude | 17.37 (0.01) | 17.38 (0.004) | 17.38 (0.004) | 17.38 (0.004) | ||||||||||||
| Pan i magnitude | 17.10 (0.01) | 17.12 (0.005) | 17.12 (0.005) | 17.12 (0.005) | ||||||||||||
| Pan z magnitude | 17.00 (0.004) | 17.03 (0.003) | 17.03 (0.003) | 17.03 (0.003) | ||||||||||||
| Pan y magnitude | 16.99 (0.01) | 17.00 (0.02) | 17.00 (0.02) | 17.00 (0.02) | ||||||||||||
| E(B-V) | 0.002 | |||||||||||||||
* Constant surface field
Special notes:
Spectra
Controls
Normalize at:
Normalize by mean flux
Range:
x:
to
y:
to
Spectra available:
Spectra without link are available upon request
Absorption lines
Photometric filters
BVRI
ugriz
Photometric fit
