GSC 03089-00929

GSC 03089-00929 / Pipoltr

A light curve for V1434 Herculis, plotted from TESS data, the 1.306 day interval between planet transits is shown in red.
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Hercules
Right ascension 17h 52m 07.0184s
Declination +37° 32 46.237
Apparent magnitude (V) 12.402
Characteristics
Spectral type G
Apparent magnitude (B) 13.114 ±0.009
Apparent magnitude (V) 12.402 ±0.006
Apparent magnitude (I) 11.603 ±0.010
Apparent magnitude (J) 11.015 ±0.022
Apparent magnitude (H) 10.655 ±0.030
Apparent magnitude (K) 10.608 ±0.028
Variable type planetary transit
Astrometry
Radial velocity (Rv)10.30±0.96 km/s
Proper motion (μ) RA: −24.462(10) mas/yr
Dec.: 34.772(11) mas/yr
Parallax (π)4.3106±0.0091 mas
Distance757 ± 2 ly
(232.0 ± 0.5 pc)
Absolute magnitude (MV)5.39±0.11
Details
Mass0.928+0.028
−0.048
 M
Radius0.826±0.012 R
Luminosity0.625+0.066
−0.058
 L
Surface gravity (log g)4.57±0.01 cgs
Temperature5650±75 K
Metallicity [Fe/H]−0.19±0.08 dex
Rotational velocity (v sin i)1.5±1.0 km/s
Age0.9+2.8
−0.8
 Gyr
Other designations
Pipoltr, TrES-3 Parent Star, V1434 Her, TOI-2126, TIC 116264089, GSC 03089-00929, 1SWASP J175207.01+373246.3, UCAC2 45017453
Database references
SIMBADdata
Exoplanet Archivedata

GSC 03089-00929, also known as V1434 Herculis and named Pipoltr, is a magnitude 12 star located approximately 757 light-years away in the constellation of Hercules. This star is a G-type main sequence star that is similar to but slightly cooler than the Sun. This star is identified in SIMBAD as a variable star per the 1SWASP survey. It hosts one known exoplanet, TrES-3b.