WASP-103

WASP-103 is an F-type main-sequence star located 1,800 ± 100 light-years (550 ± 30 parsecs) away in the constellation Hercules. Its surface temperature is 6,110±160 kelvins (K). The star's concentration of heavy elements is similar to that of the Sun. WASP-103 is slightly younger than the Sun at 4±1 billion years. The chromospheric activity of the star is elevated due to interaction with the giant planet on a close-in orbit.

WASP-103
Observation data
Epoch J2000      Equinox J2000
Constellation Hercules
Right ascension 16h 37m 15.5766s
Declination 07° 11 00.110
Apparent magnitude (V) 12.1
Characteristics
Evolutionary stage main-sequence star
Spectral type F8V
Astrometry
Radial velocity (Rv)−40.69±1.00 km/s
Proper motion (μ) RA: −9.756 mas/yr
Dec.: 2.779 mas/yr
Parallax (π)1.8332 ± 0.1073 mas
Distance1,800 ± 100 ly
(550 ± 30 pc)
Details
Mass1.220+0.039
0.036
 M
Radius1.436+0.052
0.031
 R
Luminosity3.3 L
Surface gravity (log g)4.35±0.02 cgs
Temperature6110±160 K
Metallicity [Fe/H]0.06±0.13 dex
Rotational velocity (v sin i)10.60±0.90 km/s
Age4±1 Gyr
Other designations
Gaia DR2 4439085988769170432, 2MASS J16371556+0711000
Database references
SIMBADdata

A multiplicity survey in 2015 found a suspected stellar companion to WASP-103, at a projected separation of 0.242±0.016.

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