HAT-P-23

HAT-P-23 / Moriah
Observation data
Epoch J2000      Equinox J2000
Constellation Delphinus
Right ascension 20h 24m 29.7235s
Declination +16° 45 43.812
Apparent magnitude (V) 11.94
Characteristics
Evolutionary stage main sequence
Spectral type G0
Apparent magnitude (J) 11.103±0.022
Apparent magnitude (H) 10.846±0.022
Apparent magnitude (K) 10.791±0.020
Variable type Planetary transit
Astrometry
Radial velocity (Rv)−16.67±0.88 km/s
Proper motion (μ) RA: 13.325(11) mas/yr
Dec.: −5.505(11) mas/yr
Parallax (π)2.7358±0.0108 mas
Distance1,192 ± 5 ly
(366 ± 1 pc)
Details
Mass1.13±0.035 M
Radius1.203±0.074 R
Luminosity1.58±0.23 L
Surface gravity (log g)4.33±0.05 cgs
Temperature5905±80 K
Metallicity0.15±0.04
Rotation7.015 d
Rotational velocity (v sin i)8.1±0.5 km/s
Age4.0±1.0 Gyr
Other designations
Moriah, TYC 1632-1396-1, GSC 01632-01396, 2MASS J20242972+1645437
Database references
SIMBADdata
Exoplanet Archivedata

HAT-P-23 is a G-type main-sequence star 1192 light-years away. It has a rapid rotation (rotation period equal to 7 days) for its advanced age of 4 billion years, and exhibits a strong starspot activity. The star may be in the process of being spun up by the giant planet on close orbit. The star is enriched in heavy elements, having about 140% amount of metals compared to solar abundance.