HAT-P-23

HAT-P-23 is a G-type main-sequence star about 1200 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.

HAT-P-23 / Moriah
Observation data
Epoch J2000      Equinox J2000
Constellation Delphinus
Right ascension 20h 24m 29.7235s
Declination +16° 45 43.8103
Apparent magnitude (V) 11.94
Characteristics
Spectral type G0V
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)-14.324 km/s
Proper motion (μ) RA: 13.263±0.050 mas/yr
Dec.: −5.412±0.049 mas/yr
Parallax (π)2.7129 ± 0.0351 mas
Distance1,200 ± 20 ly
(369 ± 5 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, Gaia DR2 1808938730710633984, TYC 1632-1396-1, GSC 01632-01396, 2MASS J20242972+1645437
Database references
SIMBADdata
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