HAT-P-15

Star in the constellation Perseus From Wikipedia, the free encyclopedia

HAT-P-15 is a G-type main-sequence star about 630 light-years away. The star is older than Sun yet has a concentration of heavy elements roughly 190% of solar abundance.[5] The star has no noticeable starspot activity.[7]

Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HAT-P-15 / Berehynia
Observation data
Epoch J2000      Equinox J2000
Constellation Perseus[1]
Right ascension 04h 24m 59.5350s[2]
Declination +39° 27 38.313[2]
Apparent magnitude (V) 12.41[3]
Characteristics
Spectral type G5V[citation needed]
Variable type planetary transit[4]
Astrometry
Radial velocity (Rv)31.21 km/s
Proper motion (μ) RA: 14.233(21)[2] mas/yr[2]
Dec.: −9.407(15)[2] mas/yr[2]
Parallax (π)5.1856±0.0166 mas[2]
Distance629 ± 2 ly
(192.8 ± 0.6 pc)
Details[5]
Mass1.013±0.043 M
Radius1.080±0.039 R
Luminosity1.00±0.11 L
Surface gravity (log g)4.38±0.03 cgs
Temperature5684±25 K
Metallicity0.272±0.031
Rotational velocity (v sin i)2.0±0.5 km/s
Age6.8+2.5
1.6
 Gyr
Other designations
Berehynia, TYC 2883-1687-1, GSC 02883-01687, 2MASS J04245952+3927382, Gaia DR3 179498266829041664[6]
Database references
SIMBADdata
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The spectroscopic survey in 2015 have failed to find any stellar companions to it,[8] yet imaging survey have identified a possibly two companion red dwarf stars at projected separations 1210 and 1370 AU, respectively.[9]

The star was named Berehynia in December 2019 by Ukrainian amateur astronomers.[10]

Planetary system

In 2010 a transiting hot superjovian planet b (named Tryzub in 2019[10]) was detected. It has an equilibrium temperature of 904±20 K.[4] An orbital simulation shows that any planets inward of the orbit of b would spiral inward and be destroyed within a time-span of less than a billion years.[11] The planetary orbit is well aligned with the equatorial plane of the star, misalignment equal to 13±6 degrees.[12]

Size comparison of HAT-P-15 b and Jupiter
More information Companion (in order from star), Mass ...
The HAT-P-15 planetary system[4]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination
(°)
Radius
b / Tryzub 1.946±0.066 MJ 0.0964±0.0014 10.863502±0.000027 0.19±0.019 89.1±0.2 1.072±0.043 RJ
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References

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