Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Perseus |
Right ascension | 04h 24m 59.5350s [1] |
Declination | +39° 27′ 38.313″ [1] |
Apparent magnitude (V) | 12.41 |
Characteristics | |
Spectral type | G5V |
Variable type | planetary transit [2] |
Astrometry | |
Radial velocity (Rv) | 31.21 km/s |
Proper motion (μ) |
RA: 14.233(21)
mas/
yr
[1] Dec.: −9.407(15) mas/ yr [1] |
Parallax (π) | 5.1856 ± 0.0166 mas [1] |
Distance | 629 ± 2
ly (192.8 ± 0.6 pc) |
Details [3] | |
Mass | 1.013±0.043 M☉ |
Radius | 1.080±0.039 R☉ |
Luminosity | 1.00±0.11 L☉ |
Surface gravity (log g) | 4.38±0.03 cgs |
Temperature | 5684±25 K |
Metallicity | 0.272±0.031 |
Rotational velocity (v sin i) | 2.0±0.5 km/s |
Age | 6.8+2.5 −1.6 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
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. [3] The star has no noticeable starspot activity. [5]
The spectroscopic survey in 2015 have failed to find any stellar companions to it, [6] yet imaging survey have identified a possibly two companion red dwarf stars at projected separations 1210 and 1370 AU, respectively. [7]
The star was named Berehynia in December 2019 by Ukrainian amateur astronomers. [8]
In 2010 a transiting hot superjovian planet b (named Tryzub in 2019 [8]) was detected. It has an equilibrium temperature of 904±20 K. [2] 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. [9] The planetary orbit is well aligned with the equatorial plane of the star, misalignment equal to 13±6 degrees. [10]
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 |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Perseus |
Right ascension | 04h 24m 59.5350s [1] |
Declination | +39° 27′ 38.313″ [1] |
Apparent magnitude (V) | 12.41 |
Characteristics | |
Spectral type | G5V |
Variable type | planetary transit [2] |
Astrometry | |
Radial velocity (Rv) | 31.21 km/s |
Proper motion (μ) |
RA: 14.233(21)
mas/
yr
[1] Dec.: −9.407(15) mas/ yr [1] |
Parallax (π) | 5.1856 ± 0.0166 mas [1] |
Distance | 629 ± 2
ly (192.8 ± 0.6 pc) |
Details [3] | |
Mass | 1.013±0.043 M☉ |
Radius | 1.080±0.039 R☉ |
Luminosity | 1.00±0.11 L☉ |
Surface gravity (log g) | 4.38±0.03 cgs |
Temperature | 5684±25 K |
Metallicity | 0.272±0.031 |
Rotational velocity (v sin i) | 2.0±0.5 km/s |
Age | 6.8+2.5 −1.6 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
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. [3] The star has no noticeable starspot activity. [5]
The spectroscopic survey in 2015 have failed to find any stellar companions to it, [6] yet imaging survey have identified a possibly two companion red dwarf stars at projected separations 1210 and 1370 AU, respectively. [7]
The star was named Berehynia in December 2019 by Ukrainian amateur astronomers. [8]
In 2010 a transiting hot superjovian planet b (named Tryzub in 2019 [8]) was detected. It has an equilibrium temperature of 904±20 K. [2] 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. [9] The planetary orbit is well aligned with the equatorial plane of the star, misalignment equal to 13±6 degrees. [10]
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 |