HAT-P-8

HAT-P-8 is a magnitude 10 star located 700 light-years away in Pegasus. It is a F-type star about 28% more massive than the Sun. Two red dwarf companions have been detected around HAT-P-8. The first has a spectral type of M5V and has a mass of 0.22 M. The second is even less massive, at 0.18 M, and its spectral type is M6V.

HAT-P-8
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Pegasus
Right ascension 22h 52m 09.8636s
Declination +35° 26 49.608
Apparent magnitude (V) 10.17
Characteristics
Spectral type F
Apparent magnitude (B) 10.77 ± 0.04
Apparent magnitude (V) 10.36 ± 0.03
Apparent magnitude (J) 9.214 ± 0.022
Apparent magnitude (H) 9.004 ± 0.018
Apparent magnitude (K) 8.953 ± 0.013
Variable type planetary transit
Astrometry
Radial velocity (Rv)−22.2±0.3 km/s
Proper motion (μ) RA: 74.676(19) mas/yr
Dec.: 14.944(20) mas/yr
Parallax (π)4.6606 ± 0.0208 mas
Distance700 ± 3 ly
(214.6 ± 1.0 pc)
Details
Mass1.27±0.03 M
Radius1.491+0.016
0.014
 R
Surface gravity (log g)4.1956+0.0095
0.013
 cgs
Temperature6410±140 K
Metallicity [Fe/H]-0.018+0.0072
0.056
 dex
Rotational velocity (v sin i)12.6 ± 1.0 km/s
Age3.4 ± 1 Gyr
Other designations
Gaia DR3 1891507552826485632, TYC 2757-1152-1, GSC 02757-01152, 2MASS J22520985+3526495
Database references
SIMBADdata
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.