WASP-8

WASP-8 is a binary star system 294 light-years (90 parsecs) away. The star system is much younger than the Sun at 300 million to 1.2 billion years age, and is heavily enriched in heavy elements, having nearly twice the concentration of iron compared to the Sun.

WASP-8

Artist's impression of a star like WASP-8
Observation data
Epoch J2000      Equinox J2000
Constellation Sculptor
Right ascension 23h 59m 36.07119s
Declination −35° 01 52.9236
Apparent magnitude (V) 9.87
Characteristics
WASP-8A
Evolutionary stage main-sequence
Spectral type G8V
WASP-8B
Spectral type M
Astrometry
Radial velocity (Rv)−1.38±0.26 km/s
Proper motion (μ) RA: 109.752 mas/yr
Dec.: 7.615 mas/yr
Parallax (π)11.1052 ± 0.0175 mas
Distance293.7 ± 0.5 ly
(90.0 ± 0.1 pc)
Position (relative to WASP-8A)
ComponentWASP-8B
Epoch of observation2016
Angular distance4.520±0.005
Position angle170.9±0.1°
Projected separation408 AU
Details
WASP-8A
Mass1.093±0.024 M
Radius0.976±0.020 R
Luminosity0.79 L
Surface gravity (log g)4.498±0.018 cgs
Temperature5600±80 K
Metallicity [Fe/H]0.29±0.03 dex
Rotational velocity (v sin i)1.90±0.05 km/s
Age0.3+0.9
−0.1
 Gyr
WASP-8B
Mass0.53±0.02 M
Temperature3758+47
−43
 K
Other designations
CD−35 16019, CPD−35 9465, SAO 214901, PPM 304426, WDS J23596-3502A, TOI-191, TIC 183532609, WASP-8, TYC 7522-505-1, 2MASS J23593607-3501530
Database references
SIMBADA
B

The primary, WASP-8A, is a magnitude 9.9 main-sequence yellow dwarf star. It is reported to be a G-type star with a temperature of 5600 K and has a mass 1.093±0.024, a radius 0.976±0.020 and a luminosity of 0.79 times that of the Sun. There is a companion star WASP-8B located 4.5 arcseconds away with the same proper motion, indicating a stellar binary system. The binarity was confirmed in 2020. The axis orientation of the primary star is uncertain, but it is close to pointing one of the poles to the Earth.

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