WASP-8

WASP-8 is a magnitude 9.9 main-sequence yellow dwarf star. It is reported to be a G-type star of temperature 5600 K, mass of 0.93 solar masses, radius of 0.93 solar radius, and a luminosity of 0.79 of solar luminosity. There is a companion star located 4 arcseconds away with the same proper motion indicating a stellar binary system.[3]

WASP-8
Observation data
Epoch J2000      Equinox J2000
Constellation Sculptor
Right ascension  23h 59m 36.0711s[1]
Declination −35° 01 52.920[1]
Apparent magnitude (V) 9.9
Characteristics
Spectral type G6
Astrometry
Proper motion (μ) RA: 109.878±0.571[1] mas/yr
Dec.: 7.370±0.615[1] mas/yr
Parallax (π)11.20 ± 0.27[1] mas
Distance291 ± 7 ly
(89 ± 2 pc)
Details
Mass0.93 M
Radius0.93 R
Luminosity0.79 L
Temperature5600 K
Rotational velocity (v sin i)1.90±0.05[2] km/s
Age3–5[3] Gyr
Other designations
TYC 7522-505-1, WDS J23596-3502A[4]
Database references
SIMBADdata

Planetary system

The star is orbited by two known extrasolar planet, designated WASP-8b and WASP-8c. They was catalogued as part of the SuperWASP mission and discovered by the astronomical transit method.[3] WASP-8c has the longest orbital period of any exoplanet discovered by WASP with a period of 4,323 days, over 400 times the period of the second-furthest planet, WASP-117b with a period of 10.02 days.

Measurements of WASP-8b's radius and mass give it an estimated density of 2.53 g/cm3, about twice the density of Jupiter.

The WASP-8 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 2.23 MJ 0.0793 8.16 0.3082 88.52° 1.17 RJ
c 9.45 MJ 5.28 4323

See also

Artist's impression of a star like WASP-8.

References


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