WASP-8b

Planet orbiting a star in a binary system in the constellation of Sculptor From Wikipedia, the free encyclopedia

WASP-8b is an exoplanet orbiting the star WASP-8A in the constellation of Sculptor. The star is similar to the Sun and forms a binary star with a red dwarf star (WASP-8B) of half the Sun's mass that orbits WASP-8A 4.5 arcseconds away. The system is 294 light-years (90 parsecs) away and is therefore located closer to Earth than many other star systems that are known to feature planets similar to WASP-8b. The planet and its parent star were discovered in the SuperWASP batch -6b to -15b. On 1 April 2008, Dr. Don Pollacco of Queen's University Belfast announced them at the RAS National Astronomy Meeting (NAM 2008).[5]

DiscoveredbyCameron et al. (SuperWASP)
DiscoverydateApril 1, 2008
0.0817±0.0006 AU[3]
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WASP-8b
Size comparison of WASP-8b with Jupiter.
Discovery[1]
Discovered byCameron et al. (SuperWASP)
Discovery dateApril 1, 2008
Transit
Orbital characteristics[2]
0.0817±0.0006 AU[3]
Eccentricity0.3057±0.0046
8.158715±0.000016 d
Inclination88.51°±0.09°[3]
274.21°±0.33°
Semi-amplitude221.65±1.39 m/s
StarWASP-8
Physical characteristics[3]
1.165±0.032 RJ
Mass2.216±0.035 MJ
Mean density
1.7370±0.1325 g/cm3
42.5±2.3 m/s2 (4.34 g)
Temperature1552±85 K (1,279 °C; 2,334 °F)[4]
    Close

    Orbit

    The planet orbits WASP-8A at an average distance of just 0.08 AU (12,000,000 km) and a year passes in slightly more than 8.1 days on WASP-8b, which is somewhat farther from its parent star than other hot Jupiter planets. However, WASP-8b's orbit also has a relatively high eccentricity of 0.3, which, at periastron, brings it as close to its star as said similar planets are.

    One thing that stands out extremely about WASP-8b is its orbit-spin angle to its star of 123°+3.4°
    −4.4°
    : This implies that the planet actually orbits retrograde to the spin of the parent star.[6][1][7]

    Physical characteristics

    WASP-8b belongs to a class of extrasolar planets known as hot Jupiters and has a mass about 2.2 times and a radius slightly bigger than that of the planet Jupiter. Its density is about 1.737 g/cm3; this implies that, unlike similar close-orbiting gas giants, the planet is actually denser than Jupiter (which has a density of 1.326 g/cm3).[8]

    Owing to its close distance to its star, WASP-8b is extremely hot: Its measured dayside temperature is 1,552 K (1,279 °C), this is even hotter than its equilibrium temperature of 947 K (674 °C).[8][4]

    See also

    References

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