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WASP-10b is an extrasolar planet discovered in 2008 by SuperWASP using the transit method.It takes about 3 days to orbit around WASP-10.Follow-up radial velocity observations showed that it is three times more massive than Jupiter, while the transit observations showed that its radius is only 8% larger than Jupiter's, giving the planet a density more similar to the Moon than a normal gas giant.
WASP-11b/HAT-P-10b or WASP-11Ab/HAT-P-10Ab [3] is an extrasolar planet discovered in 2008. The discovery was announced (under the designation WASP-11b) by press release by the SuperWASP project in April 2008 along with planets WASP-6b through to WASP-15b, however at this stage more data was needed to confirm the parameters of the planets and the coordinates were not given. [4]
WASP-10 is a star in the constellation Pegasus.The SuperWASP project has observed and classified this star as a variable star, perhaps due to the eclipsing planet. [2]The star is likely older than Sun, has fraction of heavy elements close to solar abundance, and is rotating rapidly, being spun up by the tides raised by the giant planet on the close orbit.
WASP or Wide Angle Search for Planets is an international consortium of several academic organisations performing an ultra-wide angle search for exoplanets using transit photometry. The array of robotic telescopes aims to survey the entire sky, simultaneously monitoring many thousands of stars at an apparent visual magnitude from about 7 to 13.
WASP-178b, also known as KELT-26b and HD 134004 b, is an ultra-hot Jupiter exoplanet discovered in 2019 orbiting WASP-178, a hot A-type star located about 1,350 light-years (410 parsecs) away in the constellation of Lupus. At over 1.8 times the radius of Jupiter, it is among the largest exoplanets.
WASP-3b is an extrasolar planet orbiting the star WASP-3 located approximately 800 light-years away in the constellation Lyra. It was discovered via the transit method by SuperWASP , and follow up radial velocity observations confirmed that WASP-3b is a planet.
WASP-33b is an extrasolar planet orbiting the star HD 15082. It was the first planet discovered to orbit a Delta Scuti variable star. With a semimajor axis of 0.026 AU (3.9 million km ; 2.4 million mi ) and a mass likely greater than Jupiter 's, [ 1 ] it belongs to the hot Jupiter class of planets.
WASP-28b or K2-1b is an extrasolar planet discovered in 2010 [4] by the Wide Angle Search for Planets (WASP) project orbiting WASP-28, a magnitude 12 star also known as 1SWASP J233427.87-013448.1, 2MASS J23342787-0134482 and K2-1. [5] [1] Since it orbits its star very closely, the planet is a strongly irradiated hot Jupiter. [1]