"This gas giant has two times Jupiter's Radius but only one half of its mass. The unusually low density is thought to be a consequence of a combination of the planet's orbital eccentricity and its proximity to its parent star, leading to tidal flexing and heating of its interior."@en . "WASP-17b-main.jpg"@en . . "284681.16"^^ . "Infinity"^^ . "1200.0"^^ . "2735.0"^^ . "The SuperWASP consortium"@en . "1.0"^^ . . "0.3105"^^ . "1.14"^^ . "*95.3% He \n*3.77% CH4 \n*0.428 N2 \n*0.292% NH3"@en . "0.98"^^ . . "322704.0"^^ . . "WASP-17 b"@en . . "WASP-17 b"@en . "None"@en . "WASP-17 b"@en . "None"@en . "0.48656"^^ .