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    HD 209458 b - Wikipedia

    HD 209458 b is an exoplanet that orbits the solar analog HD 209458 in the constellation Pegasus, some 157 light-years (48 parsecs) from the Solar System. The radius of the planet's orbit is 0.047 AU (7.0 million km; 4.4 million mi), or one-eighth the radius of Mercury's orbit (0.39 AU (36 million mi; 58 … See more

    Transits
    Spectroscopic studies first revealed the presence of a planet around HD 209458 on November 5, 1999. Astronomers had made careful photometric measurements of several stars … See more

    Magnetic field image

    In 2014, a magnetic field around HD 209458 b was inferred from the way hydrogen was evaporating from the planet. It is the first (indirect) detection of a magnetic field on an exoplanet. The magnetic field is estimated to be about one tenth as strong as … See more

    Physical characteristics image
    Overview image

    In August 2008, the measurement of HD 209458 b's Rossiter–McLaughlin effect and hence spin–orbit angle is −4.4 ± 1.4°.
    The study in 2012, … See more

    Stratosphere and upper clouds
    The atmosphere is at a pressure of one bar at an altitude of 1.29 Jupiter radii above the planet's center.
    Where the pressure … See more

    51 Pegasi b
    YZ Ceti another extra solar planet with evidence of magnetic fields
    HAT-P-11b another extra solar planet with evidence of … See more

    Charbonneau, D. (2003). "HD 209458 and the Power of the Dark Side". In Deming, Drake; Seager, Sara (eds.). Scientific Frontiers in … See more

     
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