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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, … 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) … See more

    Charbonneau, D. (2003). "HD 209458 and the Power of the Dark Side". In Deming, Drake; Seager, Sara (eds.). Scientific Frontiers in Research on Extrasolar Planets. ASP Conference Series. Vol. 294. San Francisco: ASP. pp. 449–456. 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, updated the spin-orbit angle to −5±7°. 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 … 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 magnetic fields See more

     
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  9. People also ask
    What type of star is HD 209458?The spectrum of HD 209458 presents as a late F- or early G-type main-sequence star with a stellar classification of F9 V or G0 V, respectively. It is roughly 3.5 billion years old and is spinning with a projected rotational velocity of 4.2 km/s. The star displays a moderate amount of magnetic activity in its chromosphere.
    en.wikipedia.org
    What is HD 209458 b?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 million km )).
    en.wikipedia.org
    How did HD 209458b get its name?Soon after the discovery, separate teams led by David Charbonneau and Gregory W. Henry were able to detect a transit of the planet across the surface of the star making it the first known transiting extrasolar planet. The planet received the designation HD 209458 b .
    en.wikipedia.org
    Is HD 209458 a planet?HD 209458 is a seventh- magnitude star about 150 light-years away in the constellation Pegasus. The star, which has physical characteristics similar to those of the Sun, was shown in late 1999 to have a planet, HD 209458b, by detection of the planet’s gravitational effects on the star’s motion.
    When was HD 209458 b discovered?Its discovery was announced in 1999. HD 209458 b is a gas giant exoplanet that orbits a F-type star. Its mass is 0.73 Jupiters, it takes 3.5 days to complete one orbit of its star, and is 0.04707 AU from its star. Its discovery was announced in 1999.
    Is HD 209458 visible?HD 209458 is a star with an orbiting exoplanet in the constellation Pegasus. It has an apparent visual magnitude of 7.65 and an absolute magnitude of 4.28. Because it is located at a distance of 157 light-years (48 parsecs) from the Sun as measured via parallax, it is not visible to the unaided eye.
    en.wikipedia.org
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