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    14 Herculis

    14 Herculis
    14 Herculis
    Image: Digitized Sky Survey
    An orange-yellow K-star around which an extrasolar planet has been found. The heavy element abundance of 14 Herculis is greater than that of the Sun and the discovery that it has a massive planet lends support to the idea that such large worlds tend to form in heavy element enriched environments. The planetary companion of 14 Herculis has a mass almost five times that of Jupiter and moves in an eccentric orbit about its host star with a period of 4.9 years. This puts it in the category of classical jovians along with the companion of 47 Ursae Majoris, which it most closely resembles. The discovery of second possible planet around 14 Herculis was announced in 2005.


    Host star
    Distance 59 light-years (18.1 pc)
    Spectral type K0V
    Apparent magnitude 6.67
    Temperature 4,980 °C (5,250 K)
    Luminosity (Sun=1) 0.75
    Mass (Sun =1) 0.79
    Metallicity ([Fe]/[H]) 0.35
    Position R.A. 16h 10m 24.3s, Dec. +43° 49' 03.5"
    Other designations HD 145675, HIP 79248, Gl 614, BD+44 2549


    Planet
    Mass (Jupiter=1) 4.74 ± 0.06
    Semimajor axis 2.8 AU (420 million km, 260 million miles)
    Orbital period 1796.4 ± 8.3 days
    Eccentricity 0.338 ± 0.011
    Discovery 1998, Mayor et al (Geneva), Haute-Provence Observatory
    Method of discovery radial velocity


    Related categories

       • NOTABLE STARS
       • EXTRASOLAR PLANETS



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