14 Herculis. Image: Digitized Sky Survey.
14 Herculis is an orange-yellow K-star around which an exoplanet 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. The discovery of second possible planet around 14 Herculis was announced in 2005.
|distance||59 light-years (18.1 pc)|
|temperature||4,980 °C (5,250 K)|
|position||RA 16h 10m 24.3s, Dec +43° 49' 03.5"|
|other designations||HD 145675, HIP 79248, Gl 614, BD+44 2549|
|mass (Jupiter=1)||4.74 ± 0.06|
|semimajor axis||2.8 AU (420 million km, 260 million mi)|
|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|