HD 154857 b

HD 154857 b is an exoplanet orbiting the yellow dwarf HD 154857 . It was discovered using the radial velocity method (publication by McCarthy et al. In 2004). The exoplanet orbits the central star with a period of 398.5  days at a distance of approx. 1.1 astronomical units and has a minimum mass of approx. 1.9 Jupiter's masses.

Web link

• The exoplanet in the "Encyclopedia of Extrasolar Planets"