HD 219415 is a star with 1 times the mass of the Sun, and 2.9 times its radius. It is located 538.76 light years away from the solar system.
HD 219415 is known to have 1 exoplanets in orbit around it.
HD 219415 b was discovered by the McDonald Observatory observatory, in 2012-09, using the radial velocity method. Its semi-major axis is 3.20 astronomical units, as compared to Earth's which is 1 astronomical unit. The mass of HD 219415 b is 318.000 times the mass of Earth. The radius of HD 219415 b is 13.800 that of Earth. At more than 50 Earth masses, HD 219415 b is a gas giant, a planet whose mass is mostly made up of hydrogen and helium, like Jupiter and Saturn in our solar system.