PSR B1620-26 is a star with 1.35 times the mass of the Sun, and NaN times its radius. It is located NaN light years away from the solar system.
PSR B1620-26 is known to have 1 exoplanets in orbit around it.
PSR B1620-26 b was discovered by the Hubble Space Telescope observatory, in 2003-07, using the pulsar timing method. Its semi-major axis is 23.00 astronomical units, as compared to Earth's which is 1 astronomical unit. The mass of PSR B1620-26 b is 795.000 times the mass of Earth. The radius of PSR B1620-26 b is 13.300 that of Earth. At more than 50 Earth masses, PSR B1620-26 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.