PSR B1620-26

PSR B1620-26 is a binary star located at the distance of 12,400 light-years, It is located in the Globular cluster Messier 4. It is located in the constellation Scorpius.
System
Viewed as a binary star system, PSR B1620-26 is very far away, being 3,800 parsecs (12,400light-years) outside the core of Messier 4. It consists if two stars, PSR B1620-26 A is a pulsar and PSR B1620-26 B is a white dwarf (which form a binary star system together) and a exoplanet PSR B1620-26 b which according to astronomers is the oldest planet in the universe.
White Dwarf
PSR B1620-26 B is 0.34 solar masses and orbits the pulsar every 191 days.
Planetary system
PSR B1620-26 b was discovered in the early 1990s. The planet was announced by Stephen Thorsett and his collaborators in 1993.
| Companion
(in order from star) |
Mass | Semimajor axis
(AU) |
Orbital period | Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 2.5 ± 1 MJ | 23 | ~36,500 | low | 55−8+14° | — |