In 2006 a long-period planet was discovered.

The star is known to possess one long-period extrasolar planet.

Unlike many long-period extrasolar planets, it has a low orbital eccentricity.

It was the first long-period planet around a main sequence star to be discovered.

These observation sessions, called "Long Runs", allow detection of smaller and long-period planets.

In June 2002, a massive long-period planet orbiting the star was announced.

As typical for long-period planets discovered around other stars, it has an orbital eccentricity greater than that of Jupiter.

It is a long-period planet, taking seven and a half years to orbit the star at the average distance of 3.60 AU.

As it is typical for long-period planets, it has a relatively high eccentricity of 53 20%.

As it is typical for long-period planets, this planet orbits in an eccentric path.