24 Sextanis

Pre Astro Earth
24 Sextantis (often shortened to 24 Sex) is a 7th-magnitude star located approximately 253 light years away in the constellation of Sextans. At an apparent visual magnitude of 6.61, this star can only be viewed from rural skies under good seeing conditions.

At the age of 2.8 billion years, it has reached an evolutionary stage called a subgiant star, having a stellar classification of G5 IV. Previously it was an A-type main sequence star before using up the hydrogen at its core. It has 54% more mass than the Sun, but the outer envelope has become cooler than the Sun's as it slowly expands into a giant star.

The star is known to have two giant extrasolar planets.

On July 26, 2010 the California and Carnegie Planet Search team announced the discovery of two planets around 24 Sextantis along with two planets around HD 200964. The inner planet is twice as massive as Jupiter and takes 453 days to orbit the star in a circular orbit at the average distance of 1.33 AU (199 Gm). The outer planet is 5/6 the mass of Jupiter and takes 883 days to orbit eccentrically around the star at the average distance of 2.08 AU (312 Gm).

The two planets are in a 2:1 resonance, meaning that the outer planet orbits the star once every time when the inner planet orbits the star twice. These two jovian planets are dancing around each other gravitationally.

Post Astro -After the Ascent
The planetary system is 253 light years from Sol but only 89 from Luxor and has been claimed by the Sarans for over 2000 years. The Saran name is the one used in Union Astrographic catalogs, as Hammarubis.

The system has 7 planets, 11 planetoids and a number of moons - For detailed system infornation see "Hammarubis "