spectral type double star; both stars are white. Overall, it appears to be of magnitude 3.6 and luminosity of . The primary has a magnitude of 4.53 and the secondary a magnitude of 4.31, but both have an absolute magnitude of 0.6. Its orbital period is 760 years; the two components are currently moving farther apart. θ Aquarii, sometimes called Ancha, is a G8 spectral type star with an apparent magnitude of 4.16 and an absolute magnitude of 1.4. κ Aquarii, also called Situla, has an apparent magnitude of 5.03. λ Aquarii, also called Hudoor or Ekchusis, is an M2 spectral type star of magnitude 3.74 and luminosity of . ξ Aquarii, also called Bunda, is an A7 spectral type star with an apparent magnitude of 4.69 and an absolute magnitude of 2.4. π Aquarii, also called Seat, is a B0 spectral type star with an apparent magnitude of 4.66 and an absolute magnitude of −4.1. Planetary systems Twelve exoplanet systems have been found in Aquarius as of 2013. Gliese 876, one of the nearest stars to Earth at a distance of 15 light-years, was the first red dwarf star to be found to possess a planetary system. It is orbited by four planets, including one terrestrial planet 6.6 times the mass of Earth. The planets vary in orbital period from 2 days to 124 days. 91 Aquarii is an orange giant star orbited by one planet, 91 Aquarii b. The planet's mass is 2.9 times the mass of Jupiter, and its orbital period is 182 days. Gliese 849 is a red dwarf star orbited by the first known long-period Jupiter-like planet, Gliese 849 b. The planet's mass is 0.99 times that of Jupiter and its orbital period is 1,852 days. There are also less-prominent systems in Aquarius. WASP-6, a type G8 star of magnitude 12.4, is host to one exoplanet, WASP-6 b. The star is 307 parsecs from Earth and has a mass of 0.888 solar masses and a radius of 0.87 solar radii. WASP-6 b was discovered in 2008 by the transit method. It orbits its parent star every 3.36 days at a distance of 0.042 astronomical units (AU). It is 0.503 Jupiter masses but has a proportionally larger radius of 1.224 Jupiter radii. HD 206610, a K0 star located 194 parsecs from Earth, is host to one planet, HD 206610 b. The host star is larger than