EPS HYA (Epsilon Hydrae). One of the more obscure constellations of the sky, Hydra (the Water Serpent) is known mostly for its bright Alpha star, Alphard, which lies to the south and a bit west of Regulus in Leo. South of Cancer lies the Water Serpent's head, made of a tiny distorted circlet whose stars are (from Arabic) collectively called (from Allen) "Min al Az'al, belonging to the uninhabited spot." None of the stars, including Bayer's Epsilon, has a proper name to itself, though Epsilon is singled out as the most northerly of them (while beat out in brightness by Zeta just to the east of it). Appearing undistinguished to the eye, "Eps Hya" is a remarkable multiple star with at least five members. The principal star is a fourth magnitude yellow-white class G (G5) giant that has a very close (0.2 seconds of arc away) white class A (A5) subgiant fifth magnitude (4.7) companion that together make the third magnitude (3.38) naked eye star. They orbit each other every 15.05 years at an average separation of 10.5 Astronomical Units, about the distance of Saturn from the Sun, on an eccentric path that takes them from 17.4 AU to as close as 3.6 AU (that point passed in 1991). The orbit gives the two a total mass of 5.1 times that of the Sun. The G star, at 4900 Kelvin, shines with a light of 57 solar, the A star (at 7700 Kelvin) 17 solar, which gives it a mass of double the Sun (and showing that it is really a hydrogen-fusing dwarf). The G star therefore contains 3 solar masses, which makes it a "transition star" with a dead helium core that is preparing to become a brighter giant. The G star is somewhat magnetically active, and has been detected as an X-ray source. Separated from this close double by 4.5 seconds of arc is a class F (F5) dwarf that takes 900 years to orbit the inner pair at a distance of about 190 AU. At 6600 Kelvin, it shines 2.5 times as brightly as does the Sun, but carries just over a solar mass. It too is double, its components even closer, just 0.09 AU in a period of a mere 9.9 days. Farther out (19 seconds of arc away) is a dim 10th magnitude star that orbits the inner quartet. From its brightness, it must be a class M dwarf with about a third of a solar mass. Physically some 800 AU away, it must take close to 10,000 years to make a full circuit. In a loose way, the system is similar in structure to Mizar and Alcor in Ursa Major, with an inner double-double and an outlier, though there is some indication that Epsilon Hydrae may have yet another member. From the closer pair, the brighter pair would have a separation of some three degrees, the G star shining with the light of 500 full Moons. From the brighter pair, the closer pair would be just resolvable with the human eye.
Written by Jim Kaler. Return to STARS.