Epsilon Hydri, Latinized from ε Hydri, is a single,[8] blue-white hued star in the southern constellation of Hydrus. It is a faint star with an apparent visual magnitude of 4.12,[2] but it can be seen with the naked eye. Measurements made by the Hipparcos spacecraft showed an annual parallax shift of 21.48 mas,[1] which provides a distance estimate of 152 light years. The star is moving away from the Sun with a radial velocity of +13.6 km/s.[4] It is a member of the Tucana-Horologium moving group, an association of stars that share a common motion through space.[9]
The stellar classification for this star is B9 Va,[2] indicating that is it a B-type main-sequence star that is generating energy through hydrogen fusion at its core. It is a young star, just 133[7] million years in age, and has a high rate of spin with a projected rotational velocity of 96 km/s.[5] This is giving the star a mild oblate shape with an equatorial bulge that is 5% greater than the polar radius.[10] Epsilon Hydri has an estimated 2.64 times the mass of the Sun and 2.2 times the Sun's radius.[5] It is radiating 60[5] times the Sun's luminosity from its photosphere at an effective temperature of around 10,970 K.[7]