Iota Aquarii
Iota Aquarii, Latinized from ι Aquarii, is the Bayer designation for a star in the equatorial constellation of Aquarius. It is visible to the naked eye with an apparent magnitude of +4.279. Based upon parallax measurements made during the Hipparcos mission, the distance to this star is around.
The spectrum of this star fits a stellar classification of B8 V, showing that this is a B-type main sequence star. It has 2.7 times the radius of the Sun and is spinning rapidly with a projected rotational velocity of 135 km/s. A 2010 infrared search for companions around this star was unsuccessful.
