Gamma Virginis is a star in the constellation Virgo. It has the traditional names Porrima, Postvarta and Arich. Gamma Virginis is a binary star, consisting of two stars of approximately equal apparent magnitudes 3.48 and 3.50, and of spectral type F0V. With an orbital period of 168.93 years it was an easy object for amateur astronomers until the beginning of the 1990s, but now the smaller apparent distance between the stars requires a larger telescope. Read more
The double stars of Gamma Virginis are now separated by ~1.7 arc seconds
Don’t miss the spectacular binary star event of the century: the now-imminent periastron passage of Gamma Virginis . Gamma Virginis was named Porrima by the Romans, after two different goddesses of prophecy in antiquity.
Gamma Virginis is a splendid binary for medium sized telescopes, with an orbit of 168.7 years; positioned about fourteen degrees northwest of the bright star Spica.
For over 160 of its 169-year period this pair of identical 3rd magnitude stars have been easily resolved at moderate power in a small telescope but, thanks to its extreme orbital eccentricity (about 0.9), Gamma closes for 2 or 3 months around minimum to no more than 1/3 arc second, (a dramatic climax last seen in the winter of 1835-6 by John Herschel, W.R.Dawes and Admiral Smyth.)
The visual appearance of the pair is obvious at the eyepiece over an astonishingly short time -- we are about to witness the only instance in the entire sky visible from northern latitudes of a bright pair visibly and obviously moving, as seen in a 6-inch telescope (minimum), within a 2-year period.