GG Lupi is an eclipsing binary star in the southern constellation of Lupus. Most of the time it is a magnitude 5.6 object, making it faintly visible to the naked eye, but during the primary eclipse its brightness falls to 6.1. GG Lupi is located one half-degree (one full moon diameter) west of the third-magnitude star Delta Lupi.
This star was found to be a spectroscopic binary in 1930, and its eclipses were detected in observations during 1964. Its location in the sky, distance (~490 light-years) and proper motion make it a likely member of the Scorpius–Centaurus association within the Gould's Belt star-formation region. The two stars comprising this binary are both very young main-sequence stars of spectral type B. They are estimated to be about 20 million years old, placing them near the zero-age main sequence. Their orbit is somewhat eccentric (e=0.15) and the period of apsidal precession is 102 years.
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![GG Lupi: A light curve for GG Lupi, plotted from TESS data[8]](https://upload.wikimedia.org/wikipedia/commons/thumb/e/e9/GGLupLightCurve.png/1280px-GGLupLightCurve.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)
