Rotating ellipsoidal variables are a class of close binary variable star systems whose components are ellipsoidal. They are not eclipsing, but fluctuations in apparent magnitude occur due to changes in the amount of light emitting area visible to the observer. Typical brightness fluctuations do not exceed 0.1 magnitudes. The brightest rotating ellipsoidal variable is Spica (α Virginis).
List of variables
References
External links OGLE Atlas of Variable Star Light Curves - Ellipsoidal variables

![Rotating ellipsoidal variable: A light curve for Spica, adapted from Tkachenko et al. (2016)[1]](https://upload.wikimedia.org/wikipedia/commons/thumb/0/09/AlphaVirLightCurve.png/1280px-AlphaVirLightCurve.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)
