V385 Andromedae is a variable star in the constellation Andromeda, about 360 parsecs (1,200 ly) away. It is a red giant over a hundred times larger than the sun. It has an apparent magnitude around 6.4, just about visible to the naked eye in ideal conditions.
V385 Andromedae was identified as a long-period variable in 1999 from analysis of Hipparcos photometry. It was classified as a slow irregular variable, but analysis of its light curve identified a possible 36 day period. It varies by about 0.1 magnitudes.
References
External links MASCARA page


![V385 Andromedae: A light curve for V385 Andromedae, plotted from MASCARA data[2]](https://upload.wikimedia.org/wikipedia/commons/thumb/6/6a/V385AndLightCurve.png/1280px-V385AndLightCurve.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)
