RS Coronae Borealis is a semiregular variable star located in the constellation Corona Borealis with a parallax of 2.93mas being a distance of 341 parsecs (1,110 ly). It varies between magnitudes 8.7 to 11.6 over 332 days. It is unusual in that it is a red star with a high proper motion (greater than 50 milliarcseconds a year). Located around 1072 light-years distant, it shines with a luminosity approximately 1839 times that of the Sun and has a surface temperature of 3340 K. In 1907 it was announced that Henrietta Swan Leavitt had discovered the star, then called BD+36°2672, is a variable star. It was given its variable star designation, RS Coronae Borealis, in 1910.
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![RS Coronae Borealis: A light curve for RS Coronae Borealis, plotted from Hipparcos data[6]](https://upload.wikimedia.org/wikipedia/commons/thumb/4/47/RSCrBLightCurve.png/1280px-RSCrBLightCurve.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)
