The RS Canum Venaticorum variable cardRS Canum Venaticorum variable

RS Canum Venaticorum variable

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What Wikipedia says

An RS Canum Venaticorum variable is a type of variable star. The variable type consists of close binary stars having active chromospheres which can cause large stellar spots. These spots are believed to cause variations in their observed luminosity.

Excerpt from the Wikipedia article “RS Canum Venaticorum variable”, under the CC BY-SA 4.0 license. Read the article on Wikipedia

Image: PopePompus, CC BY-SA 4.0, via Wikimedia Commons.

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