S Cephei (S Cep), also designated as HD 206362, is a carbon star and Mira-type variable in the constellation Cepheus. Based on the measurement of its annual parallax by the Gaia satellite, the star is approximately ~1,590 ly (~490 pc) away from Earth.
S Cephei is a carbon star of spectral type C7.3e. It is also a Mira-type variable star whose apparent magnitude varies from 6.6 to 12.5 in the form of a pulsation over a period of 484 days. Its variability was discovered by Karl Hencke in 1858.
See also Mu Cephei ST Cephei
References


![S Cephei: A visual band light curve for S Cephei, plotted from ASAS-SN data[8]](https://upload.wikimedia.org/wikipedia/commons/thumb/1/1d/SCepLightCurve.png/1280px-SCepLightCurve.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)
