Ross 47 is a variable star of spectral type M4 located in the constellation Orion. Based on parallax measurements, it lies 18.888 light-years (5.791 parsecs) from Earth.
Ross 47 is a small red dwarf with 23.8% of the Sun's size, and 6% of its luminosity. Its effective temperature is much cooler than the Sun's, about 3,330 K. It is a BY Draconis variable, a star which whose brightness varies across its rotation, having multiple starspots that contribute to the brightness variation. Its apparent magnitude varies from +11.48 to 11.55. Ross 47 was given the variable star designation V1352 Orionis in 1997.
References

![Ross 47: A visual band light curve for V1352 Orionis, adapted from Weis (1994)[11]](https://upload.wikimedia.org/wikipedia/commons/thumb/4/4f/V1352OriLightCurve.png/1280px-V1352OriLightCurve.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)
