R Leonis is a red giant Mira-type variable star located approximately 370 light years away in the constellation Leo.
The apparent magnitude of R Leonis varies between 4.31 and 11.65 with a period of 312 days. At maximum it can be seen with the naked eye, while at minimum a telescope of at least 7 cm is needed. The star's effective temperature is estimated to be 2,930 – 3,080 kelvins and radius spans 320 solar radii (220,000,000 kilometres; 1.5 astronomical units), roughly Mars's orbital zone.
Possible planet
In 2009 Wiesemeyer et al. proposed that quasi-periodic fluctuations observed for the star R Leonis may be due to the presence of an evaporating substellar companion, probably an extrasolar planet. They have inferred a putative mass for the orbiting body of twice the mass of Jupiter, orbital period of 5.2 years and likely orbital separation of 2.7 astronomical units. If confirmed such a planetary object could likely be an evaporating planet, with a long comet-like trail as hinted by intense SiO maser emissions.
References
External links AAVSO Variable Star of the Month. April, 2001: R Leonis Archived 2003-11-06 at the Wayback Machine


![R Leonis: The light curve of R Leonis from AAVSO V band data[7]](https://upload.wikimedia.org/wikipedia/commons/thumb/5/59/RLeoLightCurve.png/1280px-RLeoLightCurve.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)

