Star EE Leonis
Red dwarf EE Leonis is located 23 light years away from the Sun.
It is a single star of spectral class M4V, that has 26 % of solar mass.
For now, there are no known exoplanets in this star system.
More about EE Leonis
Nearby star EE Leonis is a main sequence star that fuses hydrogen atoms into helium. It is approximately 30 % of the size of Sun and temperature on its surface is around 3345 K (3072 °C), which is about 58 % of Sun's temperature.
a BY Draconis variable. Stars from this category exhibit periodic variations in their luminosity. The variability is caused by a rotation which shows and hides starspots on the surface. EE Leonis can be found in northern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope.
EE Leonis is a BY Draconis variable. Stars from this category exhibit periodic variations in their luminosity. The variability is caused by a rotation which shows and hides starspots on the surface.
Other designations of this star
EE Leo, Gliese 402, Wolf 358, HIP 53020, LTT 12891, LHS 294, Gaia EDR3 3864615459886222464
External sources
Simbad database (Wolf 358)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
Class of stars Red dwarf
Red dwarfs are small reddish stars, that are by far the most common type of star in solar neighborhood. Their mass is usually between 10 and 50 % of solar mass.
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Right ascension: 10h 50m 51.12s
Declination: 6° 48' 16.162'' (equatorial region)
Parallax: 143.539
Sun distance: 22.722 ly | 7 pc
Temperature: 3345 K | 0.58 T Sun
Luminosity: 0.00091 L Sun
Apparent magnitude (V): 11.7
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