11 Leonis Minoris
Leo Minor, Star system, Light-year, Stellar classification, Main sequence, RS Canum Venaticorum variable
Herausgegeben: Apostolis, Dismas Reinald
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 11 Leonis Minoris is a star system 37 light years away from Earth, in the constellation Leo Minor. The primary star is a yellow dwarf star of spectral type G8V, which is slightly more massive but slightly dimmer than our sun. The primary is an RS Canum Venaticorum type variable star and its brightness varies by 0.04 magnitudes. There is also a secondary star, a red dwarf star much dimmer than the primary. It orbits in a highly eccentric orbit ranging from roughly 4 AU...
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 11 Leonis Minoris is a star system 37 light years away from Earth, in the constellation Leo Minor. The primary star is a yellow dwarf star of spectral type G8V, which is slightly more massive but slightly dimmer than our sun. The primary is an RS Canum Venaticorum type variable star and its brightness varies by 0.04 magnitudes. There is also a secondary star, a red dwarf star much dimmer than the primary. It orbits in a highly eccentric orbit ranging from roughly 4 AU to 63 AU from the primary.
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