Matches in DBpedia 2015-04 for { ?s ?p "10 Canum Venaticorum is the Flamsteed designation for an ordinary star in the northern constellation of Canes Venatici. It has an apparent visual magnitude of 5.95, which, according to the Bortle scale, can be seen with the naked eye from suburban locations. Based upon an annual parallax shift of 0.05755 arc seconds as measured by the Hipparcos satellite, this system is 56.7 light-years (17.38 parsecs) from Earth.The stellar classification of 10 Canum Venaticorum is G0 V, indicating that it is a main sequence star that is fusing hydrogen into helium at its core to generate energy. It is older than the Sun, with an estimated age of six billion years. The effective temperature of the stellar atmosphere is 5,789 K, giving it the yellow hue of a G-type star.An excess of infrared emission at a wavelength of 70 μm suggests the presence of a debris disk. A temperature of 94 K indicates that this dusty disk is orbiting at a distance of about 12 AU from the host star."@en }
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- 10_Canum_Venaticorum abstract "10 Canum Venaticorum is the Flamsteed designation for an ordinary star in the northern constellation of Canes Venatici. It has an apparent visual magnitude of 5.95, which, according to the Bortle scale, can be seen with the naked eye from suburban locations. Based upon an annual parallax shift of 0.05755 arc seconds as measured by the Hipparcos satellite, this system is 56.7 light-years (17.38 parsecs) from Earth.The stellar classification of 10 Canum Venaticorum is G0 V, indicating that it is a main sequence star that is fusing hydrogen into helium at its core to generate energy. It is older than the Sun, with an estimated age of six billion years. The effective temperature of the stellar atmosphere is 5,789 K, giving it the yellow hue of a G-type star.An excess of infrared emission at a wavelength of 70 μm suggests the presence of a debris disk. A temperature of 94 K indicates that this dusty disk is orbiting at a distance of about 12 AU from the host star.".