Matches in DBpedia 2016-04 for { ?s ?p "40 Eridani is a triple star system less than 16.5 light years away from Earth, in the constellation Eridanus. It is also known as Omicron2 Eridani for all collective components. Component A is also known as Keid, from the Arabic word qayd, (egg) shells.The primary star of the system, 40 Eridani A, is easily visible to the naked eye. The pair 40 Eridani B/C was discovered on January 31, 1783, by William Herschel., p. 73 It was again observed by Friedrich Georg Wilhelm Struve in 1825 and by Otto Wilhelm von Struve in 1851. In 1910, it was discovered that although component B was a faint star, it was white in color. This meant that it had to be a small star; in fact it was a white dwarf, the first discovered."@en }
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- 40_Eridani abstract "40 Eridani is a triple star system less than 16.5 light years away from Earth, in the constellation Eridanus. It is also known as Omicron2 Eridani for all collective components. Component A is also known as Keid, from the Arabic word qayd, (egg) shells.The primary star of the system, 40 Eridani A, is easily visible to the naked eye. The pair 40 Eridani B/C was discovered on January 31, 1783, by William Herschel., p. 73 It was again observed by Friedrich Georg Wilhelm Struve in 1825 and by Otto Wilhelm von Struve in 1851. In 1910, it was discovered that although component B was a faint star, it was white in color. This meant that it had to be a small star; in fact it was a white dwarf, the first discovered.".
- Q1052822 abstract "40 Eridani is a triple star system less than 16.5 light years away from Earth, in the constellation Eridanus. It is also known as Omicron2 Eridani for all collective components. Component A is also known as Keid, from the Arabic word qayd, (egg) shells.The primary star of the system, 40 Eridani A, is easily visible to the naked eye. The pair 40 Eridani B/C was discovered on January 31, 1783, by William Herschel., p. 73 It was again observed by Friedrich Georg Wilhelm Struve in 1825 and by Otto Wilhelm von Struve in 1851. In 1910, it was discovered that although component B was a faint star, it was white in color. This meant that it had to be a small star; in fact it was a white dwarf, the first discovered.".