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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Iota Aurigae is an orange K-type bright giant with an apparent magnitude of +2.69. It is approximately 512 light-years from Earth, and is dimmed by approximately 0.6 points of magnitude by interstellar dust. During the Extreme Solar Systems conference held on June 25 29, 2007, in Santorini, Greece, Reffert et al. announced the detection of two substellar objects orbiting Iota Aurigae in 2:1 resonance. Such companions would be brown dwarfs with orbital periods of approximately 2 and 4 years.…mehr

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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Iota Aurigae is an orange K-type bright giant with an apparent magnitude of +2.69. It is approximately 512 light-years from Earth, and is dimmed by approximately 0.6 points of magnitude by interstellar dust. During the Extreme Solar Systems conference held on June 25 29, 2007, in Santorini, Greece, Reffert et al. announced the detection of two substellar objects orbiting Iota Aurigae in 2:1 resonance. Such companions would be brown dwarfs with orbital periods of approximately 2 and 4 years.