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An artist’s impression of the hot-Jupiter exoplanet tau Boötis b. Image credit: L. Calçada / ESO. Tau Boötis is a binary stellar system approximately 51 light-years away in the constellation of Boötes. It consists of a hot and young F-type star, tau Boötis A, and a smaller M3-type (red dwarf) star, tau Boötis B. In 1996, a hot-Jupiter exoplanet was discovered orbiting the primary star tau Boötis A. Named tau Boötis b, the alien world has a mass almost 6 times that of Jupiter and an orbital period of 3 days and 7.5 hours. “We present one of the first hints of detecting an exoplanet in the radio realm,” said Dr. Jake Turner, an astronomer in the Department of Astronomy and Carl Sagan Institute at Cornell University and the Department of Astronomy at the University of Virginia.

Jake turnerRay jayawardhanaDepartment of astronomyUniversity of virginiaCarl sagan institute at cornell universityFrequency arrayCarl sagan instituteCornell universityProfessor ray jayawardhanaProfessor jayawardhanaஜேக் டர்னர்துறை ஆஃப் வானியல்பல்கலைக்கழகம் ஆஃப் வர்ஜீனியாகார்ல் சாகன் நிறுவனம் இல் கார்னெல் பல்கலைக்கழகம்அதிர்வெண் வரிசைகார்ல் சாகன் நிறுவனம்