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Tau Boötis b, or more precisely Tau Boötis Ab, is an extrasolar planet approximately 51 light-years away. The planet and its host star is one of the planetary systems selected by the International Astronomical Union as part of NameExoWorlds , their public process for giving proper names to exoplanets and their host star (where no proper name ...

2024年10月24日 · Tau Bootis b is a gas giant exoplanet that orbits a F-type star. Its mass is 5.95 Jupiters, it takes 3.3 days to complete one orbit of its star, and is 0.049 AU from its star. Its discovery was announced in 1996.

Tau Boötis, Latinised from τ Boötis, is an F-type main-sequence star approximately 51 light-years away [1] in the constellation of Boötes. It is a binary star system, with the secondary star being a red dwarf. In 1999, an extrasolar planet was detected orbiting the primary star.

2024年10月10日 · Recent ground-based high-resolution spectroscopic observations of the non-transiting hot Jupiter $\tau$ Boötis b from different instruments have resulted in a tension on the presence of water vapour in the planet's atmosphere, …

2014年2月26日 · The alien world, known as Tau Boötis b, Tau Boötis Ab or the Millennium Planet, was discovered in 1996. It is a so-called hot-Jupiter that orbits closely around its host star every 3 days 7.5 hours. Located in the constellation of Boötes, around 51 light-years away from our planet, Tau Boötis b has a mass almost six times that of Jupiter.

2024年3月25日 · Recently, circularly polarized bursty and slow emission from the τ Boötis (τ Boo) exoplanetary system was tentatively detected using LOFAR (LOW-Frequency ARray) beamformed observations. If confirmed, this detection will be a major contribution to exoplanet science. However, follow-up observations are required to confirm this detection. Aims.

2023年10月9日 · Recently, Turner et al. 2021 reported a tentative detection of circularly polarized bursty emission from the $\tau$ Boo exoplanetary system using LOFAR low-frequency beamformed observations. The likely source of this emission was presumed to be from the $\tau$ Boo planetary system and a possible explanation is radio emission from the exoplanet ...

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2024年10月10日 · Recent ground-based high-resolution spectroscopic observations of the non-transiting hot Jupiter τ \tau Bo\"otis b from different instruments have resulted in a tension on the presence of water...