Tau Ceti (τ Cet) est stella Sole nostro haud dissimilis, sla 11,89 nec plura distans, et inter stellas splendidissimas constellationis Eridani decima. Enumeratione systematum stellarium proximorum locum vigesimum tertium tenet. Magnitudinem apparentem 3,49 monstrat. Stella habet discum protoplanetarium planetasque plures, quorum quattuor intra zonam habitabilem circuire censentur.
Bibliographia
- Fabo Feng, Mikko Tuomi, Hugh R.A. Jones, John Barnes, Guillem Anglada-Escude, Steven S. Vogt, R. Paul Butler, "Color difference makes a difference: four planet candidates around tau Ceti" (2017) apud ArXiv.org pro Astrophysical Journal
- Mikko Tuomi et al., "Signals embedded in the radial velocity noise. Periodic variations in the tau Ceti velocities" (2012) apud ArXiv.org pro Astronomy and Astrophysics. Alia recensio
Nexus externi
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Vicimedia Communia plura habent quae ad Tau Ceti spectant. |
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Data astronomica: "* tau Cet" apud SIMBAD. "00151" apud ARICNS. |
- "Tau Ceti" apud Sol Station
- "Tau Ceti" apud Open Exoplanets Catalogue
- Tim Stephens, "Four Earth-sized planets detected orbiting the nearest sun-like star" (9 Augusti 2017) apud Phys.org
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