Iota Tucanae
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Iota Tucanae (ι Tuc, ι Tucanae) is a solitary[10] star in the southern constellation of Tucana. Based upon an annual parallax shift of 10.72 mas as seen from Earth,[2] it is located around 304 light years from the Sun. With an apparent visual magnitude of +5.33,[3] it is faintly visible to the naked eye.
This is a yellow-hued G-type giant star with a stellar classification of G5 III.[4] The variability of the brightness of Iota Tucanae was discovered when the Hipparcos data was analyzed.[11] It is classified as a semiregular variable star, showing a periodicity of 66.8 days with an amplitude of 0.0202 in visual magnitude.[12] Iota Tucanae is an X-ray source with a luminosity of Script error: No such module "val"..[13] It has an estimated 2.2[5] times the mass of the Sun, and, at the age of 1.69 billion years,[5] it has evolved away from the main sequence, expanding to 11[7] times the Sun's radius. The star radiates 65[5] times the solar luminosity from its photosphere at an effective temperature of 5,039 K.[5]
References
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