T Microscopii Explained

T Microscopii is a semiregular variable star in the constellation Microscopium. It ranges from magnitude 6.74 to 8.11 over a period of 352 days.[1] Located around 700 light-years distant, it shines with a bolometric luminosity 7,509 times that of the Sun and has a surface temperature of .[2]

Notes and References

  1. Web site: T Microscopii . Otero, Sebastian Alberto . 20 June 2011 . AAVSO Website. American Association of Variable Star Observers. 24 March 2015.
  2. Fundamental parameters and infrared excesses of Tycho–Gaia stars . 2017 . McDonald . I. . Zijlstra . A. A. . Watson . R. A. . Monthly Notices of the Royal Astronomical Society . 471 . 1 . 770–791 . 2017MNRAS.471..770M . 1706.02208 . 10.1093/mnras/stx1433 . free . 73594365 .

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