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(Redirected from AX Microscopium)
Star in the constellation Microscopium
Lacaille 8760
Image of Lacaille 8760 (circled) in Bode's Uranographia (1801). In the corresponding catalog this star is listed as № 36 in constellation Microscopium.
Lacaille 8760Location of Lacaille 8760 in the constellation Microscopium
Lacaille 8760 (AX Microscopii) is a red dwarf star in the constellationMicroscopium. It is one of the nearest stars to the Sun at about 12.9 light-years' distance, and the brightest M-classmain-sequence star in Earth's night sky, although it is generally too faint to be seen without a telescope. At an apparent magnitude of +6.7, it may only be visible to the unaided eye under exceptionally good viewing conditions, under dark skies.
This star was originally listed in a 1763 catalog that was published posthumously by the French Abbé Nicolas-Louis de Lacaille. He observed it in the southern sky while working from an observatory at the Cape of Good Hope. Number 8760 was assigned to this star in the 1847 edition of Lacaille's catalogue of 9,766 stars by Francis Baily.
In the past, Lacaille 8760 has been classified anywhere from spectral class K7 down to M2. In 1979, the Irish astronomer Patrick Byrne discovered that it is a flare star, and it was given the variable star designation AX Microscopii, or AX Mic. As a flare star it is relatively quiescent.
Lacaille 8760 is one of the largest and brightest red dwarfs known, with about 60% the mass and 51% the radius of the Sun. It is about five billion years old and is spinning at a projected rotational velocity of 3.3 km/s, giving it a rotation period of roughly 40 days. The star is radiating 7.2% of the luminosity of the Sun from its photosphere at an effective temperature of 3,800 K.
Despite efforts by astronomers, as of 2011 no planets had been detected in orbit around this star.
Lacaille 8760 orbits around the galaxy with a relatively high ellipticity of 0.23. Its closest approach to the Sun occurred about 20,000 years ago when it came within 12 light-years (3.7 parsecs). Due to its low mass (60% of the Sun), it has an expected lifespan of about 75 billion (7.5 × 10) years, seven times longer than the Sun's.
^ Byrne, P. B.; Doyle, J. G. (January 1989), "Activity in late-type dwarfs. III - Chromospheric and transition region line fluxes for two dM stars", Astronomy and Astrophysics, 208 (1–2): 159–165, Bibcode:1989A&A...208..159B.
Allen, C.; Herrera, M. A. (April 1998), "The Galactic Orbits of Nearby UV Ceti Stars", Revista Mexicana de Astronomía y Astrofísica, 34: 37–46, Bibcode:1998RMxAA..34...37A.
Despain, K. H. (December 1981), "Low-mass evolution - Zero-age main sequence to asymptotic giant branch", Astrophysical Journal, Part 1, 251: 639–653, Bibcode:1981ApJ...251..639D, doi:10.1086/159510.
Image of Lacaille 8760 (circled) in Bode's Uranographia (1801). In the corresponding catalog this star is listed as № 36 in constellation Microscopium.
Lacaille 8760Location of Lacaille 8760 in the constellation Microscopium
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