AX Microscopii
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Lacaille 8760 (AX Microscopii) is a red dwarf star in the constellation
Microscopium Microscopium ("the Microscope") is a minor constellation in the southern celestial hemisphere, one of twelve created in the 18th century by French astronomer Nicolas-Louis de Lacaille and one of several depicting scientific instruments. The n ...
. It is one of the nearest stars to the Sun at about 12.9 light-years' distance, and the brightest M dwarf star in Earth's night sky, although it is generally too faint to be seen without a
telescope A telescope is a device used to observe distant objects by their emission, absorption, or reflection of electromagnetic radiation. Originally meaning only an optical instrument using lenses, curved mirrors, or a combination of both to observ ...
. At an
apparent magnitude Apparent magnitude () is a measure of the brightness of a star or other astronomical object observed from Earth. An object's apparent magnitude depends on its intrinsic luminosity, its distance from Earth, and any extinction of the object's ...
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 Abbé Nicolas-Louis de Lacaille (; 15 March 171321 March 1762), formerly sometimes spelled de la Caille, was a French astronomer and geodesist who named 14 out of the 88 constellations. From 1750 to 1754, he studied the sky at the Cape of Goo ...
. 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 1847 edition of Lacaille's catalogue of 9766 stars by
Francis Baily Francis Baily (28 April 177430 August 1844) was an English astronomer. He is most famous for his observations of "Baily's beads" during a total eclipse of the Sun. Baily was also a major figure in the early history of the Royal Astronomical S ...
.
Francis Baily Francis Baily (28 April 177430 August 1844) was an English astronomer. He is most famous for his observations of "Baily's beads" during a total eclipse of the Sun. Baily was also a major figure in the early history of the Royal Astronomical S ...
. ''A Catalogue of 9766 Stars'' (1847)
Page 219
/ref> In the past Lacaille 8760 has been classified anywhere from spectral class K7 down to M2. In 1979 the
Irish Irish may refer to: Common meanings * Someone or something of, from, or related to: ** Ireland, an island situated off the north-western coast of continental Europe ***Éire, Irish language name for the isle ** Northern Ireland, a constituent unit ...
astronomer Patrick Byrne discovered that it is a
flare star A flare star is a variable star that can undergo unpredictable dramatic increases in brightness for a few minutes. It is believed that the flares on flare stars are analogous to solar flares in that they are due to the magnetic energy stored in th ...
, and it was given the
variable star designation In astronomy, a variable star designation is a unique identifier given to variable stars. It uses a variation on the Bayer designation format, with an identifying label (as described below) preceding the Latin genitive of the name of the conste ...
AX Microscopii, or AX Mic. As a flare star it is relatively quiescent, only erupting on average less than once per day. 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 Stellar rotation is the angular motion of a star about its axis. The rate of rotation can be measured from the spectrum of the star, or by timing the movements of active features on the surface. The rotation of a star produces an equatorial bulg ...
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 Flattening is a measure of the compression of a circle or sphere along a diameter to form an ellipse or an ellipsoid of revolution (spheroid) respectively. Other terms used are ellipticity, or oblateness. The usual notation for flattening is ...
of 0.23. Its closest approach to the Sun occurred about 20,000 years ago when it came within . Due to its low mass (60% of the Sun), it has an expected lifespan of about 75 billion (, seven times longer than the Sun's.


References


External links


SolStation article
{{DEFAULTSORT:Lacaille 8760 M-type main-sequence stars BY Draconis variables Flare stars Local Bubble Microscopium CD-39 14192 0825 202560 105090 Microscopii, AX