Beta Tau is the traditional Bayer designation for a star in the constellation Taurus, the Bull.
Beta Tau is an A-type supergiant star, a star that has exhausted its hydrogen supply and has expanded to a radius tens or hundreds of times that of the Sun. It has an apparent magnitude of +1.68, making it the second-brightest star in Taurus after Aldebaran.
Beta Tau is located at a distance of approximately 140 light-years from Earth. It has a mass of about 6 times that of the Sun and a radius of about 35 times that of the Sun. The star is rotating rapidly, with a projected rotational velocity of about 200 kilometers per second.
The spectrum of Beta Tau shows strong lines of ionized calcium and hydrogen, indicating that it is a relatively hot star with a surface temperature of about 8,500 Kelvin. The star is also emitting X-rays, which are produced by a hot corona surrounding the star.
Beta Tau is in the post-main sequence phase of its evolution. It has exhausted its hydrogen supply and has begun to fuse helium in its core. The star is expected to eventually evolve into a red giant and then a white dwarf.
Beta Tau is a variable star of the Alpha2 Canum Venaticorum type. The star's brightness varies slightly over a period of about 2.8 days. The variations in brightness are thought to be caused by pulsations in the star's outer layers.
Beta Tau has been known to astronomers for centuries. It was mentioned in the Almagest, a treatise on astronomy written by the Greek astronomer Claudius Ptolemy in the 2nd century AD. The star was also mentioned in the Chinese astronomical catalog Shi Shi, which was compiled in the 6th century AD.
In the 19th century, the German astronomer Friedrich Wilhelm Argelander designated Beta Tau as a member of his Uranometria Nova star catalog. The star was also included in the Henry Draper Catalogue, a catalog of stellar spectra published in the early 20th century.
Property | Value |
---|---|
Bayer designation | Beta Tau |
Constellation | Taurus |
Spectral type | A7 III |
Apparent magnitude | +1.68 |
Distance | 140 ly |
Mass | 6 M☉ |
Radius | 35 R☉ |
Projected rotational velocity | 200 km/s |
Surface temperature | 8,500 K |
Property | Value |
---|---|
Variable star type | Alpha2 Canum Venaticorum |
Period | 2.8 days |
Amplitude | 0.03 magnitudes |
Year | Event |
---|---|
2nd century AD | Beta Tau mentioned in Ptolemy's Almagest |
6th century AD | Beta Tau mentioned in the Chinese astronomical catalog Shi Shi |
19th century | Beta Tau designated as a member of Argelander's Uranometria Nova star catalog |
Early 20th century | Beta Tau included in the Henry Draper Catalogue |
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