WASP-76 B Size Comparison
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WASP-76, also known as BD+01 316, is a yellow-white
main sequence In astronomy, the main sequence is a classification of stars which appear on plots of stellar color index, color versus absolute magnitude, brightness as a continuous and distinctive band. Stars on this band are known as main-sequence stars or d ...
star in the constellation of
Pisces Pisces may refer to: *Pisces (astrology), an astrological sign Astronomy *Pisces (constellation), a constellation ** Pisces Overdensity, an overdensity of stars in the Milky Way's halo that is situated in the Pisces constellation ** Pisces II, a ...
. A suspected stellar companion at a projected separation of 85
astronomical unit The astronomical unit (symbol: au or AU) is a unit of length defined to be exactly equal to . Historically, the astronomical unit was conceived as the average Earth-Sun distance (the average of Earth's aphelion and perihelion), before its m ...
s was reported in 2014. After about five billion years, WASP-76 has expanded and become more luminous than at the start of its
main sequence In astronomy, the main sequence is a classification of stars which appear on plots of stellar color index, color versus absolute magnitude, brightness as a continuous and distinctive band. Stars on this band are known as main-sequence stars or d ...
life, but most probably has not yet reached the
subgiant branch A subgiant is a star that is brighter than a normal main-sequence star of the same spectral class, but not as bright as giant stars. The term subgiant is applied both to a particular spectral luminosity class and to a stage in the evolution of ...
.


Planetary system

The "hot Jupiter" class planet
WASP-76b WASP-76b is an exoplanet classified as a Hot Jupiter. It is located in the constellation Pisces and orbits its host star, WASP-76, at a distance of approximately . Its orbital period is approximately 1.8 days, and its mass is about 0.92 times th ...
was discovered around WASP-76 in 2013. Analysis of
transit-timing variation Transit-timing variation is a method for detecting exoplanets by observing variations in the timing of a transit. This provides an extremely sensitive method capable of detecting additional planets in the system with masses potentially as small a ...
s suggest an additional planet in the system.


References


External links


WASP-76 in exoplanet.eu

WASP-76 на сайте Планетные системы
{{DEFAULTSORT:WASP-76 Planetary systems with one confirmed planet Pisces (constellation) F-type main-sequence stars Planetary transit variables Durchmusterung objects J01463185+0242019