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Beta Pictoris b.
Three exocomets discovered around the star Beta Pictoris.
Beta Pictoris.
Next articleThree exocomets discovered around the star Beta Pictoris.
Beta Pictoris.
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Previous articleThree exocomets discovered around the star Beta Pictoris.
The length of Beta Pictoris b's day is only 8 hours long.
Beta Pictoris b is more than 16 times larger and 3000 times more massive than the Earth, yet a day on the planet only lasts 8 hours.
This team alsohas observed an exoplanet around the star Beta Pictoris(eso1024), as well as several others.
Beta Pictoris b has been found to have a day that lasts only eight hours.
To supply the gas that we see around Beta Pictoris, one big comet must be completely destroyed every five minutes!
Beta Pictoris is one of the best-known examples of a star surrounded by a dusty debris disc.
This swirling halo of debris and gas was the first such configuration to be captured in image,making Beta Pictoris a celebrity star in the 1980s.
Beta Pictoris b is a young planet, only about 20 million years old- compared to 4.5 billion years for Earth.
A series of images captured between November 2013 toApril 2015 shows the exoplanet Beta Pictoris b as it moves through 1.5 years of its 22-year orbital period.
Beta Pictoris b is about 16 times larger and 3,000 times more massive than Earth, with eight-hour days.
A series of images captured between November 2013 toApril this year shows the exoplanet Beta Pictoris b as it moves through one and a half years of its 22-year orbital period.
Beta Pictoris b is about 16 times larger and 3,000 times more massive than Earth, with days lasting about eight hours.
Subsequently, irregularities have been found in the disk, which may be indicative of the presence of planetary bodies.[6]Similar discoveries of debris disks were made around the stars Fomalhaut and Beta Pictoris.
The main focus will be on Beta Pictoris b, which is about 16 times larger and 3,000 times more massive than Earth, but with days lasting only about eight hours.
Using the CRIRES instrument on the VLT, a team of Dutch astronomers from Leiden University and the Netherlands Institute for Space Research(SRON)has now found that the equatorial rotation velocity of exoplanet Beta Pictoris b is almost 62,000 mph(100,000 km/h).
The fast spin of Beta Pictoris b means that in the future it will be possible to make a global map of the planet, showing possible cloud patterns and large storms.
With the planned Mid-infrared E-ELT Imager and Spectrograph(METIS) we will be able to make global maps of exoplanets andcharacterise much smaller planets than Beta Pictoris b with this technique”, says METIS principal investigator and co-author of the new paper, Bernhard Brandl.
Beta Pictoris, a nearby star easily visible to the naked eye in the southern sky, is already hailed as the archetypal young planetary system.
First discovered in 2008, Beta Pictoris b is a gas giant planet 10 to 12 times the mass of Jupiter, with an orbit roughly the diameter of Saturn's.
Exoplanet Beta Pictoris b orbits the naked-eye star Beta Pictoris[1],[2], which lies about 63 light-years from Earth in the southern constellation of Pictor(The Painter's Easel).
Beta Pictoris b is still warm and young and over the next hundreds of millions of years, it will cool down and shrink to about the size of Jupiter, and if its angular momentum is preserved, then as it shrinks, the length of its day will decrease to about 3 hours and its equatorial rotation velocity will speed up to about 40 km/s.