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Discovered in 2016 by astronomers at the WASP-South survey, WASP-121b is 1.87 times bigger than Jupiter and 1.18 times more massive.
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Its host star, WASP-121 (TYC 7630-352-1), is an active F6-type main-sequence star about 1.5 times the size of the Sun.
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The WASP-121 system is located 881 light-years away in the constellation Puppis.
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WASP-121b is a so-called ‘hot Jupiter’ and takes just 1.3 days to orbit WASP-121. It is so close to the parent star that if it got any closer, the star’s gravity would start ripping it apart.
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Astronomers estimate the planet’s temperature to be about 4,600 degrees Fahrenheit (2,500 degrees Celsius), hot enough to boil some metals.
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Previous research found possible signs of a stratosphere on WASP-33b as well as some other hot Jupiters.
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The new study presents the best evidence yet because of the signature of hot water molecules that astronomers observed for the first time.
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This result is exciting because it shows that a common trait of most of the atmospheres in our solar system – a warm stratosphere – also can be found in exoplanet atmospheres.
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Theoretical models have suggested stratospheres may define a distinct class of ultra-hot planets, with important implications for their atmospheric physics and chemistry.
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These observations support this picture.
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To study the stratosphere of WASP-121b, the team observed a secondary eclipse of the planet using the Wide Field Camera onboard the NASA/ESA Hubble Space Telescope and the Infrared Array Camera onboard NASA’s Spitzer space telescope.
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The researchers analysed how different molecules in the stratosphere react to particular wavelengths of light.
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Water vapour in the planet’s atmosphere, for example, behaves in predictable ways in response to certain wavelengths of light, depending on the temperature of the water.
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Starlight is able to penetrate deep into a planet’s atmosphere, where it raises the temperature of the gas there.
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This gas then radiates its heat into space as infrared light.
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However, if there is cooler water vapour at the top of the atmosphere, the water molecules will prevent certain wavelengths of this light from escaping to space.
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But if the water molecules at the top of the atmosphere have a higher temperature, they will glow at the same wavelengths.
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The emission of light from water means the temperature is increasing with height.
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In Earth’s stratosphere, ozone gas traps ultraviolet radiation from the Sun, which raises the temperature of this layer of atmosphere.
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Other solar system bodies have stratospheres, too; methane is responsible for heating in the stratospheres of Jupiter and Saturn’s moon Titan, for example.
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In solar system planets, the change in temperature within a stratosphere is typically around 100 degrees Fahrenheit (about 56 degrees Celsius).
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On WASP-121b, the temperature in the stratosphere rises by 1,000 degrees Fahrenheit (560 degrees Celsius).
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The astronomers do not yet know what chemicals are causing the temperature increase in WASP-121b’s atmosphere.
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Vanadium oxide and titanium oxide are candidates, as they are commonly seen in brown dwarfs.
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Such compounds are expected to be present only on the hottest of hot Jupiters, as high temperatures are needed to keep them in a gaseous state.
Source:TH