This article is from the source 'guardian' and was first published or seen on . It last changed over 40 days ago and won't be checked again for changes.

You can find the current article at its original source at https://www.theguardian.com/science/2018/aug/15/hottest-of-ultra-hot-planets-is-so-hot-its-air-contains-vaporised-metal

The article has changed 4 times. There is an RSS feed of changes available.

Version 0 Version 1
Hottest of 'ultra-hot' planets is so hot its air contains vaporised metal Hottest of 'ultra-hot' planets is so hot its air contains vaporised metal
(about 3 hours later)
New observations of the hottest known planet have revealed temperatures similar to those typically seen at the surface of a star, as well as an atmosphere of vaporised iron and titanium.New observations of the hottest known planet have revealed temperatures similar to those typically seen at the surface of a star, as well as an atmosphere of vaporised iron and titanium.
The findings add to the diverse and, in some cases, extreme conditions seen on planets far beyond our own solar system.The findings add to the diverse and, in some cases, extreme conditions seen on planets far beyond our own solar system.
Kevin Heng, a professor at the University of Bern, who led the latest work, said: “The temperatures are so insane that even though it is a planet it has the atmosphere of a star.” Kevin Heng, a professor at the University of Bern, and co-author of the latest work, said: “The temperatures are so insane that even though it is a planet it has the atmosphere of a star.”
“The main lesson that exoplanets are teaching us is that we can’t just look in the solar system,” Heng added. “There are really weird things out there.”“The main lesson that exoplanets are teaching us is that we can’t just look in the solar system,” Heng added. “There are really weird things out there.”
The planet, called Kelt-9b, was discovered last year by an American team. It is in orbit about a star 650 light years from Earth in the constellation of Cygnus, the swan. The ultra hot planet is about 30 times closer to its host star than the Earth is to the sun – and its star is also twice as hot as the sun. As a result, temperatures on Kelt-9b reach 4,000C on the side that faces the star. This is not as hot as our Sun, which is almost 6,000C, but hotter than many stars.The planet, called Kelt-9b, was discovered last year by an American team. It is in orbit about a star 650 light years from Earth in the constellation of Cygnus, the swan. The ultra hot planet is about 30 times closer to its host star than the Earth is to the sun – and its star is also twice as hot as the sun. As a result, temperatures on Kelt-9b reach 4,000C on the side that faces the star. This is not as hot as our Sun, which is almost 6,000C, but hotter than many stars.
Due to its proximity to the star, the planet orbits the star every 36 hours, with the same side always facing inwards. This means there is constant daytime on one side and constant night on the other, creating extreme temperature variations across the planet. The temperature of the night side is probably still about 2,000C, though, Heng suggested.Due to its proximity to the star, the planet orbits the star every 36 hours, with the same side always facing inwards. This means there is constant daytime on one side and constant night on the other, creating extreme temperature variations across the planet. The temperature of the night side is probably still about 2,000C, though, Heng suggested.
Detailed measurements of the orbit suggest the planet is gaseous, probably mostly hydrogen and possibly with a small solid core. The latest observations, published in Nature, are the first to reveal the composition of the planet’s atmosphere.Detailed measurements of the orbit suggest the planet is gaseous, probably mostly hydrogen and possibly with a small solid core. The latest observations, published in Nature, are the first to reveal the composition of the planet’s atmosphere.
The team used the Galileo National Telescope in La Palma, Canary Islands, to observe the planet precisely as it was moving in front of its host star. By detecting the tiny fraction of light from the star that filters through the planet’s atmosphere, the astronomers were able to detect components in the atmosphere and show that these included iron vapour and titanium. This is the first time that metals have been spotted on planets beyond the solar system.The team used the Galileo National Telescope in La Palma, Canary Islands, to observe the planet precisely as it was moving in front of its host star. By detecting the tiny fraction of light from the star that filters through the planet’s atmosphere, the astronomers were able to detect components in the atmosphere and show that these included iron vapour and titanium. This is the first time that metals have been spotted on planets beyond the solar system.
In future, the same techniques could be used to detect hints of life elsewhere in the Universe.In future, the same techniques could be used to detect hints of life elsewhere in the Universe.
“It doesn’t matter if we’re trying to detect titanium, oxygen or some strange molecule that is indicative of life,” said Heng. “These hot planets are a testing ground for techniques that we will use when the really interesting planets start to show up over the next few years.”“It doesn’t matter if we’re trying to detect titanium, oxygen or some strange molecule that is indicative of life,” said Heng. “These hot planets are a testing ground for techniques that we will use when the really interesting planets start to show up over the next few years.”
ScienceScience
AstronomyAstronomy
newsnews
Share on FacebookShare on Facebook
Share on TwitterShare on Twitter
Share via EmailShare via Email
Share on LinkedInShare on LinkedIn
Share on PinterestShare on Pinterest
Share on Google+Share on Google+
Share on WhatsAppShare on WhatsApp
Share on MessengerShare on Messenger
Reuse this contentReuse this content