Iron and titanium have been found in the atmosphere of the super-hot giant exoplanet, KELT-9b.
Learn how scientists use chemistry and technology to analyse elements throughout the universe in this resource for Year 8 and 10 students.
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KELT-9b, one of the most unlikely planets ever discovered, has surprised astronomers yet again with the discovery that its atmosphere contains the metals iron and titanium, according to research published in the journal Nature.
The planet is truly like no other. Located around 620 light-years away from Earth in the constellation Cygnus, it is known as a Hot Jupiter – which gives a hint to its nature.
Nearly three times the size of Jupiter, its surface temperature tops 3780 degrees Celsius – the hottest exoplanet ever discovered. It is even hotter than the surface of some stars.
Finding the chemical fingerprint of a planet
On the night of 31 July 2017, as KELT-9b passed across the face of its star, the HARPS-North spectrograph attached to the Telescopio Nazionale Galileo, on the Spanish Canary Island of La Palma, began watching.
The telescope recorded changes in colour in the planet’s atmosphere, the result of chemicals with different light-filtering properties.
By subtracting the plain starlight from the light that had passed through the atmosphere, the team were left with a spectrograph of its chemical make-up.
They then homed in on titanium and iron, because the relative abundances of uncharged and charged atoms tend to change dramatically at the temperatures seen on KELT-9b. After a complex process of analysis and cross-correlation of results, they saw dramatic peaks in the ionised forms of both metals.
It has been long suspected that iron and titanium exist on some exoplanets, but to date, they have been difficult to detect.
However, the permanent heatwave on KELT-9b means the metals are floating in the atmosphere as individual charged atoms, unable to condense or form compounds.
While this is the first time iron has been detected in an exoplanet’s atmosphere, titanium has previously been detected in the form of titanium dioxide on Kepler 13Ab, another Hot Jupiter. The discovery on KELT-9b, however, is the first detection of elemental titanium in an atmosphere.
KELT-9b’s atmosphere is also known to contain hydrogen, which was easily identifiable without requiring the type of complex analysis needed to identify iron and titanium.
However, another study found that the hydrogen is literally boiling off the planet, leading to the hypothesis that its escape could also be dragging the metals higher into the atmosphere, making their detection easier.
Further studies into KELT-9b’s atmosphere are continuing, with suggestions that announcements of other metals could be forthcoming. In addition, the complex analysis required in this study could be useful for identifying obscure components in the atmospheres of other planets.
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