Rare-Earth metals in the atmosphere of a glowing-hot exoplanet

KELT-9 b is the hottest exoplanet known to date. In the summer of 2018, a joint team of astronomers from the universities of Bern and Geneva found signatures of gaseous iron and titanium in its atmosphere. Now these researchers have also been able to detect traces of vaporized sodium, magnesium, chromium, and the rare-Earth metals scandium and yttrium.

Artist’s impression of KELT-9b und its host star KELT-9
[Credit: © NASA/JPL-Caltech]

Exoplanets are planets outside our solar system that orbit around stars other than the Sun. Since the discovery of the first exoplanets in the mid-90’s, well over 3000 exoplanets have been discovered. Many of these planets are extreme compared to the planets in our solar system: Hot gas giants that orbit incredibly close to their host stars, sometimes within periods of less than a few days.
Such planets do not exist in our solar system, and their existence has defied predictions of how and why planets form. For the past 20 years, astronomers from all over the world have been working to understand where these planets come from, what they are made of, and what their climates are like.

An extremely hot gas giant

KELT-9 is a star located 650 light years from the Earth in the constellation Cygnus. Its exoplanet KELT-9 b exemplifies the most extreme of these so-called hot-Jupiters because it orbits very closely around its star that is almost twice as hot as the Sun.

Artist’s impression of a sunset over KELT-9b. Under this blazing star, the atmosphere of the planet
 is warm enough to glow in reddish-orange tones and to vaporise heavy metals such
as iron and titanium [Credit: © Denis Bajram]

Therefore, its atmosphere reaches temperatures of around 4000 °C. In such heat, all elements are almost completely vaporized and molecules are broken apart into their constituent atoms – much like is the case in the outer layers of stars. This means that the atmosphere contains no clouds or aerosols and the sky is clear, mostly transparent to light from its star.
The atoms that make up the gas of the atmosphere absorb light at very specific colors in the spectrum, and each atom has a unique «fingerprint» of colors that it absorbs. These fingerprints can be measured with a sensitive spectrograph mounted on a large telescope, allowing astronomers to discern the chemical composition of the atmospheres of planets that are many light-years away.

The exoplanet as a treasure trove

A team of researchers from the Universities of Bern and Geneva collaborated to use this technique, and made an interesting discovery: «Using the HARPS-North spectrograph on the Italian National Telescope on the island of La Palma, we found iron and titanium atoms in the hot atmosphere of KELT-9 b,» explains Kevin Heng, Director and Professor at the Center for Space and Habitabilty (CSH) at the University of Bern and a member of the National Centre of Competence in Research PlanetS.

A high-resolution image of the spectrum of our Sun [Credit: © N.A.Sharp,
NOAO/NSO/Kitt Peak FTS/AURA/NSF]

The team observed the KELT-9 system for a second time last summer, with the goal of confirming their previous detections, but also to proceed to search for additional elements that could be present in the data as well. Their survey included 73 atoms, among which some so-called rare-Earth metals. These substances are less common on Earth, but are applied in advanced materials and devices.
Jens Hoeijmakers, who is the first author of the study which is now published in the journal Astronomy & Astrophysics and who is a Postdoc at the CSH in Bern and at Geneva Observatory, says: «Our team predicted that the spectrum of this planet could well be a treasure trove where a multitude of species can be detected that have not been observed in the atmosphere of any other planet before.»

After careful analysis, the researchers indeed found strong signals of vaporized sodium, magnesium, chromium and the rare-Earth metals scandium and yttrium in the spectrum of the planet. The latter three of these have never been detected robustly in the atmosphere of an exoplanet before.

«The team also advanced their interpretation of this data, and were able to use these signals to estimate at what altitude in the planet’s atmosphere these atoms are absorbing,» says Jens Hoeijmakers. What is more, the researchers also know more about strong global wind patterns high up in the atmosphere that blow the material from one hemisphere to the other.
«With further observations, many more elements may well be discovered by using the same technique in the atmosphere of this planet in the future, and perhaps also on other planets that are heated to similarly high temperatures,» explains Jens Hoeijmakers.

Kevin Heng adds: «The chances are good that one day we will find so-called biosignatures, i.e. signs of life, on an exoplanet, using the same techniques that we are applying today. Ultimately, we want to use our research to fathom the origin and development of the solar system as well as the origin of life.»

Source: University of Bern [May 10, 2019]

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