Formation of Magma Oceans on exoplanet

Induction heating can completely change the energy budget of an exoplanet and even melt its interior. In a study published by Nature Astronomy an international team led by the Space Research Institute of the Austrian Academy of Sciences with participation of the University of Vienna explains how magma oceans can form under the surface of exoplanets as a result of induction heating.

When a conductive material is embedded in a changing magnetic field, an electrical current is produced inside the body by a process called electromagnetic induction. If the electrical current is strong enough, it can heat the material in which it flows because of electrical resistance. This process called induction heating is widely used in industry to melt materials and at home to cook using induction stoves.

Fast rotation causes heating
An international team led by the Space Research Institute (IWF) of the Austrian Academy of Sciences (OeAW) with participation of the Department of Astrophysics of the University of Vienna was inspired by these examples. "We wanted to investigate if induction heating can play a role on a much bigger scale", explains first author Kristina Kislyakova. "We were particularly interested in planets orbiting stars that have strong magnetic fields". These stars can rotate very rapidly, which causes the magnetic field at the planet's orbit to change rapidly as well. In such cases, induction heating can take place inside the planet.

Impacts on planetary habitability
The team studied low mass stars that exhibit some exotic characteristics in comparison to our Sun. They are much smaller and dimmer. Some of them rotate very fast and possess magnetic fields hundreds of times stronger than the solar one. A good example of such a low-mass star is Trappist-1, which hosts a big family of seven close-in rocky planets, three of which may have liquid water on their surface. This planetary system is a top candidate for the search of Earth-like planets.

Kislyakova and her team have calculated the energy release inside the Trappist-1 planets due to induction heating. "We have shown that for some of the planets, the heating is strong enough to drive enormous volcanic activity or even lead to the formation of a magma ocean beneath the planetary surface."

As we know from Earth, strong volcanic activity can have a severe influence on a planet’s atmosphere. "Therefore, induction heating can strongly influence the habitability of an exoplanet", adds IWF co-author Luca Fossati. This new study shows that this effect has to be taken into account when studying the habitability and evolution of planets orbiting low-mass stars.

Publication in "Nature Astronomy":
K.G. Kislyakova, L. Noack, C.P. Johnstone, V.V. Zaitsev, L. Fossati, H. Lammer, M. L. Khodachenko, P. Odert, and M. Güdel. Magma oceans and enhanced volcanism on TRAPPIST-1 planets due to induction heating. Nature Astronomy, 2017
DOI: 10.1038/s41550-017-0284-0

Wissenschaftlicher Kontakt

Dr. Kristina Kislyakova

Institut für Astrophysik
Universität Wien
1180 - Wien, Türkenschanzstraße 17
+43 1 4277-53817
+43 660 162 1177
kristina.kislyakova@univie.ac.at

Rückfragehinweis

Mag. Alexandra Frey

Pressebüro der Universität Wien
Forschung und Lehre
Universität Wien
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+43-1-4277-175 33
+43-664-60277-175 33
alexandra.frey@univie.ac.at