Magma oceans and enhanced volcanism on TRAPPIST-1 planets due to induction heating
Abstract
Low-mass M stars are plentiful in the Universe and often host small, rocky planets detectable with the current instrumentation. Recently, seven small planets have been discovered orbiting the ultracool dwarf TRAPPIST-1\cite{Gillon16,Gillon17}. We examine the role of electromagnetic induction heating of these planets, caused by the star's rotation and the planet's orbital motion. If the stellar rotation and magnetic dipole axes are inclined with respect to each other, induction heating can melt the upper mantle and enormously increase volcanic activity, sometimes producing a magma ocean below the planetary surface. We show that induction heating leads the three innermost planets, one of which is in the habitable zone, to either evolve towards a molten mantle planet, or to experience increased outgassing and volcanic activity, while the four outermost planets remain mostly unaffected.
Keywords
Cite
@article{arxiv.1710.08761,
title = {Magma oceans and enhanced volcanism on TRAPPIST-1 planets due to induction heating},
author = {K. G. Kislyakova and L. Noack and C. P. Johnstone and V. V. Zaitsev and L. Fossati and H. Lammer and M. L. Khodachenko and P. Odert and M. Guedel},
journal= {arXiv preprint arXiv:1710.08761},
year = {2017}
}
Comments
Published in Nature Astronomy; https://www.nature.com/articles/s41550-017-0284-0