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We suggest to use the Hubble Space Telescople (HST) follow-up observations ofthe TESS targets for detecting possible plasma tori along the orbits ofexoplanets orbiting M dwarfs. The source of the torus could be planetaryvolcanic activity due to tidal or electromagnetic induction heating. Fastlosses to space for planets orbiting these active stars can lead to the lostmaterial forming a torus along the planetary orbit, similar to the Io plasmatorus. We show that such torus would be potentially detectable by the HST inthe UV.

Detecting volcanically produced tori along orbits of exoplanets using UV spectroscopy