Warm, water-depleted rocky exoplanets with surface ionic liquids: A proposed class for planetary habitability

Supplementary Data for the paper entitled: "Warm, water-depleted rocky exoplanets with surface ionic liquids: A proposed class for planetary habitability" Rachana Agrawal1, Sara Seager1,2,3,4*, Iaroslav Iakubivskyi1,5, Weston P. Buchanan1, Ana Glidden1,4, Maxwell D. Seager6, William Bains7, Jingcheng Huang1, Janusz J. Petkowski8,9,* 1 Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, USA 2 Department of Physics, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, USA 3 Department of Aeronautical and Astronautical Engineering, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, USA 4 Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, USA 5 Tartu Observatory, University of Tartu, 1 Observatooriumi, 61602 Tõravere, Estonia 6 Department of Chemistry and Biochemistry, Worcester Polytechnic Institute, Worcester, MA 01609, USA 7 School of Physics and Astronomy, Cardiff University, 4 The Parade, Cardiff CF24 3AA, UK 8 Faculty of Environmental Engineering, Wroclaw University of Science and Technology, 50-370 Wroclaw, Poland 9 JJ Scientific, Warsaw, Mazowieckie, Poland *Corresponding author: Sara Seager, Janusz J. Petkowski Email: [e-mail], [e-mail]