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tokens: This study was carried out with the support by the FWF NFN project S11601-N16 ‘Pathways to Habitability: From Disks to Active Stars, Planets and Life and the related subprojects S11607-N16 and S11608-N16. HL thanks the support by FWF project ‘Characterizing Stellar and Exoplanetary Environments via Modeling of Lyman-Alpha Transit Observations of Hot Jupiters, P 27256-N27. The authors thank Dr Yamila Miguel and Dr Alessandro Mura for their valuable comments on the mineral atmospheres. RS thanks the support by the FWF project P23810-N16. The authors thank the anonymous referee for valuable comments.