Astron Astrophys Rev (2009) 17:181–249 DOI 10.1007/s00159-009-0019-z REVIEW ARTICLE What makes a planet habitable? H. Lammer · J. H. Bredehöft · A. Coustenis · M. L. Khodachenko · L. Kaltenegger · O. Grasset · D. Prieur · F. Raulin · P. Ehrenfreund · M. Yamauchi · J.-E. Wahlund · J.-M. Grießmeier · G. Stangl · C. S. Cockell · Yu.N.Kulikov · J. L. Grenfell · H. Rauer Received: 25 August 2008 / Revised: 2 February 2009 / Published online: 10 April 2009 © Springer-Verlag 2009 Abstract This work reviews factors which are important for the evolution of habitable Earth-like planets such as the effects of the host star dependent radiation and particle fluxes on the evolution of atmospheres and initial water inventories. We discuss the geodynamical and geophysical environments which are necessary for plan- ets where plate tectonics remain active over geological time scales and for planets H. Lammer (B) · M. L. Khodachenko · G. Stangl Space Research Institute, Austrian Academy of Sciences, Graz, Austria e-mail:
[email protected] M. L. Khodachenko e-mail:
[email protected] G. Stangl e-mail:
[email protected] J. H. Bredehöft Institut für Angewandte und Physikalische Chemie, Universität Bremen, Bremen, Germany e-mail:
[email protected] A. Coustenis Laboratoire d’Etudes Spatiales et d’Instrumentation en Astrophysique (LESIA), Observatoire de Meudon, Meudon, France e-mail:
[email protected] L. Kaltenegger Harvard-Smithonian Center for Astrophysics, Cambridge, MA, USA e-mail:
[email protected] O. Grasset UMR, Laboratoire de Planétologie et Géodynamique, Nantes, France e-mail:
[email protected] 123 182 H.