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[null,"1.","Record Nr.",null,"UNINA990004030020403321"]
[null,null,"Autore",null,"Dupuy, Micheline"]
[null,null,"Titolo",null,"Pour Dieu et pour le roi : la montée de l'intolerance au XVI siècle / de Marignan Wassy 1515-1562"]
[null,null,"Pubbl/distr/stampa",null,"Paris : Libr. Académique Perrin, 1984"]
[null,null,"Descrizione fisica",null,"378 p. ; 20 cm"]
[null,null,"Collana",null,"Présence de l'histoire"]
[null,null,"Disciplina",null,"944.029"]
[null,null,"Locazione",null,"FLFBC"]
[null,null,"Collocazione",null,"944.029 DUP 1"]
[null,null,"Lingua di pubblicazione",null,"Francese"]
[null,null,"Formato",null,"Materiale a stampa"]
[null,null,null,"Livello bibliografico","Monografia"]
[null,"2.","Record Nr.",null,"UNINA9910554262303321"]
[null,null,"Autore",null,"Encrenaz Therese"]
[null,null,"Titolo",null,"Planets and life / / Therese Encrenaz, James Lequeux and Fabienne Casoli"]
[null,null,"Pubbl/distr/stampa",null,"[Place of publication not identified] : , : EDP Sciences, , [2021]"]
[{"$nulls":4},"©2021"]
[null,null,"Edizione",null,"[1st ed.]"]
[null,null,"Descrizione fisica",null,"1 online resource (164 pages)"]
[null,null,"Collana",null,"Current Natural Sciences"]
[null,null,"Disciplina",null,"523.01"]
[null,null,"Soggetti",null,"Astrophysics"]
[null,null,"Lingua di pubblicazione",null,"Inglese"]
[null,null,"Formato",null,"Materiale a stampa"]
[null,null,null,"Livello bibliografico","Monografia"]
[null,null,"Nota di contenuto",null,"Frontmatter -- Foreword -- Contents -- Chapter 1. Introduction -- Chapter 2. The Formation of Terrestrial Planets -- Chapter 3. The Exploration of Terrestrial Planets -- Chapter 4. Venus, Earth and Mars: A Diverging Evolution -- Chapter 5. The Appearance of Life -- Chapter 6. The Development of Life on Earth -- Chapter 7. Life in the Solar System? -- Chapter 8. How to Search for Life on Rocky Exoplanets? -- Chapter 9. Conclusions: Some Future Directions in Exobiology -- Glossary -- Bibliography"]
[null,null,null,"Sommario/riassunto","The Earth is the only planet in the Solar System where liquid water is present on the surface, a condition that seems necessary for the development of life. Its sisters Venus and Mars are extremely different. Why did these three planets, born under fairly comparable conditions, evolve to the conditions we observe today? Understanding the physical or chemical factors that are at the origin of such divergent evolutions is a first step in an approach to the problem of the origin of life on Earth."]