Buried Volcano-Hydrothermal Systems and Minerals on Mars

The pressure and temperature conditions on planet Mars have probably never permitted the presence of liquid water at its surface, as witnessed by unaltered olivines of any age since the Naochian. Nevertheless, iron sulphates at the surface suggest hydrothermal activity at some point in time and spac...

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Bibliographic Details
Main Authors: Rouwet, Dmitri, Inguaggiato, Claudio, Leone, Giovanni
Other Authors: Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Bologna, Bologna, Italia, Universidad de Atacama, Instituo de Astronomía y Ciencias Planetarias, Copiapó, Chile
Format: Book Part
Language:English
Published: Springer Heidelberg 2021
Subjects:
Online Access:http://hdl.handle.net/2122/15044
https://link.springer.com/chapter/10.1007%2F978-3-030-84103-4_7
https://doi.org/10.1007/978-3-030-84103-4_7