The martian eolian dust chemical composition is homogeneous at the sub- mm scale. It is different from the Aeolis Palus soils and Bagnold sands with a larger content of FeO, TiO2 and lower hydration.
|Number of pages||2|
|Publication status||Published - Jul 2019|
|Event||Ninth International Conference on Mars, held 22-25 July, 2019 in Pasadena, California - California Institute of Technology , Pasadena , United States|
Duration: 22 Jul 2019 → 25 Jul 2019
Conference number: 31488-19
|Conference||Ninth International Conference on Mars, held 22-25 July, 2019 in Pasadena, California|
|Period||22/07/19 → 25/07/19|