as a matrix-supported carbonate-dominated rock composed of more than 90% carbonate mud (<63 μm) component. The identification of carbonate mudstone A recent study by Lokier and Al Junaibi (2016) has highlighted that the most common problems encountered when describing a mudstone is to incorrectly estimate the volume of 'grains' in the sample - in consequence, misidentifying mudstone as wackestone and vice versa. The original Dunham classification (1962) defined the matrix as clay and fine-silt size sediment <20 μm in diameter. This definition was redefined by Embry & Klovan (1971) to a grain size of less than or equal to 30 μm. Wright (1992) proposed a further increase to the upper limit for the matrix size in order to bring it into line with the upper limit for silt (63 μm). Mudstone mineralogy on Mars On December 13, 2016, NASA reported further evidence supporting habitability on the planet Mars as the Curiosity rover climbed higher, studying younger layers, on Mount Sharp. Also reported, the very soluble element boron was detected for the first time on Mars. In June 2018, NASA reported that Curiosity had detected kerogen and other complex organic compounds from mudstone rocks approximately 3.5 billion years old. See also Mudstone on planet Mars Aeolis quadrangle Composition of Mars Timeline of Mars Science Laboratory References es:Lutita