“…For the difficulty of data acquisition for Mars terrain images, many studies tested terrain classification methods with roves’ fully operational duplicates in Earth conditions and then applied those methods to the actual rover. The image features that are often used for terrain classification in those studies include color features based on the RGB space [ 8 , 9 , 10 , 11 , 12 ], HSV [ 6 , 7 , 13 , 14 , 15 ], and Lab [ 16 ] spaces; Gabor features [ 12 , 17 , 18 ]; the contrast [ 10 , 11 , 12 ], correlation [ 12 ], energy [ 11 , 12 , 13 ], and consistency [ 12 ] of gray-level co-occurrence matrix (GLCM); SURF features [ 19 , 20 ]; Daisy features [ 19 , 20 ]; local binary patterns (LBP) [ 19 , 20 , 21 ]; local ternary patterns (LTP) [ 19 , 20 , 21 ]; local adaptive ternary patterns (LATP) [ 19 , 20 ]; contrast context histogram (CCH) [ 20 ]; and the mean [ 2 , 9 , 13 , 14 , 15 , 22 ], entropy [ 8 , 9 , 22 ], contrast [ 8 , 23 ], correlation [ 23 ], energy [ 8 ,…”