“…For future planetary missions especially for Mars surface exploration, Raman spectroscopy has a great advantage due to its power in fast molecular (organic and inorganic) phase identification in mixtures, characterization of mineral chemistry, and the minimum‐to‐no sample preparation requirement [e.g., Rull et al ., ; Sharma et al ., ; Wang et al ., , ]. The applications of Raman spectroscopy in planetary sciences and its potential in planetary explorations have been developed since 1995, for igneous mineralogy and petrology that target the Moon, Mars, and Venus [ Freeman et al ., ; Haskin et al ., ; Kuebler et al ., ; Ling et al ., ; Wang et al ., , , , , , , ; Wang , ]; and for secondary mineralogy and alteration processes that target Mars, asteroids, and other primary planetary bodies [ Chio et al ., , ; Chou et al ., ; Gough et al ., , ; Nuding et al ., ; McSween and Treiman , ; Kong et al ., , ; Kong and Wang , ; Ling and Wang , ; Wang et al ., ; Wang and Valentine , ; Wang et al ., , , , ; Y. W. Wang et al ., ; Wang et al ., ; Wang and Ling , ; Wang and Zhou , ; Wei et al ., ; Liu and Wang , ; Wang et al ., submitted to Journal of Raman Spectroscopy ]. Recently, three Raman units have been selected as scientific payloads for 2018 ExoMars and 2020 Mars rover, with the mission goals of fine‐scale definitive mineralogy and biosignature detection.…”