“…To identify specific elements within the samples, the preprocessed LIBS spectra were compared to a spectral database that includes lines from the National Institute of Standards and Technology Atomic Database [ Kelleher et al ., ; Ralchenko et al ., ], lines from the recently published Mars emission line library [ Cousin et al ., ], and lines from our own spectral libraries [ Koujelev et al ., ; Lui and Koujelev , ; Sobron et al ., ]. Here, we constrained the database search to Al, C, Ca, Fe, K, Li, Mg, Na, S, and Si, as they are typical of most rocks and soils relevant to our investigation.…”