The success of the ChemCam and SuperCam instruments onboard the MSL Curiosity and Perseverance rovers demonstrates the potential of laser-induced breakdown spectroscopy (LIBS) as an analytical tool (Wiens et al., 2013(Wiens et al., , 2020. In this technique, the laser creates a plasma with spectra consisting of emission lines from neutral, singly-, doubly-, and even triply-ionized species; these lines are then used to quantify chemistry.A key source of variability in LIBS data is plasma temperature (Tokar et al., 2015); higher proportions of multiply-ionized lines are observed at higher temperatures. Plasma temperatures are largely determined by the energy density of the ablation laser on the target surface. In laboratory-based LIBS instruments, ablation parameters such as the focal length and target distance are kept constant, and the energy density on target can be adjusted by changing the energy of the laser beam.The Mars missions cited above calibrated their instruments using spectra collected at a uniform distance and a single plasma temperature (Anderson et al., 2022;Clegg et al., 2017). It is now apparent that plasma temperatures vary widely in Mars spectra collected under a range of target distances due to changes in the ablation spot size (