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Shiv K. Sharma is a pioneering figure in planetary instrumentation and remote sensing, whose work has fundamentally advanced our ability to analyze extraterrestrial surfaces. His primary research areas encompass laser spectroscopy, planetary geology, and astrobiology detection, with a particular focus on developing compact, multi-functional instruments for space exploration. Sharma’s most significant contribution is his integral role in the SuperCam instrument suite aboard NASA’s Mars 2020 Perseverance rover—a landmark achievement that combines laser-induced breakdown spectroscopy (LIBS) and remote Raman spectroscopy to analyze Martian rocks and soils from a distance. This work, detailed in his highly cited 2020 paper (322 citations), represents a quantum leap in in-situ planetary analysis. Beyond Mars, Sharma has pioneered the development of integrated remote sensing systems that simultaneously employ Raman spectroscopy, laser-induced fluorescence (LIF), and lidar for detecting minerals and organic compounds—critical for astrobiology missions to targets like Jupiter’s moon Europa. His prototype instruments have demonstrated the ability to identify trace biosignatures at remarkably low concentrations, establishing new standards for planetary exploration. With a career spanning decades, Sharma’s work bridges fundamental spectroscopy and applied space instrumentation, making him a foundational figure in the search for life beyond Earth.