Prebiotic chemistry and protocells during the faint young sun event

The sun generates light and heat for life on Earth to flourish. However, during the late Hadean-early Archean epoch on Earth, the "faint young sun" (FYS) was less luminous, influencing prebiotic chemistry and, by extension, the origins of life (OoL). However, higher levels of ultraviolet (UV) radiation from the FYS, especially UV-C, due to the lack of an ozone layer, would likely have impacted the assembly, stability, persistence, and functions of prebiotic cellular precursors, i.e., protocells. Consequently, it is essential to study how such UV-C radiation would have affected the synthesis and stability of prebiotically relevant molecules and protocells to better understand the plausibility of the OoL during the FYS period. In this letter, we introduce unanswered questions surrounding the structure and stability of protocells under UV-C radiation. Such a perspective may be vital to exoplanetary systems orbiting other stars, enhancing our understanding of life's potential beyond our solar system.