Eruption characteristics of lunar localized pyroclastic deposits as evidenced by remotely sensed water, mineralogy, and regolith

Explosive volcanic eruptions are responsible for producing localized pyroclatic deposits found across the lunar surface. These small pyroclastic thought to have erupted through transient, vulcanian-like eruptions. We used several remote data products, including a water abundance map, understand compositional and physical properties of these deposits. Within deposits, we strong relationships between pyroxene abundance, glass regolith density scale height, longitude. suggest that can be estimate gas content an eruption, cooling rate pyroclasts, optical eruption plume, degree fragmentation infer on distribution in interior. Further, deduce excess within represents interior content, which tied other measurements represent important petrological volcanological parameters dynamics behavior.