Abstract
A summary of lunar geology. Light feldspathic rocks which constitute the highland areas are components of the primeval crust of the Moon. Dark pyroxeneand ilmenite-rich basaltic lava flows — resulting from partial melting processes in the lunar mantle — filled the Maria basins, 3.1–3.9 × 109 years ago. Craters of all sizes and large circular basins were formed by impacting bodies from outside which produced the regolith blanket — a mass of comminuted rocks with fragments of impact breccias, impact melt glasses and impact melt rocks.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
