We are currently interested on studying the surface of the Moon. We are producing the first high-resolution geological map of the Linné crater, located in Mare Serenitatis (Moon). By studying the abundance and size-frequency distribution of the ejected boulders surrounding the crater we can understand how the impact event occurred, as well as investigate the regolith thickness at the impact site.
For details, we redirect you to the publication of our work:
- Pajola et al., 2019: Abundance and size-frequency distribution of boulders in Linné crater’s ejecta (Moon),Planetary and Space Science,Volume 165,99-109