Guilbert is a small (25.5 km diameter) impact crater on the surface of Venus. It has a continuous ejecta radius of 16.3 km, and a wall width of 2.5 km. Its name derives after Yvette Guilbert. It was accepted by the IAU in the year 1991.
Surrounding geology
The physical environment immediately surrounding the crater includes:
Lhamo Tessera, a remnant of an ancient tessera plateau (a complex ridged terrain experiencing intense multi-directional deformation). Eithinoha Corona, a large (400 km in diameter) circular structure categorized as a corona (a near-circular volcanotectonic feature). Hsueh T'ao Crater, a young, mid-size impact crater to the north.
References
Sources Hamilton, Warren B. (2005). "Plumeless Venus preserves an ancient impact-accretionary surface". In Foulger, G. R.; Natland, J. H.; Presnall, D. C.; Anderson, D. L. (eds.). Plates, Plumes, and Paradigms. Geological Society of America Special Paper. Vol. 388. Geological Society of America. pp. 781–814. doi:10.1130/2005.2388(44).



