Ray of Boulders on the Moon
November 27, 2011
Dozens of boulders, ranging from 10 m to more than 30 m in diameter, are distributed within an ejecta ray close to the crater rim (lower right). These boulders represent the deepest material excavated during crater formation. LROC NAC M159013302LR, image width is ~850 m [NASA/GSFC/Arizona State University].
Topics: Fra Mauro formation, Lunar science, NASA/GSFC/Arizona State University, Arizona State University, National Aeronautics and Space Administration, Technology Internet