Meteoritics & Planetary Science 49, Nr 10, 1851–1874 (2014) doi: 10.1111/maps.12367 Ernst Julius Opik’s€ (1916) note on the theory of explosion cratering on the Moon’s surface—The complex case of a long-overlooked benchmark paper Grzegorz RACKI1*, Christian KOEBERL2,3,Tonu~ VIIK4, Elena A. JAGT-YAZYKOVA5,6, and John W. M. JAGT7 1Faculty of Earth Sciences, University of Silesia, ul. Bezdzinska 60, 41-200 Sosnowiec, Poland 2Department of Lithospheric Research, University of Vienna, 1090 Vienna, Austria 3Natural History Museum, Burgring 7, 1010 Vienna, Austria 4Tartu Observatory, Toravere,~ Tartumaa 61602, Estonia 5Laboratory of Paleobiology, Faculty of Natural and Technical Sciences, University of Opole, ul. Oleska 22, 45-052 Opole, Poland 6Saint Petersburg State University, Universitetskaya nab. 7-9, Saint Petersburg 199034, Russia 7Natuurhistorisch Museum Maastricht, de Bosquetplein 6-7, 6211 KJ Maastricht, the Netherlands *Corresponding author. E-mail:
[email protected] (Received 09 March 2014; revision accepted 02 August 2014) Abstract–High-velocity impact as a common phenomenon in planetary evolution was ignored until well into the twentieth century, mostly because of inadequate understanding of cratering processes. An eight-page note, published in Russian by the young Ernst Julius Opik,€ a great Estonian astronomer, was among the key selenological papers, but due to the language barrier, it was barely known and mostly incorrectly cited. This particular paper is here intended to serve as an explanatory supplement to an English translation of Opik’s€ article, but also to document an early stage in our understanding of cratering. First, we outline the historical–biographical background of this benchmark paper, and second, a comprehensive discussion of its merits is presented, from past and present perspectives alike.