ABSTRACT Maximum lunar seismic activity corresponds to the rise of the pulsar CP1133 at the site. Other agreement with Earth based experiments suggests that they have a common origin. Access

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al._, _Science_, 174, 687 (1971). Article  ADS  CAS  Google Scholar  * Sadeh, D., and Meidav, M., _Nature_, 240, 136 (1972). Article  ADS  Google Scholar  Download references AUTHOR

INFORMATION Author notes * DROR SADEH: And E. O. Hulburt Center for Space Research, Naval Research Laboratory, Washington DC 20390. AUTHORS AND AFFILIATIONS * Physics and Astronomy

Department, F. and G. Wise Observatory, University of Tel-Aviv, Tel-Aviv, Israel DROR SADEH Authors * DROR SADEH View author publications You can also search for this author inPubMed Google

Scholar RIGHTS AND PERMISSIONS Reprints and permissions ABOUT THIS ARTICLE CITE THIS ARTICLE SADEH, D. Possible Sidereal Period for the Seismic Lunar Activity. _Nature_ 240, 139–140 (1972).

https://doi.org/10.1038/240139a0 Download citation * Received: 26 June 1972 * Issue Date: 17 November 1972 * DOI: https://doi.org/10.1038/240139a0 SHARE THIS ARTICLE Anyone you share the

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