Magnetic Resonance Properties of Some Lunar Material
- 30 January 1970
- journal article
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 167 (3918), 704-707
- https://doi.org/10.1126/science.167.3918.704
Abstract
Paramagnetic resonance spectra of Apollo 11 fines and rocks were measured at 9 and 35 gigahertz and at 4°, 80°, and 300°K. At both frequencies the material has an intense absorption at g = 2, with a line width of ∼950 gauss. Fe ions with strong exchange interactions produce this resonance. A comparison of the resonance absorption due to Fe3+ showed that the energy of the crystal field interaction was ∼0.1 per centimeter. Mn2+ was identified in several samples, and an absorption at g = 1.89 was tentatively attributed to Ti3+. The nuclear magnetic resonance spectra of 27Al had a distribution of asymmetry parameters η ranging from 0.25 to 0.75 and had nuclear quadrupole coupling constants e2qQ/h of approximately 3 megahertz.This publication has 4 references indexed in Scilit:
- Preliminary Examination of Lunar Samples from Apollo 11Science, 1969
- Proton-induced hydroxyl formation on the lunar surfaceJournal of Geophysical Research, 1966
- Electron Spin Resonance of Magnetic Ions in Complex OxidesPublished by Elsevier BV ,1965
- SuperparamagnetismJournal of Applied Physics, 1959