Isotopic Composition of Rare Gases in Lunar Samples
- 30 January 1970
- journal article
- research article
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 167 (3918) , 550-553
- https://doi.org/10.1126/science.167.3918.550
Abstract
After successful acquisition in August of reflected ruby laser pulses from the Apollo 11 laser ranging retro-reflector (LRRR) with the telescopes at the Lick and McDonald observatories, repeated measurements of the round-trip travel time of light have been made from the McDonald Observatory in September with an equivalent range precision of ±2.5 meters. These acquisition period observations demonstrated the performance of the LRRR through lunar night and during sunlit conditions on the moon. Instrumentation activated at the McDonald Observatory in October has yielded a precision of ±0.3 meter, and improvement to ±0.15 meter is expected shortly. Continued monitoring of the changes in the earth-moon distance as measured by the round-trip travel time of light from suitably distributed earth stations is expected to contribute to our knowledge of the earth-moon system.Keywords
This publication has 6 references indexed in Scilit:
- Preliminary Examination of Lunar Samples from Apollo 11Science, 1969
- Spallation and fissiogenic xenon and krypton from stepwise heating of the Pasamonte achondrite; The case for extinct plutonium 244 in meteorites; Relative ages of chondrites and achondritesPublished by American Geophysical Union (AGU) ,1967
- Trapped neon in meteoritesEarth and Planetary Science Letters, 1967
- Krypton and xenon isotopic composition in three carbonaceous chondritesEarth and Planetary Science Letters, 1967
- Isotopic composition of trapped krypton and xenon in chondritesEarth and Planetary Science Letters, 1967
- Heavy rare gases in silicates from the Estherville mesosideriteJournal of Geophysical Research, 1966