Skip to main content Accessibility help
×
Hostname: page-component-848d4c4894-ndmmz Total loading time: 0 Render date: 2024-04-30T18:36:42.330Z Has data issue: false hasContentIssue false

10 - Geology and Evolution of the Moon

Published online by Cambridge University Press:  06 April 2018

Kieran D. O'Hara
Affiliation:
University of Kentucky
Get access

Summary

Image of the first page of this content. For PDF version, please use the ‘Save PDF’ preceeding this image.'
Type
Chapter
Information
Publisher: Cambridge University Press
Print publication year: 2018

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Galilei, Galileo. 1610 (2004). Sidereus Nuncius. Trans., Carlos, E. S., London, 1880. Barker, P. (ed.), Byzantium Press, Oklahoma City.Google Scholar
Baldwin, R. B. 1949. The Face of the Moon. University Chicago Press, Chicago.Google Scholar
Gilbert, G. K. 1893. The moon’s face: the study of the origin of its features. Bulletin of Philosophical Society of Washington, v. 12, 241292.Google Scholar
Urey, H. C. 1951. The origin and development of the Earth and other terrestrial planets. Geochimica et Cosmochimica Acta, v. 1, 209277.Google Scholar
Shoemaker, E. and Hackman, R. J. 1962. Stratigraphic Basis for a Lunar Time Scale. In The Moon, Kopal, Z. (ed.), Academic Press, New York, 289300.Google Scholar
Wilhelms, D. E. and McCauley, J. F. 1971. Geologic map of the near side of the moon. Scale 1: 5,000,000. United States Geologic Survey, Washington, DC.Google Scholar
Wilhelms, D. E. 1987. The Geologic History of the Moon. United States Geologic Professional paper 1348, Washington, DC.Google Scholar
Stuart-Alexander, D. E and Howard, K. A. 1970. Lunar maria and circular basins – a review. ICARUS, v. 12, 440448.CrossRefGoogle Scholar
Stöffler, D. and Ryder, G. 2001. Stratigraphic and isotope ages of lunar geologic units: chronological standard for the inner solar system. Space Science Reviews, v. 96, 954.Google Scholar
Taylor, S. R. 1975. Lunar Science: a Post-Apollo View. Pergamon Press, New York.Google Scholar
LSPET Apollo 11. 1969. Science, v. 165, 12111127.CrossRefGoogle Scholar
The Moon Issue. 1970. Science, v. 167, 415794.Google Scholar
LSPET Apollo 12. 1970. Science, v. 167, 13251339.Google Scholar
Schonfeld, E. 1974. The contamination of lunar highland rocks by KREEP: interpretation of mixing models. In Kopal, Z. (ed.), Proceedings of the 5th Lunar Science Conference, v. 2, 12691286. Pergamon Press, New York.Google Scholar
Gromet, L. P., Hess, P. C., and Rutherford, M. J. 1981. An origin for the REE characteristics of KREEP. In Kopal, Z. (ed.), Proceedings 12th Lunar Science Conference, v. 1, 903913. Pergamon Press, New York.Google Scholar
LSPET Apollo 14. 1971. Science, v. 173, 681693.Google Scholar
Apollo Lunar Investigation Team. 1972. Geologic setting of Apollo 15 samples. Science, v. 175, 407415.Google Scholar
LSPET Apollo 15. 1972. Science, v. 175, 363693.Google Scholar
LSPET Apollo 16. 1973. The Apollo 16 lunar samples: petrographic and chemical description. Science, v. 179, 2334.Google Scholar
Schaeffer, O. A. and Husain, L. 1974. Chronology of lunar basin formation. In Kopal, Z. (ed.), Proceedings of the 5th Lunar Science Conference, v. 2, 15411555. Pergamon Press, New York.Google Scholar
Apollo Field Geology Investigation Team: Apollo 17 landing site. 1973. Geologic explanation of Taurus-Littrow site. Science, v. 182, 672680.Google Scholar
LSPET Apollo 17. 1973. Apollo 17 lunar samples: chemical and petrographic description. Science, v. 182, 659672.CrossRefGoogle Scholar
Warren, P. H. 1985. The Magma ocean concept and lunar evolution. Annual Review Earth Planetary Science, v. 13, 210240.Google Scholar
Shih, C. Y., Nyquist, L. E., Dasch, E. J., et al. 1993. Ages of pristine norite clasts from lunar breccias 15445 and 15455. Geochimica et Cosmochimica Acta, v. 57, 915931.Google Scholar
Tatsumoto, M and Rosholt, J. N. 1970. Age of the Moon: an isotopic study of U-Th-Pb systematic of lunar samples. Science, v. 167, 461463.Google Scholar
Wood, J. A., Dickey, J. S., Marvin, U. B. and Powell, B. N. 1970. Lunar anorthosites. Science, v. 167, 602604.Google Scholar
Wood, J. A., Dickey, J. S. Marvin, U. B. and Powell, B. N. 1970. Lunar anorthosites and a geophysical model of the moon. Proceedings of the Apollo 11 Lunar Science Conference, v. 1, 965988.Google Scholar
Phinney, R. A., O’Keefe, J. A., Adams, J. B., et al. 1969. Implications of the Surveyor 7 results. Journal of Geophysical Research, v. 74, 60536080.Google Scholar
Walker, D. and Hays, J. F. 1977. Plagioclase floatation and lunar crust formation. Geology, v. 5, 425428.2.0.CO;2>CrossRefGoogle Scholar
Taylor, S. R. and McLennan, S. M. 2009. Planetary Crusts: Their Composition, Origin and Evolution. Cambridge University Press, Cambridge.Google Scholar
Adler, I and Trombka, J. I. 1977. Orbital chemistry: lunar analysis from the X-ray and gamma ray remote sensing experiments. Physics and Chemistry of Earth, v. 10, 1743.Google Scholar
Wänke, H., Palme, K., Baddenhausen, H., et al. 1974. Chemistry of Apollo 16 and 17 samples: bulk composition, late stage accumulation and early differentiation of the moon. Proceedings of the 5th Lunar Science Conference, v. 2, 13071334. Pergamon Press, New York.Google Scholar
Taylor, S. R. and Jakes, P. 1974. The geochemical evolution of the moon. Proceedings of the 5th Lunar Science Conference, v. 2, 12871305. Pergamon Press, New York.Google Scholar
Ganapathy, R. and Anders, E. 1974. Bulk compositions of the moon and the Earth, estimated from meteorites. Proceedings of the 5th Lunar Science Conference, v. 2, 11811206. Pergamon Press, New York.Google Scholar
Ringwood, A. E. 1976. Limits on the bulk composition of the moon. ICARUS, v. 28, 325349.Google Scholar
Head, J. W. 1976. Lunar volcanism in space and time. Reviews of Geophysics and Space Physics, v. 14, 265300.Google Scholar
Basaltic Volcanism Study Project. 1981. Basaltic Volcanism on the Terrestrial Planets. Pergamon Press, New York.Google Scholar
Haskin, L. A. 1989. Rare earth elements in lunar materials. In Geochemistry and Mineralogy of the Rare Earth Elements, Lipin, B. R. and McKay, G. A. (eds.). Reviews in Mineralogy, v. 21. Mineralogical Society America, Washington DC.Google Scholar
Darwin, G. H. 1880. On the secular changes in the elements of the orbit of a satellite revolving about a tidally distorted planet. Philosophical Transactions of Royal Society of London, v. 171, 713891.Google Scholar
Ringwood, A. E. 1979. Origin of the Earth and Moon. Springer-Verlag, New York.Google Scholar
Stevenson, D. J. 1987. Origin of the moon: The collision hypothesis. Annual Review of Earth Planetary Science, 15, 271315.Google Scholar
Orloff, R. 2004. Apollo by the Numbers. National Air and Space Agency, Washington, DC.Google Scholar

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×