The geology of multi-ring impact basins: the Moon and other planets
Multi-ring basins are large impact craters formed in the early history of planets. They critically affect the evolution of the planets and their satellites. The Moon offers an exceptional chance to study these phenomena and this book provides a comprehensive geological study using data from lunar la...
Saved in:
| Main Author: | |
|---|---|
| Format: | Electronic eBook |
| Language: | English |
| Published: |
Cambridge
Cambridge University Press
1993
|
| Series: | Cambridge planetary science
8 |
| Subjects: | |
| Online Access: | BSB01 FHN01 Volltext |
| Summary: | Multi-ring basins are large impact craters formed in the early history of planets. They critically affect the evolution of the planets and their satellites. The Moon offers an exceptional chance to study these phenomena and this book provides a comprehensive geological study using data from lunar landings and remote sensing of the Moon. The author covers the formation and development of basins and considers their chemistry and mineralogy. He studies their effects on the volcanic, tectonic and geological evolution of the planet, including the catastrophic consequence on the planetary climate and evolution of life. This study is lavishly illustrated with many spectacular, highly-detailed photographs and diagrams |
| Item Description: | Title from publisher's bibliographic system (viewed on 05 Oct 2015) |
| Physical Description: | 1 online resource (xiii, 263 pages) |
| ISBN: | 9780511564581 |
| DOI: | 10.1017/CBO9780511564581 |
Staff View
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| 505 | 8 | |a 1. The multi-ring basin problem. 1.1. Multi-ring basins and their significance. 1.2. Overview of the lunar multi-ring basin controversy. 1.3. The approach of this book -- 2. From crater to basin. 2.1. The cratering process. 2.2. The morphology of fresh lunar craters. 2.3. Size-dependent morphologic thresholds: crater to basin. 2.4. Inventory of lunar multi-ring basins -- 3. The 'archetype' basin: Orientale. 3.1. Regional geology of the Orientale impact site. 3.2. Orientale morphology and geological units. 3.3. Rings and basin structures. 3.4. Remote sensing of Orientale basin deposits. 3.5. Orientale ejecta at Apollo landing sites? 3.6. The formation and evolution of the Orientale basin -- 4. An ancient basin: Nectaris. 4.1. Regional geology and setting. 4.2. Nectaris morphology and geological units. 4.3. Remote sensing observations of Nectaris basin deposits. 4.4. Apollo 16 site petrology -- the Nectaris component. 4.5. The formation and evolution of the Nectaris Basin -- 5. A modified basin: Crisium | |
| 505 | 8 | |a 5.1. Regional geological setting. 5.2. Crisium morphology and geological units. 5.3. Structural geology and rings of the Crisium basin. 5.4. Composition of Crisium basin deposits. 5.5. Crisium ejecta: petrology of the Luna 20 site. 5.6. The formation and evolution of the Crisium basin -- 6. A transitional basin: Serenitatis. 6.1. Regional geological setting and basin definition. 6.2. Serenitatis morphology and geological units. 6.3. Serenitatis basin rings and structure. 6.4. Orbital geochemical data for Serenitatis basin deposits. 6.5. Apollo 17 site geology -- the Serenitatis basin "melt sheet" 6.6. The formation and evolution of the Serenitatis basin -- 7. The largest basin: Imbrium. 7.1. Regional geology and settings. 7.2. Imbrium morphology and geological units. 7.3. Imbrium rings and basin structures. 7.4. Remote-sensing data: the composition of Imbrium ejecta. 7.5. The Fra Mauro Formation: petrology of the Apollo 14 site. 7.6. The Apennine Mountains: petrology of the Apollo 15 site | |
| 505 | 8 | |a 7.7. Petrology of the Apollo 16 site -- Imbrium basin ejecta? 7.8. The formation and evolution of the Imbrium basin -- 8. Geological processes in the formation of lunar basins. 8.1. Composition and structure of the lunar crust. 8.2. Excavation. 8.3. Impact melt and ejecta. 8.4. Ring formation. 8.5. Long-term modification of basin topography -- 9. Multi-ring basins on the terrestrial planets. 9.1. Earth. 9.2. Mercury. 9.3. Mars. 9.4. Icy satellites of Jupiter and Saturn. 9.5. Venus -- 10. Multi-ring basins and planetary evolution. 10.1. The building blocks of planetary surfaces. 10.2. Effects of basins on planetary evolution. 10.3. Conclusion | |
| 520 | |a Multi-ring basins are large impact craters formed in the early history of planets. They critically affect the evolution of the planets and their satellites. The Moon offers an exceptional chance to study these phenomena and this book provides a comprehensive geological study using data from lunar landings and remote sensing of the Moon. The author covers the formation and development of basins and considers their chemistry and mineralogy. He studies their effects on the volcanic, tectonic and geological evolution of the planet, including the catastrophic consequence on the planetary climate and evolution of life. This study is lavishly illustrated with many spectacular, highly-detailed photographs and diagrams | ||
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Record in the Search Index
| _version_ | 1804176883996164096 |
|---|---|
| any_adam_object | |
| author | Spudis, Paul D. |
| author_facet | Spudis, Paul D. |
| author_role | aut |
| author_sort | Spudis, Paul D. |
| author_variant | p d s pd pds |
| building | Verbundindex |
| bvnumber | BV043941810 |
| classification_rvk | US 8340 US 8900 |
| collection | ZDB-20-CBO |
| contents | 1. The multi-ring basin problem. 1.1. Multi-ring basins and their significance. 1.2. Overview of the lunar multi-ring basin controversy. 1.3. The approach of this book -- 2. From crater to basin. 2.1. The cratering process. 2.2. The morphology of fresh lunar craters. 2.3. Size-dependent morphologic thresholds: crater to basin. 2.4. Inventory of lunar multi-ring basins -- 3. The 'archetype' basin: Orientale. 3.1. Regional geology of the Orientale impact site. 3.2. Orientale morphology and geological units. 3.3. Rings and basin structures. 3.4. Remote sensing of Orientale basin deposits. 3.5. Orientale ejecta at Apollo landing sites? 3.6. The formation and evolution of the Orientale basin -- 4. An ancient basin: Nectaris. 4.1. Regional geology and setting. 4.2. Nectaris morphology and geological units. 4.3. Remote sensing observations of Nectaris basin deposits. 4.4. Apollo 16 site petrology -- the Nectaris component. 4.5. The formation and evolution of the Nectaris Basin -- 5. A modified basin: Crisium 5.1. Regional geological setting. 5.2. Crisium morphology and geological units. 5.3. Structural geology and rings of the Crisium basin. 5.4. Composition of Crisium basin deposits. 5.5. Crisium ejecta: petrology of the Luna 20 site. 5.6. The formation and evolution of the Crisium basin -- 6. A transitional basin: Serenitatis. 6.1. Regional geological setting and basin definition. 6.2. Serenitatis morphology and geological units. 6.3. Serenitatis basin rings and structure. 6.4. Orbital geochemical data for Serenitatis basin deposits. 6.5. Apollo 17 site geology -- the Serenitatis basin "melt sheet" 6.6. The formation and evolution of the Serenitatis basin -- 7. The largest basin: Imbrium. 7.1. Regional geology and settings. 7.2. Imbrium morphology and geological units. 7.3. Imbrium rings and basin structures. 7.4. Remote-sensing data: the composition of Imbrium ejecta. 7.5. The Fra Mauro Formation: petrology of the Apollo 14 site. 7.6. The Apennine Mountains: petrology of the Apollo 15 site 7.7. Petrology of the Apollo 16 site -- Imbrium basin ejecta? 7.8. The formation and evolution of the Imbrium basin -- 8. Geological processes in the formation of lunar basins. 8.1. Composition and structure of the lunar crust. 8.2. Excavation. 8.3. Impact melt and ejecta. 8.4. Ring formation. 8.5. Long-term modification of basin topography -- 9. Multi-ring basins on the terrestrial planets. 9.1. Earth. 9.2. Mercury. 9.3. Mars. 9.4. Icy satellites of Jupiter and Saturn. 9.5. Venus -- 10. Multi-ring basins and planetary evolution. 10.1. The building blocks of planetary surfaces. 10.2. Effects of basins on planetary evolution. 10.3. Conclusion |
| ctrlnum | (ZDB-20-CBO)CR9780511564581 (OCoLC)849941156 (DE-599)BVBBV043941810 |
| dewey-full | 551.3/97/09991 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 551 - Geology, hydrology, meteorology |
| dewey-raw | 551.3/97/09991 |
| dewey-search | 551.3/97/09991 |
| dewey-sort | 3551.3 297 49991 |
| dewey-tens | 550 - Earth sciences |
| discipline | Geologie / Paläontologie Physik |
| doi_str_mv | 10.1017/CBO9780511564581 |
| format | Electronic eBook |
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| geographic_facet | Mond |
| id | DE-604.BV043941810 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T07:39:16Z |
| institution | BVB |
| isbn | 9780511564581 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-029350780 |
| oclc_num | 849941156 |
| open_access_boolean | |
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| owner_facet | DE-12 DE-92 |
| physical | 1 online resource (xiii, 263 pages) |
| psigel | ZDB-20-CBO ZDB-20-CBO BSB_PDA_CBO ZDB-20-CBO FHN_PDA_CBO |
| publishDate | 1993 |
| publishDateSearch | 1993 |
| publishDateSort | 1993 |
| publisher | Cambridge University Press |
| record_format | marc |
| series2 | Cambridge planetary science |
| spelling | Spudis, Paul D. Verfasser aut The geology of multi-ring impact basins the Moon and other planets Paul D. Spudis Cambridge Cambridge University Press 1993 1 online resource (xiii, 263 pages) txt rdacontent c rdamedia cr rdacarrier Cambridge planetary science 8 Title from publisher's bibliographic system (viewed on 05 Oct 2015) 1. The multi-ring basin problem. 1.1. Multi-ring basins and their significance. 1.2. Overview of the lunar multi-ring basin controversy. 1.3. The approach of this book -- 2. From crater to basin. 2.1. The cratering process. 2.2. The morphology of fresh lunar craters. 2.3. Size-dependent morphologic thresholds: crater to basin. 2.4. Inventory of lunar multi-ring basins -- 3. The 'archetype' basin: Orientale. 3.1. Regional geology of the Orientale impact site. 3.2. Orientale morphology and geological units. 3.3. Rings and basin structures. 3.4. Remote sensing of Orientale basin deposits. 3.5. Orientale ejecta at Apollo landing sites? 3.6. The formation and evolution of the Orientale basin -- 4. An ancient basin: Nectaris. 4.1. Regional geology and setting. 4.2. Nectaris morphology and geological units. 4.3. Remote sensing observations of Nectaris basin deposits. 4.4. Apollo 16 site petrology -- the Nectaris component. 4.5. The formation and evolution of the Nectaris Basin -- 5. A modified basin: Crisium 5.1. Regional geological setting. 5.2. Crisium morphology and geological units. 5.3. Structural geology and rings of the Crisium basin. 5.4. Composition of Crisium basin deposits. 5.5. Crisium ejecta: petrology of the Luna 20 site. 5.6. The formation and evolution of the Crisium basin -- 6. A transitional basin: Serenitatis. 6.1. Regional geological setting and basin definition. 6.2. Serenitatis morphology and geological units. 6.3. Serenitatis basin rings and structure. 6.4. Orbital geochemical data for Serenitatis basin deposits. 6.5. Apollo 17 site geology -- the Serenitatis basin "melt sheet" 6.6. The formation and evolution of the Serenitatis basin -- 7. The largest basin: Imbrium. 7.1. Regional geology and settings. 7.2. Imbrium morphology and geological units. 7.3. Imbrium rings and basin structures. 7.4. Remote-sensing data: the composition of Imbrium ejecta. 7.5. The Fra Mauro Formation: petrology of the Apollo 14 site. 7.6. The Apennine Mountains: petrology of the Apollo 15 site 7.7. Petrology of the Apollo 16 site -- Imbrium basin ejecta? 7.8. The formation and evolution of the Imbrium basin -- 8. Geological processes in the formation of lunar basins. 8.1. Composition and structure of the lunar crust. 8.2. Excavation. 8.3. Impact melt and ejecta. 8.4. Ring formation. 8.5. Long-term modification of basin topography -- 9. Multi-ring basins on the terrestrial planets. 9.1. Earth. 9.2. Mercury. 9.3. Mars. 9.4. Icy satellites of Jupiter and Saturn. 9.5. Venus -- 10. Multi-ring basins and planetary evolution. 10.1. The building blocks of planetary surfaces. 10.2. Effects of basins on planetary evolution. 10.3. Conclusion Multi-ring basins are large impact craters formed in the early history of planets. They critically affect the evolution of the planets and their satellites. The Moon offers an exceptional chance to study these phenomena and this book provides a comprehensive geological study using data from lunar landings and remote sensing of the Moon. The author covers the formation and development of basins and considers their chemistry and mineralogy. He studies their effects on the volcanic, tectonic and geological evolution of the planet, including the catastrophic consequence on the planetary climate and evolution of life. This study is lavishly illustrated with many spectacular, highly-detailed photographs and diagrams Multiring basins (Astrogeology) Lunar basins Lunar geology Planetary landforms Planet (DE-588)4046212-2 gnd rswk-swf Geologie (DE-588)4020227-6 gnd rswk-swf Mehrfachringbassin (DE-588)4349536-9 gnd rswk-swf Mond (DE-588)1085673251 gnd rswk-swf Mehrfachringbassin (DE-588)4349536-9 s Mond (DE-588)1085673251 g Geologie (DE-588)4020227-6 s 1\p DE-604 Planet (DE-588)4046212-2 s 2\p DE-604 Erscheint auch als Druckausgabe 978-0-521-26103-6 Erscheint auch als Druckausgabe 978-0-521-61923-3 https://doi.org/10.1017/CBO9780511564581 Verlag URL des Erstveröffentlichers Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 2\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Spudis, Paul D. The geology of multi-ring impact basins the Moon and other planets 1. The multi-ring basin problem. 1.1. Multi-ring basins and their significance. 1.2. Overview of the lunar multi-ring basin controversy. 1.3. The approach of this book -- 2. From crater to basin. 2.1. The cratering process. 2.2. The morphology of fresh lunar craters. 2.3. Size-dependent morphologic thresholds: crater to basin. 2.4. Inventory of lunar multi-ring basins -- 3. The 'archetype' basin: Orientale. 3.1. Regional geology of the Orientale impact site. 3.2. Orientale morphology and geological units. 3.3. Rings and basin structures. 3.4. Remote sensing of Orientale basin deposits. 3.5. Orientale ejecta at Apollo landing sites? 3.6. The formation and evolution of the Orientale basin -- 4. An ancient basin: Nectaris. 4.1. Regional geology and setting. 4.2. Nectaris morphology and geological units. 4.3. Remote sensing observations of Nectaris basin deposits. 4.4. Apollo 16 site petrology -- the Nectaris component. 4.5. The formation and evolution of the Nectaris Basin -- 5. A modified basin: Crisium 5.1. Regional geological setting. 5.2. Crisium morphology and geological units. 5.3. Structural geology and rings of the Crisium basin. 5.4. Composition of Crisium basin deposits. 5.5. Crisium ejecta: petrology of the Luna 20 site. 5.6. The formation and evolution of the Crisium basin -- 6. A transitional basin: Serenitatis. 6.1. Regional geological setting and basin definition. 6.2. Serenitatis morphology and geological units. 6.3. Serenitatis basin rings and structure. 6.4. Orbital geochemical data for Serenitatis basin deposits. 6.5. Apollo 17 site geology -- the Serenitatis basin "melt sheet" 6.6. The formation and evolution of the Serenitatis basin -- 7. The largest basin: Imbrium. 7.1. Regional geology and settings. 7.2. Imbrium morphology and geological units. 7.3. Imbrium rings and basin structures. 7.4. Remote-sensing data: the composition of Imbrium ejecta. 7.5. The Fra Mauro Formation: petrology of the Apollo 14 site. 7.6. The Apennine Mountains: petrology of the Apollo 15 site 7.7. Petrology of the Apollo 16 site -- Imbrium basin ejecta? 7.8. The formation and evolution of the Imbrium basin -- 8. Geological processes in the formation of lunar basins. 8.1. Composition and structure of the lunar crust. 8.2. Excavation. 8.3. Impact melt and ejecta. 8.4. Ring formation. 8.5. Long-term modification of basin topography -- 9. Multi-ring basins on the terrestrial planets. 9.1. Earth. 9.2. Mercury. 9.3. Mars. 9.4. Icy satellites of Jupiter and Saturn. 9.5. Venus -- 10. Multi-ring basins and planetary evolution. 10.1. The building blocks of planetary surfaces. 10.2. Effects of basins on planetary evolution. 10.3. Conclusion Multiring basins (Astrogeology) Lunar basins Lunar geology Planetary landforms Planet (DE-588)4046212-2 gnd Geologie (DE-588)4020227-6 gnd Mehrfachringbassin (DE-588)4349536-9 gnd |
| subject_GND | (DE-588)4046212-2 (DE-588)4020227-6 (DE-588)4349536-9 (DE-588)1085673251 |
| title | The geology of multi-ring impact basins the Moon and other planets |
| title_auth | The geology of multi-ring impact basins the Moon and other planets |
| title_exact_search | The geology of multi-ring impact basins the Moon and other planets |
| title_full | The geology of multi-ring impact basins the Moon and other planets Paul D. Spudis |
| title_fullStr | The geology of multi-ring impact basins the Moon and other planets Paul D. Spudis |
| title_full_unstemmed | The geology of multi-ring impact basins the Moon and other planets Paul D. Spudis |
| title_short | The geology of multi-ring impact basins |
| title_sort | the geology of multi ring impact basins the moon and other planets |
| title_sub | the Moon and other planets |
| topic | Multiring basins (Astrogeology) Lunar basins Lunar geology Planetary landforms Planet (DE-588)4046212-2 gnd Geologie (DE-588)4020227-6 gnd Mehrfachringbassin (DE-588)4349536-9 gnd |
| topic_facet | Multiring basins (Astrogeology) Lunar basins Lunar geology Planetary landforms Planet Geologie Mehrfachringbassin Mond |
| url | https://doi.org/10.1017/CBO9780511564581 |
| work_keys_str_mv | AT spudispauld thegeologyofmultiringimpactbasinsthemoonandotherplanets |