Cosmochemistry:
How did the Solar System's chemical composition evolve? This textbook provides the answers in the first interdisciplinary introduction to cosmochemistry. It makes this exciting and evolving field accessible to undergraduate and graduate students from a range of backgrounds, including geology, c...
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| 1. Verfasser: | |
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| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Cambridge
Cambridge University Press
2010
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| Schlagworte: | |
| Online-Zugang: | BSB01 FHN01 Volltext |
| Zusammenfassung: | How did the Solar System's chemical composition evolve? This textbook provides the answers in the first interdisciplinary introduction to cosmochemistry. It makes this exciting and evolving field accessible to undergraduate and graduate students from a range of backgrounds, including geology, chemistry, astronomy and physics. The authors - two established leaders who have pioneered developments in the field - provide a complete background to cosmochemical processes and discoveries, enabling students outside geochemistry to understand and explore the Solar System's composition. Topics covered include: - synthesis of nuclides in stars - partitioning of elements between solids, liquids and gas in the solar nebula - overviews of the chemistry of extraterrestrial materials - isotopic tools used to investigate processes such as planet accretion and element fractionation - chronology of the early Solar System - geochemical exploration of planets Boxes provide basic definitions and mini-courses in mineralogy, organic chemistry, and other essential background information for students. Review questions and additional reading for each chapter encourage students to explore cosmochemistry further |
| Beschreibung: | Title from publisher's bibliographic system (viewed on 05 Oct 2015) |
| Beschreibung: | 1 online resource (xviii, 549 pages) |
| ISBN: | 9780511804502 |
| DOI: | 10.1017/CBO9780511804502 |
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| 505 | 8 | |a Machine generated contents note: Preface; 1. Introduction to cosmochemistry; 2. Nuclides and elements - the building blocks of matter; 3. Origin of the elements; 4. Solar System and cosmic abundances - elements and isotopes; 5. Presolar grains - a record of stellar nucleosynthesis and processes in interstellar space; 6. Meteorites - a record of nebular and planetary processes; 7. Cosmochemical and geochemical fractionations; 8. Radioisotopes as chronometers; 9. Chronology of the early Solar System; 10. The most volatile elements and compounds - organic matter, noble gases, and ices; 11. Chemistry of anhydrous planetesimals; 12. Chemistry of comets and other ice-bearing planetesimals; 13. Geochemical exploration of planets - Moon and Mars as case studies; 14. Cosmochemical models for the formation of the Solar System; Appendix: some analytical techniques commonly used in cosmochemistry; Index | |
| 520 | |a How did the Solar System's chemical composition evolve? This textbook provides the answers in the first interdisciplinary introduction to cosmochemistry. It makes this exciting and evolving field accessible to undergraduate and graduate students from a range of backgrounds, including geology, chemistry, astronomy and physics. The authors - two established leaders who have pioneered developments in the field - provide a complete background to cosmochemical processes and discoveries, enabling students outside geochemistry to understand and explore the Solar System's composition. Topics covered include: - synthesis of nuclides in stars - partitioning of elements between solids, liquids and gas in the solar nebula - overviews of the chemistry of extraterrestrial materials - isotopic tools used to investigate processes such as planet accretion and element fractionation - chronology of the early Solar System - geochemical exploration of planets Boxes provide basic definitions and mini-courses in mineralogy, organic chemistry, and other essential background information for students. Review questions and additional reading for each chapter encourage students to explore cosmochemistry further | ||
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Datensatz im Suchindex
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| contents | Machine generated contents note: Preface; 1. Introduction to cosmochemistry; 2. Nuclides and elements - the building blocks of matter; 3. Origin of the elements; 4. Solar System and cosmic abundances - elements and isotopes; 5. Presolar grains - a record of stellar nucleosynthesis and processes in interstellar space; 6. Meteorites - a record of nebular and planetary processes; 7. Cosmochemical and geochemical fractionations; 8. Radioisotopes as chronometers; 9. Chronology of the early Solar System; 10. The most volatile elements and compounds - organic matter, noble gases, and ices; 11. Chemistry of anhydrous planetesimals; 12. Chemistry of comets and other ice-bearing planetesimals; 13. Geochemical exploration of planets - Moon and Mars as case studies; 14. Cosmochemical models for the formation of the Solar System; Appendix: some analytical techniques commonly used in cosmochemistry; Index |
| ctrlnum | (ZDB-20-CBO)CR9780511804502 (OCoLC)774042994 (DE-599)BVBBV043943447 |
| dewey-full | 523/.02 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
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| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Chemie / Pharmazie Physik |
| doi_str_mv | 10.1017/CBO9780511804502 |
| format | Electronic eBook |
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| spelling | McSween, Harry Y. Verfasser aut Cosmochemistry Harry Y. McSween, Jr., Gary R. Huss Cambridge Cambridge University Press 2010 1 online resource (xviii, 549 pages) txt rdacontent c rdamedia cr rdacarrier Title from publisher's bibliographic system (viewed on 05 Oct 2015) Machine generated contents note: Preface; 1. Introduction to cosmochemistry; 2. Nuclides and elements - the building blocks of matter; 3. Origin of the elements; 4. Solar System and cosmic abundances - elements and isotopes; 5. Presolar grains - a record of stellar nucleosynthesis and processes in interstellar space; 6. Meteorites - a record of nebular and planetary processes; 7. Cosmochemical and geochemical fractionations; 8. Radioisotopes as chronometers; 9. Chronology of the early Solar System; 10. The most volatile elements and compounds - organic matter, noble gases, and ices; 11. Chemistry of anhydrous planetesimals; 12. Chemistry of comets and other ice-bearing planetesimals; 13. Geochemical exploration of planets - Moon and Mars as case studies; 14. Cosmochemical models for the formation of the Solar System; Appendix: some analytical techniques commonly used in cosmochemistry; Index How did the Solar System's chemical composition evolve? This textbook provides the answers in the first interdisciplinary introduction to cosmochemistry. It makes this exciting and evolving field accessible to undergraduate and graduate students from a range of backgrounds, including geology, chemistry, astronomy and physics. The authors - two established leaders who have pioneered developments in the field - provide a complete background to cosmochemical processes and discoveries, enabling students outside geochemistry to understand and explore the Solar System's composition. Topics covered include: - synthesis of nuclides in stars - partitioning of elements between solids, liquids and gas in the solar nebula - overviews of the chemistry of extraterrestrial materials - isotopic tools used to investigate processes such as planet accretion and element fractionation - chronology of the early Solar System - geochemical exploration of planets Boxes provide basic definitions and mini-courses in mineralogy, organic chemistry, and other essential background information for students. Review questions and additional reading for each chapter encourage students to explore cosmochemistry further Cosmochemistry Kosmochemie (DE-588)4133733-5 gnd rswk-swf 1\p (DE-588)4123623-3 Lehrbuch gnd-content Kosmochemie (DE-588)4133733-5 s 2\p DE-604 Huss, Gary R. Sonstige oth Erscheint auch als Druckausgabe 978-0-521-87862-3 https://doi.org/10.1017/CBO9780511804502 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 | McSween, Harry Y. Cosmochemistry Machine generated contents note: Preface; 1. Introduction to cosmochemistry; 2. Nuclides and elements - the building blocks of matter; 3. Origin of the elements; 4. Solar System and cosmic abundances - elements and isotopes; 5. Presolar grains - a record of stellar nucleosynthesis and processes in interstellar space; 6. Meteorites - a record of nebular and planetary processes; 7. Cosmochemical and geochemical fractionations; 8. Radioisotopes as chronometers; 9. Chronology of the early Solar System; 10. The most volatile elements and compounds - organic matter, noble gases, and ices; 11. Chemistry of anhydrous planetesimals; 12. Chemistry of comets and other ice-bearing planetesimals; 13. Geochemical exploration of planets - Moon and Mars as case studies; 14. Cosmochemical models for the formation of the Solar System; Appendix: some analytical techniques commonly used in cosmochemistry; Index Cosmochemistry Kosmochemie (DE-588)4133733-5 gnd |
| subject_GND | (DE-588)4133733-5 (DE-588)4123623-3 |
| title | Cosmochemistry |
| title_auth | Cosmochemistry |
| title_exact_search | Cosmochemistry |
| title_full | Cosmochemistry Harry Y. McSween, Jr., Gary R. Huss |
| title_fullStr | Cosmochemistry Harry Y. McSween, Jr., Gary R. Huss |
| title_full_unstemmed | Cosmochemistry Harry Y. McSween, Jr., Gary R. Huss |
| title_short | Cosmochemistry |
| title_sort | cosmochemistry |
| topic | Cosmochemistry Kosmochemie (DE-588)4133733-5 gnd |
| topic_facet | Cosmochemistry Kosmochemie Lehrbuch |
| url | https://doi.org/10.1017/CBO9780511804502 |
| work_keys_str_mv | AT mcsweenharryy cosmochemistry AT hussgaryr cosmochemistry |