Cosmochemistry and the Origin of Life: Proceedings of the NATO Advanced Study Institute held at Maratea, Italy, June 1–12, 1981
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1983
|
| Schriftenreihe: | NATO Advanced Study Institutes Series, Series C — Mathematical and Physical Sciences
101 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | For the first time in human history, developments in many branches of science provide us with an opportunity of formulating a comprehensive picture of the universe from its beginning to the present time. It is an awesome reflection that the carbon in our bodies is the very carbon which was generated during the birth of a star. There is a perceptible continuum through the billions of years which can be revealed by the study of chemistry. Studies in nucleosynthesis have related the origin of the elements to the life history of the stars. The chemical elements we find on earth, Hydrogen, Carbon, Oxygen, and Nitrogen, were created in astronomical processes that took place in the past, and these elements are not spread throughout space in the form of stars and galaxies. Radioastronomers have discovered a vast array of organic molecules in the interstellar medium which have a bearing on prebiological chemical processes. Many of the molecules found so far contain the four elements, C, N, O, H. Except for the chemically unreactive He, these four elements are the most abundant in the galaxy. The origin of polyatomic interstellar molecules is an unresolved problem. While we can explain the formation of some diatomic molecules as due to two atom collisions, it is much more difficult to form polyatomic molecules by collisions between diatomic molecules and atoms. There may be other production mechanisms at work such as reactions taking place on the surface of interstellar dust grains |
| Beschreibung: | 1 Online-Ressource (VIII, 386 p) |
| ISBN: | 9789400970724 9789400970748 |
| DOI: | 10.1007/978-94-009-7072-4 |
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| 245 | 1 | 0 | |a Cosmochemistry and the Origin of Life |b Proceedings of the NATO Advanced Study Institute held at Maratea, Italy, June 1–12, 1981 |c edited by Cyril Ponnamperuma |
| 246 | 1 | 3 | |a Proceedings of the NATO Advanced Study Institute, Maratea, Italy, June 1-12, 1981 |
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| 490 | 1 | |a NATO Advanced Study Institutes Series, Series C — Mathematical and Physical Sciences |v 101 | |
| 500 | |a For the first time in human history, developments in many branches of science provide us with an opportunity of formulating a comprehensive picture of the universe from its beginning to the present time. It is an awesome reflection that the carbon in our bodies is the very carbon which was generated during the birth of a star. There is a perceptible continuum through the billions of years which can be revealed by the study of chemistry. Studies in nucleosynthesis have related the origin of the elements to the life history of the stars. The chemical elements we find on earth, Hydrogen, Carbon, Oxygen, and Nitrogen, were created in astronomical processes that took place in the past, and these elements are not spread throughout space in the form of stars and galaxies. Radioastronomers have discovered a vast array of organic molecules in the interstellar medium which have a bearing on prebiological chemical processes. Many of the molecules found so far contain the four elements, C, N, O, H. Except for the chemically unreactive He, these four elements are the most abundant in the galaxy. The origin of polyatomic interstellar molecules is an unresolved problem. While we can explain the formation of some diatomic molecules as due to two atom collisions, it is much more difficult to form polyatomic molecules by collisions between diatomic molecules and atoms. There may be other production mechanisms at work such as reactions taking place on the surface of interstellar dust grains | ||
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Datensatz im Suchindex
| _version_ | 1804153082231128064 |
|---|---|
| any_adam_object | |
| author | Ponnamperuma, Cyril 1923-1994 |
| author_GND | (DE-588)17231139X |
| author_facet | Ponnamperuma, Cyril 1923-1994 |
| author_role | aut |
| author_sort | Ponnamperuma, Cyril 1923-1994 |
| author_variant | c p cp |
| building | Verbundindex |
| bvnumber | BV042415314 |
| classification_tum | PHY 000 |
| collection | ZDB-2-PHA ZDB-2-BAE |
| ctrlnum | (OCoLC)863790405 (DE-599)BVBBV042415314 |
| dewey-full | 523.01 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.01 |
| dewey-search | 523.01 |
| dewey-sort | 3523.01 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1007/978-94-009-7072-4 |
| format | Electronic eBook |
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| id | DE-604.BV042415314 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:57Z |
| institution | BVB |
| isbn | 9789400970724 9789400970748 |
| language | English |
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| physical | 1 Online-Ressource (VIII, 386 p) |
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| publisher | Springer Netherlands |
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| series | NATO Advanced Study Institutes Series, Series C — Mathematical and Physical Sciences |
| series2 | NATO Advanced Study Institutes Series, Series C — Mathematical and Physical Sciences |
| spelling | Ponnamperuma, Cyril 1923-1994 Verfasser (DE-588)17231139X aut Cosmochemistry and the Origin of Life Proceedings of the NATO Advanced Study Institute held at Maratea, Italy, June 1–12, 1981 edited by Cyril Ponnamperuma Proceedings of the NATO Advanced Study Institute, Maratea, Italy, June 1-12, 1981 Dordrecht Springer Netherlands 1983 1 Online-Ressource (VIII, 386 p) txt rdacontent c rdamedia cr rdacarrier NATO Advanced Study Institutes Series, Series C — Mathematical and Physical Sciences 101 For the first time in human history, developments in many branches of science provide us with an opportunity of formulating a comprehensive picture of the universe from its beginning to the present time. It is an awesome reflection that the carbon in our bodies is the very carbon which was generated during the birth of a star. There is a perceptible continuum through the billions of years which can be revealed by the study of chemistry. Studies in nucleosynthesis have related the origin of the elements to the life history of the stars. The chemical elements we find on earth, Hydrogen, Carbon, Oxygen, and Nitrogen, were created in astronomical processes that took place in the past, and these elements are not spread throughout space in the form of stars and galaxies. Radioastronomers have discovered a vast array of organic molecules in the interstellar medium which have a bearing on prebiological chemical processes. Many of the molecules found so far contain the four elements, C, N, O, H. Except for the chemically unreactive He, these four elements are the most abundant in the galaxy. The origin of polyatomic interstellar molecules is an unresolved problem. While we can explain the formation of some diatomic molecules as due to two atom collisions, it is much more difficult to form polyatomic molecules by collisions between diatomic molecules and atoms. There may be other production mechanisms at work such as reactions taking place on the surface of interstellar dust grains Physics Geochemistry Astrophysics and Astroparticles Leben (DE-588)4034831-3 gnd rswk-swf Entstehung (DE-588)4156614-2 gnd rswk-swf Chemische Evolution (DE-588)4147631-1 gnd rswk-swf Kosmochemie (DE-588)4133733-5 gnd rswk-swf 1\p (DE-588)1071861417 Konferenzschrift 1981 Maratea gnd-content 2\p (DE-588)1071861417 Konferenzschrift gnd-content Kosmochemie (DE-588)4133733-5 s Leben (DE-588)4034831-3 s Entstehung (DE-588)4156614-2 s 3\p DE-604 Chemische Evolution (DE-588)4147631-1 s 4\p DE-604 NATO Advanced Study Institutes Series, Series C — Mathematical and Physical Sciences 101 (DE-604)BV000003915 101 https://doi.org/10.1007/978-94-009-7072-4 Verlag 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 3\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 4\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Ponnamperuma, Cyril 1923-1994 Cosmochemistry and the Origin of Life Proceedings of the NATO Advanced Study Institute held at Maratea, Italy, June 1–12, 1981 NATO Advanced Study Institutes Series, Series C — Mathematical and Physical Sciences Physics Geochemistry Astrophysics and Astroparticles Leben (DE-588)4034831-3 gnd Entstehung (DE-588)4156614-2 gnd Chemische Evolution (DE-588)4147631-1 gnd Kosmochemie (DE-588)4133733-5 gnd |
| subject_GND | (DE-588)4034831-3 (DE-588)4156614-2 (DE-588)4147631-1 (DE-588)4133733-5 (DE-588)1071861417 |
| title | Cosmochemistry and the Origin of Life Proceedings of the NATO Advanced Study Institute held at Maratea, Italy, June 1–12, 1981 |
| title_alt | Proceedings of the NATO Advanced Study Institute, Maratea, Italy, June 1-12, 1981 |
| title_auth | Cosmochemistry and the Origin of Life Proceedings of the NATO Advanced Study Institute held at Maratea, Italy, June 1–12, 1981 |
| title_exact_search | Cosmochemistry and the Origin of Life Proceedings of the NATO Advanced Study Institute held at Maratea, Italy, June 1–12, 1981 |
| title_full | Cosmochemistry and the Origin of Life Proceedings of the NATO Advanced Study Institute held at Maratea, Italy, June 1–12, 1981 edited by Cyril Ponnamperuma |
| title_fullStr | Cosmochemistry and the Origin of Life Proceedings of the NATO Advanced Study Institute held at Maratea, Italy, June 1–12, 1981 edited by Cyril Ponnamperuma |
| title_full_unstemmed | Cosmochemistry and the Origin of Life Proceedings of the NATO Advanced Study Institute held at Maratea, Italy, June 1–12, 1981 edited by Cyril Ponnamperuma |
| title_short | Cosmochemistry and the Origin of Life |
| title_sort | cosmochemistry and the origin of life proceedings of the nato advanced study institute held at maratea italy june 1 12 1981 |
| title_sub | Proceedings of the NATO Advanced Study Institute held at Maratea, Italy, June 1–12, 1981 |
| topic | Physics Geochemistry Astrophysics and Astroparticles Leben (DE-588)4034831-3 gnd Entstehung (DE-588)4156614-2 gnd Chemische Evolution (DE-588)4147631-1 gnd Kosmochemie (DE-588)4133733-5 gnd |
| topic_facet | Physics Geochemistry Astrophysics and Astroparticles Leben Entstehung Chemische Evolution Kosmochemie Konferenzschrift 1981 Maratea Konferenzschrift |
| url | https://doi.org/10.1007/978-94-009-7072-4 |
| volume_link | (DE-604)BV000003915 |
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