9789027715449 - cosmochemistry and the origin of life: proceedings of the nato advanced study institute held at maratea, italy, june 1-12, 1981: 101 (nato science series c:, 101) (14 resultados)
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Hardcover. Condición: Gut. 386 S. Ehem. Bibliotheksexemplar mit Signatur und Stempel. GUTER Zustand, ein paar Gebrauchsspuren. Ex-library with stamp and library-signature. GOOD condition, some traces of use. K00916 9027715440 Sprache: Englisch Gewicht in Gramm: 1150.
Cosmochemistry and the Origin of Life : NATO Advanced Study Institutes Series
NATO Advanced Study Institute (1981 : Maratea, Italy); Ponnamperuma, Cyril (EDT); North Atlantic Treaty Organization. Scientific Affairs Division (COR)
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Gebunden. Condición: New.
Cosmochemistry and the Origin of Life : NATO Advanced Study Institutes Series
NATO Advanced Study Institute (1981 : Maratea, Italy); Ponnamperuma, Cyril (EDT); North Atlantic Treaty Organization. Scientific Affairs Division (COR)
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Cosmochemistry and the Origin of Life : NATO Advanced Study Institutes Series
NATO Advanced Study Institute (1981 : Maratea, Italy); Ponnamperuma, Cyril (EDT); North Atlantic Treaty Organization. Scientific Affairs Division (COR)
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Cosmochemistry and the Origin of Life : NATO Advanced Study Institutes Series
NATO Advanced Study Institute (1981 : Maratea, Italy); Ponnamperuma, Cyril (EDT); North Atlantic Treaty Organization. Scientific Affairs Division (COR)
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Buch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - For the first time in human history, developments in many branches of science provide us with an opportunity of formula ting 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, 0, H. Except for the chem ically 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 produc tion mechanisms at work such as reactions taking place on the surface of interstellar dust grains.
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Buch. Condición: Neu. Cosmochemistry and the Origin of Life | Proceedings of the NATO Advanced Study Institute held at Maratea, Italy, June 1-12, 1981 | Cyril Ponnamperuma | Buch | viii | Englisch | 1983 | Springer Netherland | EAN 9789027715449 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121…Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu Print on Demand.
Idioma: Inglés
Editorial: Springer Netherlands, Springer Netherlands Jan 1983, 1983
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Buch. Condición: Neu. This item is printed on demand - Print on Demand Titel. Neuware -For the first time in human history, developments in many branches of science provide us with an opportunity of formula ting a comprehensive picture of the universe from its beginning to the present time. It is an awesome reflection that the c…arbon 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, 0, H. Except for the chem ically 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 produc tion mechanisms at work such as reactions taking place on the surface of interstellar dust grains.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 400 pp. Englisch.
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Condición: New. Print on Demand pp. 404 54:B&W 6.14 x 9.21in or 234 x 156mm (Royal 8vo) Blue Cloth w/Jacket on White w/Gloss Lam.
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Condición: New. PRINT ON DEMAND pp. 404.
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Buch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -For the first time in human history, developments in many branches of science provide us with an opportunity of formula ting a comprehensive picture of the universe from its beginning to the present time. It is an awesome reflection that t…he 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, 0, H. Except for the chem ically 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 produc tion mechanisms at work such as reactions taking place on the surface of interstellar dust grains. 400 pp. Englisch.
