Chemistry of the Lower Atmosphere:
About three years ago Catherine de Berg and I published a short article in Nature in which we attempted to explain why the chemistry of the atmosphere of the Earth is today so completely different from that of our two neighbor ing planets, Mars and Venus. Our atmosphere is composed mainly of N2 and...
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| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Boston, MA
Springer US
1973
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| Online-Zugang: | BTU01 Volltext |
| Zusammenfassung: | About three years ago Catherine de Berg and I published a short article in Nature in which we attempted to explain why the chemistry of the atmosphere of the Earth is today so completely different from that of our two neighbor ing planets, Mars and Venus. Our atmosphere is composed mainly of N2 and O with traces of A, H0, CO , 0 , etc. , while the atmospheres of both 2 2 2 3 Mars and Venus are almost entirely made up of CO , Also, the Earth appears 2 to be the only one ofthe three planets which has oceans ofliquid water on the surface. Since the presence of liquid water on Earth is probably an essential requirement for life to have originated and evolved to its present state, the question of the apparent absence ofliquid water on Mars and Venus suddenly acquires significant proportions. In our paper in Nature, and later in a more detailed discussion of the subject (Planetary Atmospheres, in Exobiology, edited by C. Ponnamperuma, North Holland Publishing Co. ), we tried to describe why we believe that in the early history of the solar system all the terrestrial planets lost the atmospheres of H2 and He which they had acquired from the solar nebula at the time of their formation. These planets, completely devoid of atmos pheres, like the Moon today, started accumulating new gases which were exhumed from the interior by the commencement of volcanic activity |
| Beschreibung: | 1 Online-Ressource (XII, 335 p) |
| ISBN: | 9781468419863 |
| DOI: | 10.1007/978-1-4684-1986-3 |
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| 520 | |a About three years ago Catherine de Berg and I published a short article in Nature in which we attempted to explain why the chemistry of the atmosphere of the Earth is today so completely different from that of our two neighbor ing planets, Mars and Venus. Our atmosphere is composed mainly of N2 and O with traces of A, H0, CO , 0 , etc. , while the atmospheres of both 2 2 2 3 Mars and Venus are almost entirely made up of CO , Also, the Earth appears 2 to be the only one ofthe three planets which has oceans ofliquid water on the surface. Since the presence of liquid water on Earth is probably an essential requirement for life to have originated and evolved to its present state, the question of the apparent absence ofliquid water on Mars and Venus suddenly acquires significant proportions. In our paper in Nature, and later in a more detailed discussion of the subject (Planetary Atmospheres, in Exobiology, edited by C. Ponnamperuma, North Holland Publishing Co. ), we tried to describe why we believe that in the early history of the solar system all the terrestrial planets lost the atmospheres of H2 and He which they had acquired from the solar nebula at the time of their formation. These planets, completely devoid of atmos pheres, like the Moon today, started accumulating new gases which were exhumed from the interior by the commencement of volcanic activity | ||
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| illustrated | Not Illustrated |
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| isbn | 9781468419863 |
| language | English |
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| spelling | Chemistry of the Lower Atmosphere edited by S. I. Rasool Boston, MA Springer US 1973 1 Online-Ressource (XII, 335 p) txt rdacontent c rdamedia cr rdacarrier About three years ago Catherine de Berg and I published a short article in Nature in which we attempted to explain why the chemistry of the atmosphere of the Earth is today so completely different from that of our two neighbor ing planets, Mars and Venus. Our atmosphere is composed mainly of N2 and O with traces of A, H0, CO , 0 , etc. , while the atmospheres of both 2 2 2 3 Mars and Venus are almost entirely made up of CO , Also, the Earth appears 2 to be the only one ofthe three planets which has oceans ofliquid water on the surface. Since the presence of liquid water on Earth is probably an essential requirement for life to have originated and evolved to its present state, the question of the apparent absence ofliquid water on Mars and Venus suddenly acquires significant proportions. In our paper in Nature, and later in a more detailed discussion of the subject (Planetary Atmospheres, in Exobiology, edited by C. Ponnamperuma, North Holland Publishing Co. ), we tried to describe why we believe that in the early history of the solar system all the terrestrial planets lost the atmospheres of H2 and He which they had acquired from the solar nebula at the time of their formation. These planets, completely devoid of atmos pheres, like the Moon today, started accumulating new gases which were exhumed from the interior by the commencement of volcanic activity Earth Sciences Geochemistry Earth sciences Atmosphäre (DE-588)4003397-1 gnd rswk-swf Innere Atmosphäre (DE-588)4274385-0 gnd rswk-swf Atmosphäre (DE-588)4003397-1 s 1\p DE-604 Innere Atmosphäre (DE-588)4274385-0 s 2\p DE-604 Rasool, S. I. edt Erscheint auch als Druck-Ausgabe 9781468419887 https://doi.org/10.1007/978-1-4684-1986-3 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 | Chemistry of the Lower Atmosphere Earth Sciences Geochemistry Earth sciences Atmosphäre (DE-588)4003397-1 gnd Innere Atmosphäre (DE-588)4274385-0 gnd |
| subject_GND | (DE-588)4003397-1 (DE-588)4274385-0 |
| title | Chemistry of the Lower Atmosphere |
| title_auth | Chemistry of the Lower Atmosphere |
| title_exact_search | Chemistry of the Lower Atmosphere |
| title_full | Chemistry of the Lower Atmosphere edited by S. I. Rasool |
| title_fullStr | Chemistry of the Lower Atmosphere edited by S. I. Rasool |
| title_full_unstemmed | Chemistry of the Lower Atmosphere edited by S. I. Rasool |
| title_short | Chemistry of the Lower Atmosphere |
| title_sort | chemistry of the lower atmosphere |
| topic | Earth Sciences Geochemistry Earth sciences Atmosphäre (DE-588)4003397-1 gnd Innere Atmosphäre (DE-588)4274385-0 gnd |
| topic_facet | Earth Sciences Geochemistry Earth sciences Atmosphäre Innere Atmosphäre |
| url | https://doi.org/10.1007/978-1-4684-1986-3 |
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