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Planets and life /
The Earth is the only planet in the Solar System where liquid water is present on the surface, a condition that seems necessary for the development of life. Its sisters Venus and Mars are extremely different. Why did these three planets, born under fairly comparable conditions, evolve to the conditi...
| Clasificación: | Libro Electrónico |
|---|---|
| Autores principales: | , , |
| Formato: | Electrónico eBook |
| Idioma: | Inglés |
| Publicado: |
Les Ulis :
EDP Sciences,
[2021]
|
| Colección: | Current natural sciences.
|
| Temas: | |
| Acceso en línea: | Texto completo |
MARC
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| 003 | OCoLC | ||
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| 020 | |a 2759825701 | ||
| 020 | |a 9782759825707 |q (electronic bk.) | ||
| 024 | 7 | |a 10.1051/978-2-7598-2570-7 |2 doi | |
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| 100 | 1 | |a Encrenaz, Thérèse, |d 1946- |e author. |4 aut |4 http://id.loc.gov/vocabulary/relators/aut | |
| 245 | 1 | 0 | |a Planets and life / |c Thérèse Encrenaz, James Lequeux, Fabienne Casoli. |
| 264 | 1 | |a Les Ulis : |b EDP Sciences, |c [2021] | |
| 264 | 4 | |c ©2021 | |
| 300 | |a 1 online resource (166 pages) | ||
| 336 | |a text |b txt |2 rdacontent | ||
| 337 | |a computer |b c |2 rdamedia | ||
| 338 | |a online resource |b cr |2 rdacarrier | ||
| 347 | |a text file | ||
| 347 | |b PDF | ||
| 490 | 1 | |a Current Natural Sciences | |
| 505 | 0 | 0 | |t Frontmatter -- |t Foreword -- |t Contents -- |t Chapter 1. Introduction -- |t Chapter 2. The Formation of Terrestrial Planets -- |t Chapter 3. The Exploration of Terrestrial Planets -- |t Chapter 4. Venus, Earth and Mars: A Diverging Evolution -- |t Chapter 5. The Appearance of Life -- |t Chapter 6. The Development of Life on Earth -- |t Chapter 7. Life in the Solar System? -- |t Chapter 8. How to Search for Life on Rocky Exoplanets? -- |t Chapter 9. Conclusions: Some Future Directions in Exobiology -- |t Glossary -- |t Bibliography |
| 520 | |a The Earth is the only planet in the Solar System where liquid water is present on the surface, a condition that seems necessary for the development of life. Its sisters Venus and Mars are extremely different. Why did these three planets, born under fairly comparable conditions, evolve to the conditions we observe today? Understanding the physical or chemical factors that are at the origin of such divergent evolutions is a first step in an approach to the problem of the origin of life on Earth. | ||
| 546 | |a In English. | ||
| 588 | 0 | |a Online resource; title from PDF title page (publisher's Web site, viewed 27. Okt 2021). | |
| 590 | |a eBooks on EBSCOhost |b EBSCO eBook Subscription Academic Collection - Worldwide | ||
| 651 | 0 | |a Earth (Planet) | |
| 651 | 0 | |a Mars (Planet) | |
| 651 | 0 | |a Venus (Planet) | |
| 650 | 0 | |a Life |x Origin. | |
| 650 | 4 | |a Astrophysics. | |
| 651 | 6 | |a Terre. | |
| 651 | 6 | |a Mars (Planète) | |
| 651 | 6 | |a Vénus (Planète) | |
| 650 | 6 | |a Vie |x Origines. | |
| 650 | 7 | |a SCIENCE |x Physics |x Astrophysics. |2 bisacsh | |
| 650 | 7 | |a Life |x Origin |2 fast | |
| 651 | 7 | |a Earth (Planet) |2 fast | |
| 651 | 7 | |a Mars (Planet) |2 fast | |
| 651 | 7 | |a Venus (Planet) |2 fast | |
| 700 | 1 | |a Casoli, F. |q (Fabienne), |d 1959- |e author. |4 aut |4 http://id.loc.gov/vocabulary/relators/aut | |
| 700 | 1 | |a Lequeux, James, |e author |4 aut |4 http://id.loc.gov/vocabulary/relators/aut | |
| 776 | 0 | 8 | |i Print version: |z 9782759825639 |
| 830 | 0 | |a Current natural sciences. | |
| 856 | 4 | 0 | |u https://ebsco.uam.elogim.com/login.aspx?direct=true&scope=site&db=nlebk&AN=3102864 |z Texto completo |
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