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Protoplanetary Dust: Astrophysical and Cosmochemical Perspectives [Mīkstie vāki]

Edited by (University of Arizona), Edited by (Space Telescope Science Institute, Baltimore)
  • Formāts: Paperback / softback, 396 pages, height x width x depth: 244x170x21 mm, weight: 630 g, Worked examples or Exercises; Printed music items
  • Sērija : Cambridge Planetary Science
  • Izdošanas datums: 20-Feb-2014
  • Izdevniecība: Cambridge University Press
  • ISBN-10: 110762942X
  • ISBN-13: 9781107629424
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  • Mīkstie vāki
  • Cena: 75,52 €
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Protoplanetary Dust: Astrophysical and Cosmochemical PerspectivesPalielināt
  • Formāts: Paperback / softback, 396 pages, height x width x depth: 244x170x21 mm, weight: 630 g, Worked examples or Exercises; Printed music items
  • Sērija : Cambridge Planetary Science
  • Izdošanas datums: 20-Feb-2014
  • Izdevniecība: Cambridge University Press
  • ISBN-10: 110762942X
  • ISBN-13: 9781107629424
Citas grāmatas par šo tēmu:
Permanent link: https://www.kriso.lv/db/9781107629424.html
Keywords:
Planet formation studies uniquely benefit from three disciplines: astronomical observations of extrasolar planet-forming disks, analysis of material from the early Solar System, and laboratory astrophysics experiments. Pre-planetary solids, fine dust, and chondritic components are central elements linking these studies. This book is the first comprehensive overview of planet formation, in which astronomers, cosmochemists, and laboratory astrophysicists jointly discuss the latest insights from the Spitzer and Hubble space telescopes, new interferometers, space missions including Stardust and Deep Impact, and laboratory techniques. Following the evolution of solids from their genesis through protoplanetary disks to rocky planets, the book discusses in detail how the latest results from these disciplines fit into a coherent picture. This volume provides a clear introduction and valuable reference for students and researchers in astronomy, cosmochemistry, laboratory astrophysics, and planetary sciences.

The first comprehensive overview of planet formation, this book is a clear introduction and valuable reference for students and researchers in astronomy, cosmochemistry, laboratory astrophysics and planetary sciences. Following the evolution of solids, astronomers, cosmochemists and laboratory astrophysicists jointly discuss the latest insights.

Recenzijas

'Protoplanetary Dust is a terrific edition (No. 12) to the Cambridge Planetary Science Series. This book should be required reading for all cosmochemists (and astronomers), and it would serve as a excellent text for an interesting graduate course on the origin of solar systems.' Geochemical News ' an excellent read, very much at the research edge in the field, and very up to date in the sources used. I would recommend it highly to graduate students, but also for the bookshelves of professionals in the field.' The Observatory ' can be recommended not only to planetary scientists working in the field of planet formation but also to students who seek an introduction to this enormously challenging topic. The organization of the contents makes it possible to concentrate on certain aspects, as few people will be experts in all topics. Having the book on your shelf gives you the confidence that the comprehensive overview of the history of solids in our solar system from a simple grain to the beautiful planet we live on is just a move away.' Ruth Ziethe, European Space Research and Technology Centre, European Space Agency

Papildus informācija

The first comprehensive overview of planet formation for students and researchers in astronomy, cosmochemistry, laboratory astrophysics and planetary sciences.
List of contributing authors xi
Preface xv
Acknowledgments xviii
1 Planet formation and protoplanetary dust 1(26)
1.1 Types of extraterrestrial material available
2(4)
1.2 Chronology of planet formation
6(2)
1.3 Protostellar collapse
8(1)
1.4 Structural evolution of protoplanetary disks
9(2)
1.5 Chemical evolution of the gas disks
11(1)
1.6 Laboratory dust analogs
12(1)
1.7 Dust composition in protoplanetary disks
13(1)
1.8 Dust coagulation
14(1)
1.9 Thermal processing of the pre-planetary material
15(2)
1.10 Dispersal of protoplanetary disks
17(1)
1.11 Accretion of planetesimals and rocky planets
18(1)
1.12 Key challenges and perspectives
19(8)
2 The origins of protoplanetary dust and the formation of accretion disks 27(39)
2.1 Dust in the interstellar medium
28(12)
2.2 Presolar grains in primitive Solar System materials
40(12)
2.3 Star formation
52(14)
3 Evolution of protoplanetary disk structures 66(31)
3.1 Some properties of protoplanetary disks
67(3)
3.2 Protoplanetary disk structure and evolution
70(10)
3.3 Particle dynamics
80(5)
3.4 Protoplanetary disk dynamics and dust evolution
85(7)
3.5 Summary
92(5)
4 Chemical and isotopic evolution of the solar nebula and protoplanetary disks 97(31)
4.1 Protoplanetary disks
99(11)
4.2 Chemical constraints from early Solar System materials
110(1)
4.3 Isotopic anomalies and condensation sequence
111(2)
4.4 Oxygen isotopes
113(9)
4.5 Summary
122(6)
5 Laboratory studies of simple dust analogs in astrophysical environments 128(33)
5.1 Dust-analog synthesis
131(5)
5.2 Characterization techniques
136(4)
5.3 Dust processing
140(3)
5.4 Grain-growth studies
143(6)
5.5 Grain-catalysis studies
149(6)
5.6 Conclusion
155(6)
6 Dust composition in protoplanetary disks 161(30)
6.1 Modeling the dust composition
162(2)
6.2 Laboratory studies of Solar System dust
164(2)
6.3 Dust composition in Solar System samples
166(4)
6.4 Remote sensing of dust around young stars and in comets
170(7)
6.5 Composition of the dust
177(8)
6.6 Processing history of grains as derived from the dust composition
185(6)
7 Dust particle size evolution 191(39)
7.1 Dust coagulation in the Solar System and in extrasolar protoplanetary disks
192(1)
7.2 Nomenclature and definitions
193(3)
7.3 Coagulation basics
196(1)
7.4 Laboratory simulations of dust coagulation
197(1)
7.5 Observational tracers of grain coagulation
198(8)
7.6 Chondritic meteorites
206(8)
7.7 What do chondrite matrices tell us about the grain size of nebular dust?
214(3)
7.8 Dust coagulation: how and when?
217(2)
7.9 Constraints on dust coagulation from amorphous silicates
219(2)
7.10 When did dust coagulation occur?
221(2)
7.11 Astronomical versus meteoritic constraints
223(7)
8 Thermal processing in protoplanetary nebulae 230(33)
8.1 Thermal processing: annealing and evaporation
231(3)
8.2 Observations of thermal processing in protoplanetary disks
234(7)
8.3 Thermal processing in the Solar System: chondrites
241(9)
8.4 Heating mechanisms
250(6)
8.5 How would Solar System formation look to an outside observer
256(1)
8.6 Promising future experiments
257(6)
9 The clearing of protoplanetary disks and of the proto-solar nebula 263(36)
9.1 The observed lifetime of protoplanetary disks
263(11)
9.2 Disk dispersal processes
274(3)
9.3 Our Solar System
277(11)
9.4 Discussion
288(11)
10 Accretion of planetesimals and the formation of rocky planets 299(37)
10.1 Observational constraints on rocky-planet formation
300(4)
10.2 Planetesimal formation
304(8)
10.3 Growth of rocky planets
312(9)
10.4 The effect of the giant planets and the formation of the Asteroid Belt
321(7)
10.5 Summary
328(8)
Appendix 1 Common minerals in the Solar System 336(4)
Appendix 2 Mass spectrometry 340(3)
Appendix 3 Basics of light absorption and scattering theory 343(6)
Glossary 349(14)
Index 363
Dįniel Apai is an Assistant Astronomer at the Space Telescope Science Institute. His research focuses on the observational characterization of the origins and properties of extrasolar planets and planetary systems. Dante Lauretta is an Associate Professor of Planetary Science and Cosmochemistry at the University of Arizona's Lunar and Planetary Laboratory. His research interests include the chemistry and mineralogy of asteroids and comets as determined by in situ laboratory analysis and spacecraft observations.