Protoplanetary Dust

Protoplanetary Dust PDF

Author: Dániel Apai

Publisher: Cambridge University Press

Published: 2010-01-21

Total Pages: 397

ISBN-13: 0521517729

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The first comprehensive overview of planet formation for students and researchers in astronomy, cosmochemistry, laboratory astrophysics and planetary sciences.

Astrophysics of Planet Formation

Astrophysics of Planet Formation PDF

Author: Philip J. Armitage

Publisher: Cambridge University Press

Published: 2020-01-30

Total Pages: 345

ISBN-13: 1108420508

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A self-contained graduate-level introduction to the physical processes that shape planetary systems, covering all stages of planet formation.

Dust-Gas Instabilities in Protoplanetary Disks

Dust-Gas Instabilities in Protoplanetary Disks PDF

Author: Ryosuke Tominaga

Publisher: Springer Nature

Published: 2022-04-25

Total Pages: 125

ISBN-13: 9811917655

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How planets form is one of the long-standing questions in astrophysics. In particular, formation scenarios of planetesimals which are kilometer-sized bodies and a precursor of planets are still unclear and under debate although some promising mechanisms have been proposed. This book highlight disk instabilities that have the potential to explain the origin of planetesimals. Using linear analyses and numerical simulations, it addresses how a disk evolves through the development of instabilities, and also presents a new instability driven by dust coagulation. As a result, the simulation demonstrates a scenario of planetesimal formation: A successive development of multiple instabilities triggers planetesimal formation in resulting dusty rings.

Protoplanetary Dust

Protoplanetary Dust PDF

Author: Dàniel Apai

Publisher:

Published: 2014-05-14

Total Pages: 397

ISBN-13: 9780511675409

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The first comprehensive overview of planet formation for students and researchers in astronomy, cosmochemistry, laboratory astrophysics and planetary sciences.

Formation, Evolution, and Dynamics of Young Solar Systems

Formation, Evolution, and Dynamics of Young Solar Systems PDF

Author: Martin Pessah

Publisher: Springer

Published: 2017-12-04

Total Pages: 374

ISBN-13: 3319606093

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This book's interdisciplinary scope aims at bridging various communities: 1) cosmochemists, who study meteoritic samples from our own solar system, 2) (sub-) millimetre astronomers, who measure the distribution of dust and gas of star-forming regions and planet-forming discs, 3) disc modellers, who describe the complex photo-chemical structure of parametric discs to fit these to observation, 4) computational astrophysicists, who attempt to decipher the dynamical structure of magnetised gaseous discs, and the effects the resulting internal structure has on the aerodynamic re-distribution of embedded solids, 5) theoreticians in planet formation theory, who aim to piece it all together eventually arriving at a coherent holistic picture of the architectures of planetary systems discovered by 6) the exoplanet observers, who provide us with unprecedented samples of exoplanet worlds. Combining these diverse fields the book sheds light onto the riddles that research on planet formation is currently confronted with, and paves the way for a comprehensive understanding of the formation, evolution, and dynamics of young solar systems. The chapters ‘Chondrules – Ubiquitous Chondritic Solids Tracking the Evolution of the Solar Protoplanetary Disk’, ‘Dust Coagulation with Porosity Evolution’ and ‘The Emerging Paradigm of Pebble Accretion’ are published open access under a CC BY 4.0 license via link.springer.com.

Protostars and Planets VI

Protostars and Planets VI PDF

Author: Henrik Beuther

Publisher: University of Arizona Press

Published: 2014-12-18

Total Pages: 945

ISBN-13: 0816531242

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Proceedings of a conference held in Heidelberg, Germany, July 15-20, 2013.

From Protoplanetary Disks to Planet Formation

From Protoplanetary Disks to Planet Formation PDF

Author: Philip J. Armitage

Publisher: Springer

Published: 2019-02-02

Total Pages: 260

ISBN-13: 3662586878

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Is the Sun and its planetary system special? How did the Solar system form? Are there similar systems in the Galaxy? How common are habitable planets? What processes take place in the early life of stars and in their surrounding circumstellar disks that could impact whether life emerges or not? This book is based on the lectures by Philip Armitage and Wilhelm Kley presented at 45th Saas-Fee Advanced Course „From Protoplanetary Disks to Planet Formation“ of the Swiss Society for Astrophysics and Astronomy. The first part deals with the physical processes occurring in proto-planetary disks starting with the observational context, structure and evolution of the proto-planetary disk, turbulence and accretion, particle evolution and structure formation. The second part covers planet formation and disk-planet interactions. This includes in detail dust and planetesimal formation, growth to protoplanets, terrestrial planet formation, giant planet formation, migration of planets, multi-planet systems and circumbinary planets. As Saas-Fee advanced course this book offers PhD students an in-depth treatment of the topic enabling them to enter on a research project in the field.

Protostars and Planets V

Protostars and Planets V PDF

Author: Bo Reipurth

Publisher: University of Arizona Press

Published: 2007

Total Pages: 994

ISBN-13: 9780816526543

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'Protostars and Planets V' builds on the latest results from recent advances in ground and space-based astronomy and in numerical computing techniques to offer the most detailed and up-to-date picture of star and planet formation - including the formation and early evolution of our own solar system.

From Dust To Stars

From Dust To Stars PDF

Author: Norbert S. Schulz

Publisher: Springer Science & Business Media

Published: 2007-03-06

Total Pages: 409

ISBN-13: 3540273212

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Studies of stellar formation in galaxies have a profound impact on our understanding of the present and the early universe. The book describes complex physical processes involved in the creation of stars and during their young lives. It illustrates how these processes reveal themselves from radio wavelengths to high energy X-rays and gamma -rays, with special reference towards high energy signatures. Several sections devoted to key analysis techniques demonstrate how modern research in this field is pursued.