Planetary astrophysics:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Buch |
| Sprache: | English |
| Veröffentlicht: |
Newcastle upon Tyne
Cambridge Scholars Publishing
2023
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| Schlagworte: | |
| Online-Zugang: | Inhaltsverzeichnis |
| Beschreibung: | ix, 270 Seiten Diagramme |
| ISBN: | 9781527501188 |
Internformat
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| 100 | 1 | |a Marzari, Francesco |e Verfasser |4 aut | |
| 245 | 1 | 0 | |a Planetary astrophysics |c by Francesco Marzari |
| 264 | 1 | |a Newcastle upon Tyne |b Cambridge Scholars Publishing |c 2023 | |
| 300 | |a ix, 270 Seiten |b Diagramme | ||
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Datensatz im Suchindex
| _version_ | 1805074772683390976 |
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Table of Contents Preface. x 1. The solar system. 1 1.1 The context 1.2 Solar System population 1.3 The standard model of planet formation 1.4 Circumstellar disks, the cradles of planets 1.5 Pebble and planetesimal formation 1.6 Planetesimal accumulation 1.7 Pebble accretion 1.8 Gas infall onto giant planet cores 1.9 Structure of the giant planets 1.10 The icy planets 2. Exoplanets. 19 2.1 The context 2.2 Detection methods 2.3 The Rossiter-McLaughlin effect 2.4 Orbital and mass distributions of known exoplanets 2.5 Hot/warm Jupiters 2.6 Solar system analogs 2.7 Earths, Super-Earths and Neptune-size planets 2.8 Debris disks 2.9 Dynamics of exoplanets: migration and P-P scattering 2.10 Planet migration driven by the interaction with the protoplanetary disk 2.11 Planet-Planet scattering and the eccentricity excitation 2.12 Population synthesis models
vi Table of Contents 3. The magnetic field of planets. 40 3.1 The context 3.2 Earth's magnetic field (IGRF) 3.3 Source of Earth’s magnetic field 3.4 Planetary rotation and magnetic field 3.5 Magnetic field reversal 3.6 Dipolar approximation 3.7 Motion of charged particles in a dipolar magnetic field 3.8 The gyration motion 3.9 The drift motion 3.10 The mirror motion 3.11 Van Allen Belts 3.12 The magnetosphere of the Earth 3.13 Northern lights (aurora borealis) 4. The sun and the solar wind. 64 4.1 The context 4.2 Physical properties of the sun 4.3 The solar wind 4.4 Relation between the solar wind and the interplanetary magnetic field 4.5 Planetary migration due to magnetic interaction 5. Non-gravitational forces in planetary systems. 73 5.1 The context 5.2 Dust particles 5.3 Radiation pressure and Poynting-Robertson drag 5.4 Relativistic derivation of the Poynting-Robertson drag force 5.5 Effects of radiation pressure on the orbit of dust particles 5.6 Effects of Poynting-Robertson drag on the dynamics of dust particles 5.7 Yarkovsky effect 5.8 Relevance of the Yarkovsky effect in the asteroid belt 5.9 Gas drag 5.10 Epstein drag law 5.11 Dust traps at pressure bumps 5.12 Stokes drag law
Planetary Astrophysics vii 6. Tidal forces and spin-orbit resonances. 100 6.1 The context 6.2 Formation of a tidal bulge 6.3 A simplified one-dimensional model for the tidal shift 6.4 The tidal dissipation function Q 6.5 The Earth-Moon system 6.6 Tidal coupling and dynamical evolution: tide on the planet 6.7 Tidal coupling and dynamical evolution: tide on the satellite 6.8 Tidal interaction of planets with their star 6.9 Evolution of a satellite spin 6.10 Spin-orbit resonances 6.11 The Hamiltonian approach 6.12 Resonance overlapping and chaos: the Chirikov criterion 7. The three body problem. 133 7.1 The context 7.2 Hill’s equations and zero velocity curves 7.3 The Jacoby constant, alias the Hamiltonian 7.4 The Lagrangian equilibrium points 7.5 Trojan asteroids 7.6 Trojan capture mechanisms 7.7 Hill’s sphere 7.8 The Tisserand invariant 8. Orbiting around an irregular body. 149 8.1 The context 8.2 Gravity field of an irregular body 8.3 Flattening of a planet due to rotation 8.4 Variations of the orbital elements of a satellite due to the J2 perturbations 9. Secular theories for multi-planet systems. 162 9.1 The context 9.2 The disturbing function 9.3 The Laplace-Lagrange secular theory 9.4 The Laplace-Lagrange theory for small bodies 9.5 The Lidov-Kozai secular theory 9.6 Secular theories for planets in binaries
viii Table of Contents 10. Mean motion resonances. . 186 10.1 The context 10.2 The Hamiltonian of the planar restricted 3-body problem 10.3 The pendulum model for first order resonances 10.4 Resonance superposition and chaotic evolution 10.5 Resonances between two planets 11. Modeling circumstellar disks. 197 11.1 The context 11.2 Basics of fluid dynamics 11.3 Fluid dynamics applications: the shape of the nozzle 11.4 Fluid dynamics applications: Parker’s solution for the solar wind 11.5 Circumstellar disks 11.6 Viscous mass accretion rate on the star 11.7 Photoevaporation Appendices. 224 Appe ndix A: Orbital elements. 225 A.l : The Hohmann transfer A.2: Transformation from r, v to a, e, Μ and viceversa A.3: The orbit in 3D A.4: Angular momentum and energy in the barycentric reference frame Appe ndix B: Computation of the field lines of a vector field in 2D. 237 Appen dix C: Absorption and emission of light.238 Appen dix D: Special relativity concepts. 240 D.l: Four-vectors D.2: Lorentz transformations D.3: The relativistic Doppler effect Appen dix E: Canonical transformations. 246 Appendix F: Recursive Rodriguez’s formula for computing Legendre’s
polynomials. 249 Appendix G: The planetary Lagrange equations. 250
Planetary Astrophysics ix Appendix H: Method to derive the Laplace-Lagrange planetary equations for the non-singular variables. 255 Appendix I: The Hamiltonian of the two body problem. 257 Appendix J: Sound waves in a fluid. 259 Appendix K: Relativistic formulation of the Euler equations. 262 Appendix L: Ideal MHD (magnetohydrodynamics). 264 L.l: The equations of MHD L.2: The magnetic pressure L.3: Alfven’s theorem and freezing of magnetic field lines in a plasma |
| adam_txt |
Table of Contents Preface. x 1. The solar system. 1 1.1 The context 1.2 Solar System population 1.3 The standard model of planet formation 1.4 Circumstellar disks, the cradles of planets 1.5 Pebble and planetesimal formation 1.6 Planetesimal accumulation 1.7 Pebble accretion 1.8 Gas infall onto giant planet cores 1.9 Structure of the giant planets 1.10 The icy planets 2. Exoplanets. 19 2.1 The context 2.2 Detection methods 2.3 The Rossiter-McLaughlin effect 2.4 Orbital and mass distributions of known exoplanets 2.5 Hot/warm Jupiters 2.6 Solar system analogs 2.7 Earths, Super-Earths and Neptune-size planets 2.8 Debris disks 2.9 Dynamics of exoplanets: migration and P-P scattering 2.10 Planet migration driven by the interaction with the protoplanetary disk 2.11 Planet-Planet scattering and the eccentricity excitation 2.12 Population synthesis models
vi Table of Contents 3. The magnetic field of planets. 40 3.1 The context 3.2 Earth's magnetic field (IGRF) 3.3 Source of Earth’s magnetic field 3.4 Planetary rotation and magnetic field 3.5 Magnetic field reversal 3.6 Dipolar approximation 3.7 Motion of charged particles in a dipolar magnetic field 3.8 The gyration motion 3.9 The drift motion 3.10 The mirror motion 3.11 Van Allen Belts 3.12 The magnetosphere of the Earth 3.13 Northern lights (aurora borealis) 4. The sun and the solar wind. 64 4.1 The context 4.2 Physical properties of the sun 4.3 The solar wind 4.4 Relation between the solar wind and the interplanetary magnetic field 4.5 Planetary migration due to magnetic interaction 5. Non-gravitational forces in planetary systems. 73 5.1 The context 5.2 Dust particles 5.3 Radiation pressure and Poynting-Robertson drag 5.4 Relativistic derivation of the Poynting-Robertson drag force 5.5 Effects of radiation pressure on the orbit of dust particles 5.6 Effects of Poynting-Robertson drag on the dynamics of dust particles 5.7 Yarkovsky effect 5.8 Relevance of the Yarkovsky effect in the asteroid belt 5.9 Gas drag 5.10 Epstein drag law 5.11 Dust traps at pressure bumps 5.12 Stokes drag law
Planetary Astrophysics vii 6. Tidal forces and spin-orbit resonances. 100 6.1 The context 6.2 Formation of a tidal bulge 6.3 A simplified one-dimensional model for the tidal shift 6.4 The tidal dissipation function Q 6.5 The Earth-Moon system 6.6 Tidal coupling and dynamical evolution: tide on the planet 6.7 Tidal coupling and dynamical evolution: tide on the satellite 6.8 Tidal interaction of planets with their star 6.9 Evolution of a satellite spin 6.10 Spin-orbit resonances 6.11 The Hamiltonian approach 6.12 Resonance overlapping and chaos: the Chirikov criterion 7. The three body problem. 133 7.1 The context 7.2 Hill’s equations and zero velocity curves 7.3 The Jacoby constant, alias the Hamiltonian 7.4 The Lagrangian equilibrium points 7.5 Trojan asteroids 7.6 Trojan capture mechanisms 7.7 Hill’s sphere 7.8 The Tisserand invariant 8. Orbiting around an irregular body. 149 8.1 The context 8.2 Gravity field of an irregular body 8.3 Flattening of a planet due to rotation 8.4 Variations of the orbital elements of a satellite due to the J2 perturbations 9. Secular theories for multi-planet systems. 162 9.1 The context 9.2 The disturbing function 9.3 The Laplace-Lagrange secular theory 9.4 The Laplace-Lagrange theory for small bodies 9.5 The Lidov-Kozai secular theory 9.6 Secular theories for planets in binaries
viii Table of Contents 10. Mean motion resonances. . 186 10.1 The context 10.2 The Hamiltonian of the planar restricted 3-body problem 10.3 The pendulum model for first order resonances 10.4 Resonance superposition and chaotic evolution 10.5 Resonances between two planets 11. Modeling circumstellar disks. 197 11.1 The context 11.2 Basics of fluid dynamics 11.3 Fluid dynamics applications: the shape of the nozzle 11.4 Fluid dynamics applications: Parker’s solution for the solar wind 11.5 Circumstellar disks 11.6 Viscous mass accretion rate on the star 11.7 Photoevaporation Appendices. 224 Appe ndix A: Orbital elements. 225 A.l : The Hohmann transfer A.2: Transformation from r, v to a, e, Μ and viceversa A.3: The orbit in 3D A.4: Angular momentum and energy in the barycentric reference frame Appe ndix B: Computation of the field lines of a vector field in 2D. 237 Appen dix C: Absorption and emission of light.238 Appen dix D: Special relativity concepts. 240 D.l: Four-vectors D.2: Lorentz transformations D.3: The relativistic Doppler effect Appen dix E: Canonical transformations. 246 Appendix F: Recursive Rodriguez’s formula for computing Legendre’s
polynomials. 249 Appendix G: The planetary Lagrange equations. 250
Planetary Astrophysics ix Appendix H: Method to derive the Laplace-Lagrange planetary equations for the non-singular variables. 255 Appendix I: The Hamiltonian of the two body problem. 257 Appendix J: Sound waves in a fluid. 259 Appendix K: Relativistic formulation of the Euler equations. 262 Appendix L: Ideal MHD (magnetohydrodynamics). 264 L.l: The equations of MHD L.2: The magnetic pressure L.3: Alfven’s theorem and freezing of magnetic field lines in a plasma |
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| spelling | Marzari, Francesco Verfasser aut Planetary astrophysics by Francesco Marzari Newcastle upon Tyne Cambridge Scholars Publishing 2023 ix, 270 Seiten Diagramme txt rdacontent n rdamedia nc rdacarrier Planetensystem (DE-588)4126386-8 gnd rswk-swf Extrasolarer Planet (DE-588)4456110-6 gnd rswk-swf Planetensystem (DE-588)4126386-8 s Extrasolarer Planet (DE-588)4456110-6 s DE-604 Digitalisierung UB Bayreuth - ADAM Catalogue Enrichment application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=034951257&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis |
| spellingShingle | Marzari, Francesco Planetary astrophysics Planetensystem (DE-588)4126386-8 gnd Extrasolarer Planet (DE-588)4456110-6 gnd |
| subject_GND | (DE-588)4126386-8 (DE-588)4456110-6 |
| title | Planetary astrophysics |
| title_auth | Planetary astrophysics |
| title_exact_search | Planetary astrophysics |
| title_exact_search_txtP | Planetary astrophysics |
| title_full | Planetary astrophysics by Francesco Marzari |
| title_fullStr | Planetary astrophysics by Francesco Marzari |
| title_full_unstemmed | Planetary astrophysics by Francesco Marzari |
| title_short | Planetary astrophysics |
| title_sort | planetary astrophysics |
| topic | Planetensystem (DE-588)4126386-8 gnd Extrasolarer Planet (DE-588)4456110-6 gnd |
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