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Titan After Cassini-Huygens.
- Format:
- Book
- Author/Creator:
- Lopes, Rosaly M.C.
- Language:
- English
- Subjects (All):
- Titan (Satellite).
- Physical Description:
- 1 online resource
- Place of Publication:
- Amsterdam, Netherlands ; Cambridge, MA : Elsevier, 2025.
- Contents:
- Intro
- Titan After Cassini-Huygens
- Copyright
- Contents
- Contributors
- Chapter 1: Introduction: Titan, the Earth of the outer solar system
- 1. Introduction
- 2. Book structure
- 3. Titan's bulk properties
- 4. Titan's regions and nomenclature
- Acknowledgments
- Chapter 2: History of Titan exploration
- 1. Prologue
- 2. The initial steps
- 3. Joint ESA-NASA study
- 4. Mission overview
- 5. Launch
- 6. Cruise
- 7. Saturn orbit insertion (SOI)
- 8. Beginning the tour: Cassini's Prime Mission
- 9. Huygens probe mission
- 10. Titan and satellite tour
- 11. Viewing Saturn's rings edge-on: Equinox Mission (EM)
- 12. Summer in the northern hemisphere: SM
- 13. Satisfying planetary protection requirements: Grand finale orbits
- 14. Epilogue
- Appendix
- References
- Chapter 3: The origin and evolution of Titan
- 1. Introduction: Key issues in the origin and evolution of Titan
- 2. Cassini-Huygens and other data sets relevant to origin and evolution
- 2.1. Atmospheric composition: Molecular and isotopic
- 2.2. Surface properties
- 3. Models of the growth of satellites around Saturn
- 3.1. Context: Growth of Saturn
- 3.2. Titan's accretion in the Saturn environment
- 4. Earliest evolution of Titan
- 4.1. Evolution of a primitive ammonia-water ``magma ́́ocean and crust formation
- 4.2. Interior differentiation and water-organics-rock interactions
- 4.3. Conversion of NH3 to N2 by various mechanisms
- 5. Coupled evolution of the interior and atmosphere of Titan up to the last billion years
- 5.1. Evolution of Titan's internal ocean and link with its orbit
- 5.2. Isotopic constraints on the atmosphere evolution
- 6. The last billion years
- 6.1. Evidence for and against a standing global methane-ethane ocean in the past
- 6.2. The resupply of methane over the last billion years: Steady state or episodic?
- 7. What we seek to learn from Dragonfly and future missions about the origin and evolution of Titan
- Chapter 4: Titan orbital and rotational dynamics
- 2. Observations and dynamical characteristics
- 3. Short-term evolution
- 3.1. The orbital motion
- 3.2. Titan's rotation
- 4. Long-term evolution
- 4.1. Evolution and origin of the Titan-Hyperion resonance
- 4.2. Past resonance crossings with Iapetus
- 4.3. Migration of Titan and the evolution of Saturn's obliquity
- 5. Conclusion
- Chapter 5: Titan's magnetic and plasma environment
- 2. Titan internal field and upper atmosphere/exosphere/ionosphere
- 2.1. Internal magnetic field
- 2.2. Titan's atmosphere, ionosphere, and exosphere
- 3. Upstream from Titan
- 4. Induced magnetosphere through specific cases
- 5. General trends
- 6. Ion pickup and escape
- 7. Numerical simulations
- 8. Conclusions and outstanding questions
- Notes:
- Electronic reproduction. Ann Arbor, MI Available via World Wide Web.
- ISBN:
- 9780323991629
- 0323991629
- Publisher Number:
- 40032664593
- Access Restriction:
- Restricted for use by site license.
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