Book contents
- Chondrules
- Cambridge Planetary Science
- Chondrules
- Copyright page
- Contents
- Contributors
- 1 Introduction
- Part I Observations of Chondrules
- Part II Possible Chondrule-Forming Mechanisms
- 13 Formation of Chondrules by Planetesimal Collisions
- 14 Making Chondrules by Splashing Molten Planetesimals
- 15 Formation of Chondrules by Shock Waves
- 16 Evaluating Non-Shock, Non-Collisional Models for Chondrule Formation
- 17 Summary of Key Outcomes
- Index
- Plate Section (PDF Only)
- References
17 - Summary of Key Outcomes
from Part II - Possible Chondrule-Forming Mechanisms
Published online by Cambridge University Press: 30 June 2018
Book contents
- Chondrules
- Cambridge Planetary Science
- Chondrules
- Copyright page
- Contents
- Contributors
- 1 Introduction
- Part I Observations of Chondrules
- Part II Possible Chondrule-Forming Mechanisms
- 13 Formation of Chondrules by Planetesimal Collisions
- 14 Making Chondrules by Splashing Molten Planetesimals
- 15 Formation of Chondrules by Shock Waves
- 16 Evaluating Non-Shock, Non-Collisional Models for Chondrule Formation
- 17 Summary of Key Outcomes
- Index
- Plate Section (PDF Only)
- References
Summary
Here we review the conclusions from the book chapters and outline some ideas for directions of future research. We discuss what we know and do not know about chondrule precursors, the chronology of chondrule formation, physical (temperature, dust/gas ratio, total pressure) and chemical conditions (fO2, partial pressure of Na, S, SiO, …) in chondrule-forming regions during chondrule formation, chondrule thermal histories, and chondrule formation models.
- Type
- Chapter
- Information
- ChondrulesRecords of Protoplanetary Disk Processes, pp. 428 - 436Publisher: Cambridge University PressPrint publication year: 2018
References
Asphaug, E., Jutzi, M., and Movshovitz, M. (2011). Chondrule formation during planetesimal accretion. Earth and Planetary Science Letters, 308, 369–379.CrossRefGoogle Scholar
Boley, A. C., Morris, M. A., and Desch, S. J. (2013). High-temperature processing of solids through solar nebular bow shocks: 3D radiation hydrodynamics simulations with particles. Astrophysical Journal, 776, 101‒124.CrossRefGoogle Scholar
Bollard, J., Connelly, J., and Bizzarro, M. (2015). Pb-Pb dating of individual chondrules from the CBa chondrite Gujba: Assessment of the impact plume formation model. Meteoritics and Planetary Science, 50, 1197‒1216.CrossRefGoogle ScholarPubMed
Connolly, H. C. Jr., and Desch, S. J. (2004). On the origin of the “Kleine Kügelchen” Called chondrules. Chemie der Erde-Geochemistry, 64, 95‒125.CrossRefGoogle Scholar
Hewins, R., Jones, R. H., and Scott, E. R. D. (Eds.). (1996). Chondrules and the Protoplanetary Disk. Cambridge, UK: Cambridge University Press.Google Scholar
Johnson, B. C., Minton, D. A., Melosh, H. J., and Zuber, M. T. (2015). Impact jetting as the origin of chondrules. Nature, 517, 339–341.CrossRefGoogle ScholarPubMed
Kargel, J. S., Fegley, B. Jr., and Schaefer, L. (2003). Ceramic volcanism on refractory worlds: The cases of Io and chondrite CAIs. Lunar and Planetary Science Conference XXXIV, abstract #1964.Google Scholar
Krot, A. N., Amelin, Y., Cassen, P., and Meibom, A. (2005). Young chondrules in CB chondrites from a giant impact in the early Solar System. Nature, 436, 989–92.CrossRefGoogle Scholar
Walsh, K. J., Morbidelli, A., Raymond, S. N., O’Brian, P., and Mandell, A. M. (2011). A low mass for Mars from Jupiter’s gas-driven migration. Nature, 475, 206–209.CrossRefGoogle ScholarPubMed
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