Prediction of observable quantities tracing the process of planetesimal formation

追踪小行星形成过程的可观测量的预测

• 批准号: 35121508
• 负责人: Professor Dr. Sebastian Wolf
• 金额: --
• 依托单位: Institut für Theoretische Physik und Astrophysik
• 依托单位国家: 德国
• 项目类别: Research Units
• 财政年份: 2006
• 资助国家: 德国
• 起止时间: 2005-12-31 至 2011-12-31
• 项目状态: 已结题
• 来源: https://gepris.dfg.de/gepris/projekt/35121508?language=en
• 关键词: Prediction; observable; quantities; tracing; process

This project aims at connecting the theoretical predictions for planetesimal formation and evolution processes derived in the various projects of the Forschergruppe with existing observations. Moreover, predictions for future observations will be investigated providing powerful tools to verify the results of the Forschergruppe. In the new funding phase, the project is split in three parts. In part one we will continue to investigate the observability of specific processes tracing the formation of planetesimals on the basis of the new results provided by the other teams of the Forschergruppe. We will also provide instantaneous feedback to these teams concerning the feasibility to verify their predictions (primarily projects A1, A4, C1, C2, C3), allowing them to optimize the strategy of their investigations. In the second part we will use the new constraints for disk and planetesimal formation for the analysis of specific observations. The third, minor part will be to perform new observations of circumstellar disks at the potential stage of planetesimal formation.

该项目旨在将研究小组的各种项目中得出的关于星子形成和演化过程的理论预测与现有观测相联系。此外，对未来观测的预测将进行调查，提供强大的工具来验证研究小组的结果。在新的筹资阶段，该项目分为三个部分。在第一部分中，我们将继续调查的可观测性的跟踪星子的形成的基础上，由其他研究小组提供的新结果的具体过程。我们还将向这些团队提供关于验证其预测（主要是项目A1，A4，C1，C2，C3）的可行性的即时反馈，使他们能够优化其调查策略。在第二部分中，我们将使用新的限制盘和星子形成的具体观测的分析。第三，次要的部分将是在星子形成的潜在阶段对星周盘进行新的观测。