…larger mass [1]. This means e.g. a typical binary star system would not have stable L4/L5 points. The reference [1] works through this in careful detail and is an excellent reference on this topic. [1] Solar System Dynamics, Murray and Dermott, Cambridge University Press.
…elucidate exoplanet systems. There are plenty of systems discovered by Kepler, CoRoT etc. that require a deep, fundamental understanding of the processes that shape(d) them. [1] http://www.amazon.com/Solar-System-Dynamics-Carl-Murray/dp/0...
……更大的质量 [1]。这意味着，比如一个典型的双星系统就不会有稳定的 L4/L5 点。参考文献 [1] 对此进行了严谨详尽的推导，是该领域极佳的参考资料。[1] 《Solar System Dynamics》，Murray 和 Dermott 著，剑桥大学出版社。
…larger mass [1]. This means e.g. a typical binary star system would not have stable L4/L5 points. The reference [1] works through this in careful detail and is an excellent reference on this topic. [1] Solar System Dynamics, Murray and Dermott, Cambridge University Press.
……阐明系外行星系统。Kepler、CoRoT 等发现了大量系统，需要对其形成演化过程有深入、根本性的理解。[1] http://www.amazon.com/Solar-System-Dynamics-Carl-Murray/dp/0...
…elucidate exoplanet systems. There are plenty of systems discovered by Kepler, CoRoT etc. that require a deep, fundamental understanding of the processes that shape(d) them. [1] http://www.amazon.com/Solar-System-Dynamics-Carl-Murray/dp/0...