Rufu Raluca, Canup Robin M
Department of Earth and Planetary Sciences, Weizmann Institute of Science, Rehovot 76100, Israel.
Southwest Research Institute, Boulder, Colorado 80302, USA.
Astron J. 2017 Nov;154(5). doi: 10.3847/1538-3881/aa9184. Epub 2017 Nov 6.
The Neptunian satellite system is unusual. The major satellites of Jupiter, Saturn and Uranus are all in prograde, low inclination orbits. Neptune on the other hand, has the fewest satellites and most of the system's mass is within one irregular satellite, Triton. Triton was most likely captured by Neptune and destroyed the primordial regular satellite system. We investigate the interactions between a newly captured Triton and a prior Neptunian satellite system. We find that a prior satellite system with a mass ratio similar to the Uranian system or smaller has a substantial likelihood of reproducing the current Neptunian system, while a more massive system has a low probability of leading to the current configuration. Moreover, Triton's interaction with a prior satellite system may offer a mechanism to decrease its high initial semimajor axis fast enough to preserve small irregular satellites (Nereid-like), that might otherwise be lost during a prolonged Triton circularization via tides alone.
海王星的卫星系统与众不同。木星、土星和天王星的主要卫星都处于顺行、低倾角轨道。另一方面,海王星的卫星最少,且该系统的大部分质量集中在一颗不规则卫星——海卫一上。海卫一很可能是被海王星捕获的,并且破坏了原始的规则卫星系统。我们研究了新捕获的海卫一与之前的海王星卫星系统之间的相互作用。我们发现,质量比与天王星系统相似或更小的先前卫星系统,有很大可能性重现当前的海王星系统,而质量更大的系统则不太可能形成当前的构型。此外,海卫一与先前卫星系统的相互作用可能提供一种机制,使其能够足够快地减小其较高的初始半长轴,从而保留那些可能仅通过潮汐作用在海卫一长期圆化过程中丢失的小不规则卫星(类似海卫二)。