论文标题
天王星，木星，海王星和土星的原始圆盘中的温度分布以及其卫星系统中的共同结构
Temperature Distributions in the Protosatellite Disks of Uranus, Jupiter, Neptune and Saturn and Common Structure in Their Satellite Systems
论文作者
论文摘要
我们在天王星，木星和海王星的卫星和环系统的轨道半径中观察到相似的结构。这刺激了一项研究，即这些系统的演变和土星系统的发展是由涉及辐射与其亚元音（原始片磁盘）相互作用的共同机制引发的。提出了一个模型，其特征是通过刺激的辐射分子缔合（SRMA）反应产生共振。在此模型中，在远离原球星的特定距离的磁盘与磁盘的局部热能与磁盘上撞击光子的能量之间有匹配的地方，从原行星磁盘上提取热能。辐射是由Uranian，Jovian和Neptunian磁盘的一部分氢分子光谱以及Saturnian磁盘的一部分氢原子光谱提供的。发现阐明了卫星系统的早期演化和结构，包括复杂的土星环系。它们还将卫星轨道半径分布与原始磁盘中的温度分布（TD）形状联系起来。在天王星原始磁盘（Mousis 2004）和土星（Mousis Gautier和Bockelee-Moran，2002年）中，理论上确定的TD在本研究中至关重要。
We observe similar structures in the orbital radii of satellite and ring systems of Uranus, Jupiter and Neptune. This stimulates an investigation that the evolution of these systems and Saturn's system is initiated by a common mechanism that involves the interaction of radiation with their subnebulae (protosatellite disks). A model is presented that is characterized by resonance created through stimulated radiative molecular association (SRMA) reactions. In this model thermal energy is extracted from a protoplanetary disk at specific distances from the protoplanet wherever there is a match between the local thermal energy of the disk and the energy of photons impinging on the disk. Radiation is supplied by a portion of the hydrogen molecule's spectrum for the Uranian, Jovian and Neptunian disks and a portion of the hydrogen atom's spectrum for the Saturnian disk. Findings shed light on the early evolution and structure of satellite systems including the complicated ring system of Saturn. They also link satellite orbital radii size distributions to shapes of temperature distributions (TD's) in protosatellite disks. Theoretically determined TD's in the protosatellite disks of Uranus (Mousis 2004) and Saturn (Mousis Gautier and Bockelee-Moran, 2002) are essential to the present investigation.
