论文标题
黄道中KBO的轨道聚类是否可以是由于太阳环形场产生的时空拖动引起的？
Can Orbital Clustering of KBOs in the Ecliptic be due to the Solar Toroidal Field Generated Spacetime Dragging?
论文作者
论文摘要
Kuiper带对象（KBOS）显示出大于海王星大的围栏距离的外行星的轨道聚类，而距离天气大于150 au的半轴轴。这意味着迄今一种未知的动力学机制来抵消由巨型太阳系行星引起的轨道元素的随机化。使用环形场诱导的框架拖拉，我们在这里推断出观察到的Kuiper带区域的范围，Kuiper带中的Sedna的半大轴轴，以及Ecliptic中KBO的轨道聚类，而无需假设由跨烟 - 摩托车（TNOS）（tnos）（TNOS）（TNOS）（tnos）（tnos）的动力学效应）。我们还计算了内行星的轨道进动率，并在观测准确性的范围内显示了它们的对应关系，与最近的行星胚层。
The Kuiper belt objects (KBOs) exhibit an orbital clustering of the outer planets lying at perihelion distances larger than Neptune and semimajor axes greater than 150 AU from the Sun. This implies a hitherto unknown dynamical mechanism to counter randomizing of the orbital elements caused by the giant solar system planets. Using the toroidal field induced frame-dragging we deduce here the observed range of the Kuiper belt region, the semi-major axis of Sedna like objects in the Kuiper belt, as well as the orbital clustering of the KBOs in the ecliptic, without assuming dynamical effects induced by trans-Neptunian-objects (TNOs). We also calculate the orbital precession rates for the inner planets and show their correspondence, within the range of observational accuracy, with recent planetary ephemerides.
