论文标题
Titius-Bode关系的可靠性及其对搜索系外行星的影响
The reliability of the Titius-Bode relation and its implications for the search for exoplanets
论文作者
论文摘要
我们太阳系中行星的主要半疗法服从了一个简单的几何进程，称为Titius-Bode关系（TBR），其物理起源仍然存在争议。已经表明，系外行驶系统遵循A_N = A_0 E^（Bn）形式的相似（但不是相同）的进程，其中A_0，B是每个系统的常数。自从其制定以来，Titius-Bode的关系已被证明在我们的太阳系中具有很高的预测性。使用来自27个具有5个或更多行星的系术系统的数据并应用提出的方法，我们得出结论，对于具有至少4个行星的系统，可以获得可靠的TB样拟合，并且TBR的精度为78％。通过统计测试，我们表明，实际系外行星系统中行星的周期与随机分布不一致。相反，他们表明其配置是由它们相互相互作用塑造的。
The major semiaxes of the planets in our Solar System obey a simple geometric progression known as the Titius-Bode Relation (TBR), whose physical origin remains disputed. It has been shown that the exoplanetary systems follow a similar (but not identical) progression of the form a_n= a_0 e^(bn), where a_0, b are constants to be determined for each system. Since its formulation, the Titius-Bode Relation has proved to be highly predictive in our Solar System. Using data from 27 exoplanetary systems with 5 or more planets and applying a proposed method, we conclude that reliable TB-like fits can be obtained for systems with at least 4 planets and that the precision of the TBR is 78%. By means of a statistical test we show that the periods of planets in real exoplanetary systems are not consistent with a random distribution. Rather, they show signs that their configuration is shaped by their mutual interactions.
