第76章 对火星轨道变化问题的最后解释（1/1）

第76章 对火星轨道变化问题的最后解释

作者君在作品相关中已经解释过这个问题，并在此列出相关参考文献中的一篇开源论文。

以下是文章内容：

long-terentricity of entricity or inclination in any orbital eleurs sourrence of any orbital crossing between either of a pair of planets takes place. this is because we know frourate seentricities and inclinations of the terrestrial planets， especially of ess )， where we show raw orbital eleuurate enough， which partly justifies our entricity of jupiter (0.05) is ording to one of the basic properties of syuracy of nuuracy than the urate integration with a stepsize of 0.125 d (1/64 of the entricities and orbital inclinations for the inner four planets in the initial and final part of the integration n+1 is shown in fig. 4. as expected， the character of the variation of planetary orbital eleentricity， seeentricities and inclinations of entricity and inclination of earth in n+2 integration. in fig. 5， the dark area shows that at the tientricity and inclination of earth only changes slightly over the entire period covered by the n+2 integration. this nearly regular trend is qualitatively the saaletti &ao 1998). this entricities of venus and earth can be disturbed easily by jupiter and saturn， which results in a positive correlation in the angular entricities and inclinations (fig. 13) show this very long-terentricity and inclination of pluto are synchronized with the libration of its arguentricity becoentricity becoentricity of jupiter)， since the disturbance caused by jovian planets is a forced oscillation having an aentricity， for example o(ej)0.05， is far from sufficient to provoke instability in the terrestrial planets having such a wide separation as 26rh. thus we assume that the present wide dynamical separation among terrestrial planets (> 26rh) is probably one of the most significant conditions for maintaining the stability of the planetary system over a 109-yr time-span. our detailed analysis of the relationship between dynamical distance between planets and the instability time-scale of solar system planetary motion is now on-going.

although our numerical integrations span the lifetime of the solar system， the number of integrations is far from sufficient to fill the initial phase space. it is necessary to perform more and more numerical integrations to confirm and examine in detail the long-term stability of our planetary dynamics.

——以上文段引自 ito， t.& tanikawa， k. long-term integrations and stability of planetary orbits in our solar system. mon. not. r. astron. soc. 336， 483–500 (2002)

这只是作者君参考的一篇文章，关于太阳系的稳定性。

还有其他论文，不过也都是英文的，相关课题的中文文献很少，那些论文下载一篇要九美元（《nature》真是暴利），作者君写这篇文章的时候已经回家，不在检测中心，所以没有数据库的使用权，下不起，就不贴上来了。

(本章完)