第76章 对火星轨道变化问题的最后解释（1/12）
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：
ong-termintegrationsandstabilityoflaaryorbitsinourolarsystem
bstract
eresenttheresultsofverylong-termnumericalintegrationsoflaaryorbitalmotionsover109-yrtime-sansincludingallninelas.quickinsectionofournumericaldatashosthatthelaarymotion，atleastinoursimledynamicalmodel，seemstobequitestableevenoverthisverylongtime-san.closerlookattheloest-frequencyoscillationsusingalo-assfiltershosustheotentiallydiffusivecharacterofterrestriallaarymotion，eseciallythatofercury.hebehaviouroftheeentricityofercuryinourintegrationsisqualitativelysimilartotheresultsfromacquesaskar'ssecularerturbationtheory(e.g.emax～0.35over～±4yr).oever，therearenoaarentsecularincreasesofeentricityorinclinationinanyorbitalelementsofthelas，hichmayberevealedbystilllonger-termnumericalintegrations.ehavealsoerformedacouleoftrialintegrationsincludingmotionsoftheouterfivelasoverthedurationof±51010yr.heresultindicatesthatthethreemajorresonancesintheetune–lutosystemhavebeenmaintainedoverthe1011-yrtime-san.
1ntroduction
1.1efinitionoftheroblem
hequestionofthestabilityofourolarsystemhasbeendebatedoverseveralhundredyears，sincetheeraofeton.heroblemhasattractedmanyfamousmathematiciansovertheyearsandhaslayedacentralroleinthedevelomentofnon-lineardynamicsandchaostheory.oever，edonotyethaveadefiniteansertothequestionofhetherourolarsystemisstableornot.hisisartlyaresultofthefactthatthedefinitionoftheterm‘stability’isvaguehenitisusedinrelationtotheroblemoflaarymotionintheolarsystem.ctuallyitisnoteasytogiveaclear，rigorou
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