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-termintegrationsandstabilityofplanetaryorbitsinourSolarsystem
Abstract
Wepresenttheresultsofverylong-termnumericalintegrationsofplanetaryorbitalmotionsover109 -， atleastinoursimpledynamicalmodel， -frequencyoscillationsusingalow-passfiltershowsusthepotentiallydiffusivecharacterofterrestrialplanetarymotion， 'ssecularperturbationtheory (e.g.emax0.35over ± 4Gyr).However， therearenoapparentsecularincreasesofeccentricityorinclinationinanyorbitalelementsoftheplanets， ± 5 × 1010yr.TheresultindicatesthatthethreemajorresonancesintheNeptuneCPlutosystemhavebeenmaintainedoverthe1011-yrtime-span.
1Introduction
1.1Definitionoftheproblem
ThequestionofthestabilityofourSolarsystemhasbeendebatedoverseveralhundredyears， ， ‘stability’ ， rigorousandphysicallymeaningfuldefinitionofthestabilityofourSolarsystem.
Amongmanydefinitionsofstability， hereweadopttheHilldefinition (Gladman1993): actuallythisisnotadefinitionofstability， ， startingfromacertaininitialconfiguration (Chambers， Wetherill & Boss1996; Ito & Tanikawa1999).， about ±， (Yoshinaga， Kokubo & Makino1999).OfcoursethisstatementcannotbesimplyappliedtosystemswithstableorbitalresonancessuchastheNeptuneCPlutosystem.
1.2Previousstudiesandaimsofthisresearch
