第76章 对火星轨道变化问题的最后解释（9/12）
icitiesandinclinationsofercuryonatime-scaleofseveral109yr.oever，theeffectoftheossibleinstabilityoftheorbitofercurymaynotfatallyaffecttheglobalstabilityoftheholelaarysystemoingtothesmallmassofercury.eillmentionbrieflythelong-termorbitalevolutionofercurylaterinection4usinglo-assfilteredorbitalelements.
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heorbitalmotionoftheouterfivelasseemsrigorouslystableandquiteregularoverthistime-san(seealsoection5).
3.2ime–frequencymas
lthoughthelaarymotionexhibitsverylong-termstabilitydefinedasthenon-existenceofcloseencounterevents，thechaoticnatureoflaarydynamicscanchangetheoscillatoryeriodandamlitudeoflaaryorbitalmotiongraduallyoversuchlongtime-sans.vensuchslightfluctuationsoforbitalvariationinthefrequencydomain，articularlyinthecaseofarth，canotentiallyhaveasignificanteffectonitssurfaceclimatesystemthroughsolarinsolationvariation(cf.erger1988).
ogiveanovervieofthelong-termchangeineriodicityinlaaryorbitalmotion，eerformedmanyfastouriertransformations(s)alongthetimeaxis，andsuerosedtheresultingeriodgramstodrato-dimensionaltime–frequencymas.hesecificaroachtodraingthesetime–frequencymasinthisaerisverysimle–muchsimlerthantheaveletanalysisoraskar's(1990，1993)frequencyanalysis.
ividethelo-assfilteredorbitaldataintomanyfragmentsofthesamelenh.helenhofeachdatasegmentshouldbeamultileof2inordertoalythe.
achfragmentofthedatahasalargeoverlaingart:forexamle，hentheithdatabeginsfromt=tiandendsatt=ti+，thenextdatasegmentrangesfromti+δ≤ti+δ+，hereδ?.econtinuethisdivisionuntilereachacertainnumberbyhichtn+reachesthetotalinteg
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