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第76章 对火星轨道变化问题的最后解释(5/12)

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lasthatsans±51010yr.nection6ealsodiscussthelong-termstabilityofthelaarymotionanditsossiblecause.

2escritionofthenumericalintegrations

(本部分涉及比较复杂的积分计算,作者君就不贴上来了,贴上来了起点也不一定能成功显示。)

2.3umericalmethod

eutilizeasecond-orderisdom–olmansymlecticmaasourmainintegrationmethod(isdom&inoshita,oshida&&akai1991)ithasecialstart-uroceduretoreducethetruncationerrorofanglevariables,‘armstart’(aha&&remaine1992,1994).

hestesizeforthenumericalintegrationsis8dthroughoutallintegrationsoftheninelas(±1,2,3),hichisabout111oftheorbitaleriodoftheinnermostla(ercury).sforthedeterminationofstesize,eartlyfollothereviousnumericalintegrationofallninelasinussman&&isdom(1988,7.2d)andaha&&remaine(1994,22532d).eroundedthedecimalartofthetheirstesizesto8tomakethestesizeamultileof2inordertoreducetheaumulationofround-offerrorintheutationrocesses.nrelationtothis,isdom&&olman(1991)erformednumericalintegrationsoftheouterfivelaaryorbitsusingthesymlecticmaithastesizeof400d,110.83oftheorbitaleriodofuiter.heirresultseemstobeaurateenough,hichartlyjustifiesourmethodofdeterminingthestesize.oever,sincetheeentricityofuiter(~0.05)ismuchsmallerthanthatofercury(~0.2),eneedsomecarehenearetheseintegrationssimlyintermsofstesizes.

ntheintegrationoftheouterfivelas(±),efixedthestesizeat400d.

eadotauss'fandgfunctionsinthesymlecticmatogetheriththethird-orderalleymethod(anby1992)asasolverforelerequations.henumberofmaximumiterationsesetinalley'smethodis15,buttheyneverreachedthemaximuminanyofourintegrations.

heintervalofthedataoututis200000d(~547yr)forthecalculat
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