对火星轨道变化问题的最后解释(第13/16页)
ntunbsp; the other hand， the sejor axesvenus and earth are less likelybe disturbedthe jovia the energy exchan ylited only within the venus–earth pair， which resultsa negative correlationthe exchanorbital energythe pair.
as for the outer jovian plary subsyste jupiter–saturn and uranus–neptune seenbsp;todynaca， the strengththeir couplingnotstrong&nbsppared with thatthe venus–earth pair.
551010yr integrationsouter plary orbits
since the jovian plary sses arelarr than the terrestrial plary sses，treat the jovian plary systenbsp;asindependent plary systenbsp;in terthe studyits dynaca，addeoupletrial integrations that span51010 yr， including only the outer five pls the four jovian pls plu results exhibit the rigorous stabilitythe outer plary systenbsp;over this lon configuration， and variationentricities and inclination show this very longternbsp;stabilitythe outer five plsboth theand the frequencdo not showhere， the typical frequencythe orbital oscillationpluto and the other outer plsalst constant during these very longternbsp;integration periods， whichdenstratedthe ti–frequencyon our webpa.
in these two integrations， the relative nurical errorthe total energy was 106 and thatthe total angular ntunbsp;was 1010.
5.1 resonancesthe neptune–pluto systebr>
kinoshita & nakai 1996 integrated the outer five plary orbits they found that four jor resonances between neptune and pluto are intained during the whole integration period， and that the resonances ythecausesthe stabilitythe orbior four resonances foundprevious research a
本章未完，请点击下一页继续阅读 》》
as for the outer jovian plary subsyste jupiter–saturn and uranus–neptune seenbsp;todynaca， the strengththeir couplingnotstrong&nbsppared with thatthe venus–earth pair.
551010yr integrationsouter plary orbits
since the jovian plary sses arelarr than the terrestrial plary sses，treat the jovian plary systenbsp;asindependent plary systenbsp;in terthe studyits dynaca，addeoupletrial integrations that span51010 yr， including only the outer five pls the four jovian pls plu results exhibit the rigorous stabilitythe outer plary systenbsp;over this lon configuration， and variationentricities and inclination show this very longternbsp;stabilitythe outer five plsboth theand the frequencdo not showhere， the typical frequencythe orbital oscillationpluto and the other outer plsalst constant during these very longternbsp;integration periods， whichdenstratedthe ti–frequencyon our webpa.
in these two integrations， the relative nurical errorthe total energy was 106 and thatthe total angular ntunbsp;was 1010.
5.1 resonancesthe neptune–pluto systebr>
kinoshita & nakai 1996 integrated the outer five plary orbits they found that four jor resonances between neptune and pluto are intained during the whole integration period， and that the resonances ythecausesthe stabilitythe orbior four resonances foundprevious research a
本章未完，请点击下一页继续阅读 》》