对火星轨道变化问题的最后解释(第7/16页)
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errorplar estite the nurical errorthe plary longitudes，perford the followin pared the resultourlongternbsp;integrations withtest integrations， which spanshorter periods but withhigher uracy than thhis purpose，perford are urate integration with a d 164theintegrations spanning 3105 yr， starting with theinitial conditionsin thonsider that this test integration provideswitseudotrue solutionplary orbita， we pare the test integration with theintegration， n1. for the period3105 yr，seifferencean anoliesthe earth between the two the casethifference canextrapolatedthe value 8700， aboutrotationsearth after 5 gyr， since the errorlongitudes increases linearly within the sylectic p. silarly， the longitude errorpluto canestited12. this value for plutoch better than the resultkinoshita & nakai 1996 where the differenceestited60.
3 nurical results – i. glancethe raw data
in this sectionbriefly review the longternbsp;stabilityplary orbital tion throughsnapshotsraw nurica orbital tionpls indicates longternbsp;stabilityallour nurical integrations:orbital crossings nor close encounters between any pairpls took place.
3.1 neral descriptionthe stabilityplary orbits
first，briefly lookthe neral characterthe longternbsp;stabilityplar interest here focuses particularlythe inner four terrestrial pls for which the orbital tiscales areshorter than thosethe outer fivcan see clearly fronbsp;the planar orbital configurations shownfigs 2 and 3， orbital positionsthe terrestrial pls differ little between the initial and final parteach nurical integration， whi
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3 nurical results – i. glancethe raw data
in this sectionbriefly review the longternbsp;stabilityplary orbital tion throughsnapshotsraw nurica orbital tionpls indicates longternbsp;stabilityallour nurical integrations:orbital crossings nor close encounters between any pairpls took place.
3.1 neral descriptionthe stabilityplary orbits
first，briefly lookthe neral characterthe longternbsp;stabilityplar interest here focuses particularlythe inner four terrestrial pls for which the orbital tiscales areshorter than thosethe outer fivcan see clearly fronbsp;the planar orbital configurations shownfigs 2 and 3， orbital positionsthe terrestrial pls differ little between the initial and final parteach nurical integration， whi
本章未完，请点击下一页继续阅读 》》