对火星轨道变化问题的最后解释(第2/16页)
ry tionthe solar syste actuallyis not easygivlear， rigorous and physically aningful definitionthe stabilitr solar syste
angdefinitionsstability， hereadopt the hill definition gladn 1993: actually thisnoefinitionstability， buefinystenbsp;as bing unstable whelose encounter urs sowherethe syste starting fronbsp;a certain initial configuration chaers， wetherill & boss 1996; ito & tanikaw;is definedexperiencinlose encounter when two bodies approach one another withinareathe larr hil the systenbsp;is definedbeinstate that our plary systenbsp;is dynacally stableno close encounter happens during the aour solar syste about ， this definition yreplacedonewhichurrenceany orbital crossing between eithera pairpls takebecauseknow fronbsp;experience thatorbital crossingvery likelyleada close encounterplary and prlary syste yoshinaga， kokubo & makin course this statent cannotsily appliedsyste with stable orbital resonances suchthe neptune–pluto syste
1.2previous studies andof this research
in additionthe vaguenessthe conceptstability， the plsour solar systenbsp;shoharacter typicaldynacal chaos sussn & wisdonbsp;1988， causethis chaotic behaviournow partly understoodbeinesultresonance overlapping murray & holn 1999; lecar， franklin & hol，would require integrating overenseleplary syste including all nine pls foeriod covering severalgyrthoroughly understand the longternbsp;evolutionplary orbits， since chaotic dynacal syste are characterizedtheir strong dependenceinitial conditions.
fronbsp;that pointview，of the previou
本章未完，请点击下一页继续阅读 》》
angdefinitionsstability， hereadopt the hill definition gladn 1993: actually thisnoefinitionstability， buefinystenbsp;as bing unstable whelose encounter urs sowherethe syste starting fronbsp;a certain initial configuration chaers， wetherill & boss 1996; ito & tanikaw;is definedexperiencinlose encounter when two bodies approach one another withinareathe larr hil the systenbsp;is definedbeinstate that our plary systenbsp;is dynacally stableno close encounter happens during the aour solar syste about ， this definition yreplacedonewhichurrenceany orbital crossing between eithera pairpls takebecauseknow fronbsp;experience thatorbital crossingvery likelyleada close encounterplary and prlary syste yoshinaga， kokubo & makin course this statent cannotsily appliedsyste with stable orbital resonances suchthe neptune–pluto syste
1.2previous studies andof this research
in additionthe vaguenessthe conceptstability， the plsour solar systenbsp;shoharacter typicaldynacal chaos sussn & wisdonbsp;1988， causethis chaotic behaviournow partly understoodbeinesultresonance overlapping murray & holn 1999; lecar， franklin & hol，would require integrating overenseleplary syste including all nine pls foeriod covering severalgyrthoroughly understand the longternbsp;evolutionplary orbits， since chaotic dynacal syste are characterizedtheir strong dependenceinitial conditions.
fronbsp;that pointview，of the previou
本章未完，请点击下一页继续阅读 》》