"dr\u00E1hov\u00FDmi rezonancemi"@cs . . "dr\u00E1hov\u00FDch rezonanc\u00EDch"@cs . . . . . . "spin-orbit\u00E1ln\u00ED rezonanci"@cs . "Laplaceovy rezonance"@cs . "dr\u00E1hov\u00E9 rezonance"@cs . . "Dr\u00E1hov\u00E1 rezonance, orbit\u00E1ln\u00ED rezonance, Laplaceova rezonance nebo t\u00E9\u017E komensurabilita je vlastnost pohybu dvou t\u011Bles ve slune\u010Dn\u00ED soustav\u011B, p\u0159i kter\u00E9 jsou jejich doby ob\u011Bhu v pom\u011Bru mal\u00FDch cel\u00FDch \u010D\u00EDsel. V takov\u00E9m p\u0159\u00EDpad\u011B nast\u00E1v\u00E1 mezi t\u011Blesy gravita\u010Dn\u00ED vazba (rezonance), kter\u00E1 ovliv\u0148uje stabilitu tohoto uspo\u0159\u00E1d\u00E1n\u00ED."@cs . "Laplaceovy resonance"@cs . . . . "rezonuje"@cs . . "dr\u00E1hov\u00E9 resonanci"@cs . . "rezonanci"@cs . . . "rezonanc\u00ED"@cs . "orbit\u00E1ln\u00ED rezonanci"@cs . "Dr\u00E1hov\u00E1 rezonance"@cs . "1758"^^ . . "rezonance"@cs . "rezonan\u010Dn\u00EDho"@cs . . . . . . "dr\u00E1hov\u00E1 rezonance"@cs . "31981"^^ . "rezonanci ob\u011Bhu"@cs . . . . "Dr\u00E1hov\u00E1 rezonance"@cs . "slad\u011Bnou"@cs . . "15952656"^^ . . . "dr\u00E1hovou rezonanci"@cs . "dr\u00E1hovou rezonanc\u00ED"@cs . "rezonan\u010Dn\u00ED"@cs . "dr\u00E1hov\u00E9 rezonanci"@cs . . . . "26"^^ . "Dr\u00E1hov\u00E1 rezonance, orbit\u00E1ln\u00ED rezonance, Laplaceova rezonance nebo t\u00E9\u017E komensurabilita je vlastnost pohybu dvou t\u011Bles ve slune\u010Dn\u00ED soustav\u011B, p\u0159i kter\u00E9 jsou jejich doby ob\u011Bhu v pom\u011Bru mal\u00FDch cel\u00FDch \u010D\u00EDsel. V takov\u00E9m p\u0159\u00EDpad\u011B nast\u00E1v\u00E1 mezi t\u011Blesy gravita\u010Dn\u00ED vazba (rezonance), kter\u00E1 ovliv\u0148uje stabilitu tohoto uspo\u0159\u00E1d\u00E1n\u00ED. Ob\u011B\u017En\u00E9 dr\u00E1hy, po kter\u00FDch se tato t\u011Blesa pohybuj\u00ED, naz\u00FDv\u00E1me komensurabiln\u00ED.Typick\u00FDm p\u0159\u00EDpadem je komensurabilita ob\u011B\u017En\u00FDch drah planet Jupitera a Saturnu, jejich\u017E ob\u011B\u017En\u00E9 doby (11,86 roku, resp. 29,46 roku) jsou v pom\u011Bru 2:5. Jin\u00FDm p\u0159\u00EDkladem mohou b\u00FDt troj\u00E1ni, planetky, ob\u00EDhaj\u00EDc\u00ED po stejn\u00E9 dr\u00E1ze jako Jupiter a tedy pohybuj\u00EDc\u00ED se v komensurabilit\u011B 1:1, nebo plutina, transneptunick\u00E1 t\u011Blesa, pohybuj\u00EDc\u00ED se po komensurabiln\u00EDch drah\u00E1ch s Neptunem v pom\u011Bru 3:2.Komensurabilita se velice \u010Dasto vyskytuje i v soustav\u00E1ch m\u011Bs\u00EDc\u016F planet a hraje v\u00FDznamnou roli v jemn\u00E9 struktu\u0159e prstenc\u016F planet. Komensurabilita s Jupiterem m\u00E1 velk\u00FD v\u00FDznam i p\u0159i vytv\u00E1\u0159en\u00ED Kirkwoodov\u00FDch mezer v hlavn\u00EDm p\u00E1su planetek."@cs . "dr\u00E1hov\u00E1 (orbit\u00E1ln\u00ED) rezonance"@cs .