Talk:Hilda asteroid

Apr 20, 2026 - 04:32

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Hildas and the Kirkwood Gaps: Reply

← Previous revision		Revision as of 23:00, 19 April 2026
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	:The 4:1, 3:1, 5:2, 7:3 resonances are empty because interacting secular resonances inside the MMR resonances cause the orbits to become chaotic resulting in large jumps in eccentricity and planet crossing orbits.		:The 4:1, 3:1, 5:2, 7:3 resonances are empty because interacting secular resonances inside the MMR resonances cause the orbits to become chaotic resulting in large jumps in eccentricity and planet crossing orbits.
	:https://www.oca.eu/morby/papers/1041a.pdf [[User:Agmartin\|Agmartin]] ([[User talk:Agmartin\|talk]]) 20:06, 25 September 2013 (UTC)		:https://www.oca.eu/morby/papers/1041a.pdf [[User:Agmartin\|Agmartin]] ([[User talk:Agmartin\|talk]]) 20:06, 25 September 2013 (UTC)
			::I'm aware of why the other resonance points result in unstable orbits. Why doesn't this happen at with the Hildas? [[User:MiguelMunoz\|MiguelMunoz]] ([[User talk:MiguelMunoz\|talk]]) 23:00, 19 April 2026 (UTC)

	== Similar families? ==		== Similar families? ==