English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Through a semi-analytic approach of the Kozai resonance inside an MMR, weshow phase diagrams (e,{\omega}) that suggest the possibility of a scatteredparticle, after being captured in an MMR with Neptune, to become a detachedobject. We ran several numerical integrations with thousands of particlesperturbed by the four major planets, and there are cases with and withoutNeptune's residual migration. These were developed to check the semi-analyticapproach and to better understand the dynamical mechanisms that produce thedetached objects close to an MMR. The numerical simulations with and without aresidual migration for Neptune stress the importance of a particular resonancemode, which we name the hibernating mode, on the formation of fossilizeddetached objects close to MMRs. When considering Neptune's residual migrationwe are able to show the formation of detached orbits. These objects arefossilized and cannot be trapped in the MMRs again. We find a ratio of thenumber of fossilized objects with moderate perihelion distance (35 < q < 40 au)to the number of objects with high perihelion distance (q > 40 au) as 3.0/1 forobjects close to the 2:5, and 1.7/1 for objects close to the 1:3 resonance. Weestimate that the two fossilized population have a total mass between 0.1 and0.3 Pluto's mass.

Dynamical formation of detached trans-Neptunian objects close to the 2:5 and 1:3 mean motion resonances with Neptune