TOI-2195 A b is an inflated hot Neptune that likely originated as a Jovian planet losing ~90% mass through Roche lobe overflow during EKL-driven high-eccentricity migration triggered by a wide binary companion.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
years
2026 3verdicts
UNVERDICTED 3representative citing papers
Relaxing the double-averaged approximation shows short-range forces catalyze extreme eccentricity and secular j_z evolution in hierarchical triples via discrete jumps in adiabatic invariants at quadrupole order.
Secular chaos regulated by the inner-to-outer ZLK timescale ratio R enables high-eccentricity tidal migration in 3+1 systems at sub-critical inclinations, producing polar hot Jupiters.
citing papers explorer
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Short-Range Forces Can Catalyze Extreme Orbital Evolution in Hierarchical Triples
Relaxing the double-averaged approximation shows short-range forces catalyze extreme eccentricity and secular j_z evolution in hierarchical triples via discrete jumps in adiabatic invariants at quadrupole order.