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LATENT REFERENCES / TAG2

Orbital Resonance and Secular Resonance

Archive curator and editor: Keigo Yoshida

This reference note belongs to Tag2 in Latent References, an archive curated by Keigo Yoshida. Its archive region is Physics. The note preserves its source text and links so that readers can trace the material behind the 3D map.

Collection
Tag2
Archive region
Physics

Archived reference note

English translation of the archived note. JP shows the original text. Source links and literal code are retained; the translation does not update or independently verify the source claims.

Orbital resonance (Japanese pronunciation: kido kyomei; orbital resonance1) is, in celestial mechanics, a change in the orbits of 2 bodies orbiting another body as a result of their mutual gravitational influence1. It includes mean-motion resonance2, which acts over short timescales comparable to the orbital period, and secular resonance3, which acts over long timescales of 104 - 106 years. #physics

Source updated 2024-08-05 · Snapshot 2026-10-08

Source links and calculated neighbors

Cosine values measure shared lexical features, not truth, agreement or identical meaning. Original reference links are labeled separately.

  • Lagrange PointsComputed lexical cosine similarity 0.195 · shared title, text, tags and references
  • Landau DampingComputed lexical cosine similarity 0.188 · shared title, text, tags and references
  • Kirkwood GapsComputed lexical cosine similarity 0.184 · shared title, text, tags and references
  • Coupled Oscillator SystemsComputed lexical cosine similarity 0.175 · shared title, text, tags and references
  • Phase SingularitiesComputed lexical cosine similarity 0.172 · shared title, text, tags and references
  • Protoplanetary DiskComputed lexical cosine similarity 0.166 · shared title, text, tags and references
  • Subatomic ParticlesComputed lexical cosine similarity 0.162 · shared title, text, tags and references