Non-equal-mass planet systems are less dynamically stable than equal-mass systems at the same Hill-radius spacing, especially away from first-order resonances, which may help explain the observed peas-in-a-pod mass uniformity.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.EP 1years
2024 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Enhanced Stability in Planetary Systems with Similar Masses
Non-equal-mass planet systems are less dynamically stable than equal-mass systems at the same Hill-radius spacing, especially away from first-order resonances, which may help explain the observed peas-in-a-pod mass uniformity.