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Enhanced Stability in Planetary Systems with Similar Masses

  • Authors: Dong-Hong Wu, Sheng Jin, Jason H. Steffen

Dong-Hong Wu et al 2025 The Astronomical Journal 169 .

  • Provider: AAS Journals

Caption: Figure 1.

Dynamical instability timescale t/t0 as a function of the spacing parameter K. The error bars are given by the 16th and 84th percentile of the dynamical instability timescale distribution. Blue dots represent results from equal-mass systems, while the orange, green and red markers correspond to systems with modified Gini index ﹩{{ \mathcal G }}_{m}﹩ within the ranges [0, 0.32], [0.32, 0.65] and [0.65, 0.97], respectively. Gray and purple vertical dashed lines indicate the locations of first and second-order MMRs for planet pairs in equal-mass systems, respectively.

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