Split Peas in a Pod: Intra-System Uniformity of Super-Earths and Sub-Neptunes
Sarah C. Millholland, Joshua N. Winn

TL;DR
This study investigates the uniformity of planet sizes within multi-planet systems, revealing that planets of the same category tend to be more similar in size, with implications for planetary formation and composition.
Contribution
It demonstrates that intra-system size uniformity is stronger within the same planet category and explores differences between super-Earths and sub-Neptunes, including effects of stellar metallicity.
Findings
Intra-system size uniformity is twice as strong within the same planet category.
Sub-Neptunes are on average 1.7 times larger than super-Earths in the same system.
Low-metallicity stars host planets with more uniform sizes, with modest statistical significance.
Abstract
The planets within compact multi-planet systems tend to have similar sizes, masses, and orbital period ratios, like "peas in a pod". This pattern was detected when considering planets with radii between 1 and 4 . However, these same planets show a bimodal radius distribution, with few planets between 1.5 and 2 . The smaller "super-Earths" are consistent with being stripped rocky cores, while the larger "sub-Neptunes" likely have gaseous H/He envelopes. Given these distinct structures, it is worthwhile to test for intra-system uniformity separately within each category of planets. Here, we find that the tendency for intra-system uniformity is twice as strong when considering planets within the same size category than it is when combining all planets together. The sub-Neptunes tend to be times larger than the super-Earths in the same system,…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
