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Small Bodies in the Distant Solar System

Lawler, Samantha M. & Pike, Rosemary E. (2024)

Published
Oct 6, 2024
Journal
arXiv preprint
DOI
10.48550/arXiv.2410.04338

At a GlanceAI

Short review of distant small bodies as a record of giant-planet migration, with emphasis on survey biases.

SummaryAI

Lawler and Pike summarize what Kuiper Belt objects tell us about planet formation: orbits constrain how the giant planets migrated, while sizes, shapes and surfaces constrain formation and collision rates. The review stresses that every telescopic survey is biased and that de-biased comparisons with simulations are what made progress possible. Some orbits remain hard to explain, and the authors point to upcoming surveys such as the Vera Rubin Observatory as the next step.

Method SnapshotAI

Narrative review (preprint).

BackgroundAI

Basic Solar System dynamics; no specialist background needed.