Perspectives on the distribution of orbits of distant Trans-Neptunian Objects
JJ Kavelaars, Samantha M. Lawler, Michele T. Bannister, Cory, Shankman

TL;DR
This paper analyzes the orbital patterns of distant Trans-Neptunian Objects to understand the outer Solar System's structure, considering observational biases and gravitational influences, and discusses implications of these patterns for planetary science.
Contribution
It provides a comprehensive discussion on how observational biases and gravitational processes shape the observed orbital distributions of TNOs, offering insights into the outer Solar System's history.
Findings
Orbital patterns suggest possible hidden processes in the outer Solar System.
Observational biases significantly influence the known TNO orbit data.
Gravitational interactions shape the distribution of TNO orbits.
Abstract
Looking at the orbits of small bodies with large semimajor axes, we are compelled to see patterns. Some of these patterns are noted as strong indicators of new or hidden processes in the outer Solar System, others are substantially generated by observational biases, and still others may be completely overlooked. We can gain insight into the current and past structure of the outer Solar System through a careful examination of these orbit patterns. In this chapter, we discuss the implications of the observed orbital distribution of distant trans-Neptunian objects (TNOs). We start with some cautions on how observational biases must affect the known set of TNO orbits. Some of these biases are intrinsic to the process of discovering TNOs, while others can be reduced or eliminated through careful observational survey design. We discuss some orbital element correlations that have received…
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