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Machine learning classification of outer solar system objects

Published on:

8 May 2024

Primary Category:

Earth and Planetary Astrophysics

Paper Authors:

Kathryn Volk,

Renu Malhotra

Bullets

Key Details

Model matches human judgement 98% of the time when classifying TNOs

Custom data features identify resonant dynamics missed by simpler methods

Vastly more efficient than manual classification with exponentially growing datasets

Will enable robust comparison of models to new observations from Vera Rubin Observatory

Provides classification probabilities; improves on binary secure/insecure designations

AI generated summary

Machine learning classification of outer solar system objects

This paper presents a supervised machine learning model to classify icy bodies beyond Neptune called trans-Neptunian objects (TNOs) into different dynamical groups. The model was trained on a large and diverse dataset of real and synthetic TNO orbits. It uses custom features from numerical integrations to identify complex resonant dynamics. When tested, the model matched human judgement 98% of the time, offering major improvements in efficiency over manual classification as observations increase exponentially.

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