Onboard Machine Learning for High-Energy Observatories for Spacecraft Autonomy and Ground Segment Operations

Next-generation space observatories for high-energy gamma-ray astrophysics will increase scientific return using onboard machine learning (ML). This is now possible thanks to today’s low-power, radiation-tolerant processors and artificial intelligence accelerators. This paper provides an overview of current and future ML applications in gamma-ray space missions focused on high-energy transient phenomena. We discuss onboard ML use cases that will be implemented in the future, including real-time event detection and classification (e.g., gamma-ray bursts), and autonomous decision-making, such as rapid repointing to transient events or optimising instrument configuration based on the scientific target or environmental conditions.

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Publication Details

Journal
Particles
Published
2025-12-12
DOI
https://doi.org/10.3390/particles8040102
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
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article

Onboard Machine Learning for High-Energy Observatories for Spacecraft Autonomy and Ground Segment Operations

Particles
Gamma-ray bursts and supernovae
article

Onboard Machine Learning for High-Energy Observatories for Spacecraft Autonomy and Ground Segment Operations

article en

Abstract

Next-generation space observatories for high-energy gamma-ray astrophysics will increase scientific return using onboard machine learning (ML). This is now possible thanks to today’s low-power, radiation-tolerant processors and artificial intelligence accelerators. This paper provides an overview of current and future ML applications in gamma-ray space missions focused on high-energy transient phenomena. We discuss onboard ML use cases that will be implemented in the future, including real-time event detection and classification (e.g., gamma-ray bursts), and autonomous decision-making, such as rapid repointing to transient events or optimising instrument configuration based on the scientific target or environmental conditions.

ParticlesVol. 8(4)
University of Padua (IT), Astronomical Observatory of Rome (IT), Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna (IT), Institute for Space Astrophysics and Planetology (IT)
Openalex Percentile: Top 35%
Gamma-ray bursts and supernovae
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