Monitoring JUICE deployment operations with high-accuracy accelerometer data

The Jupiter Icy Moons Explorer (JUICE) mission is a cornerstone of ESA's Cosmic Vision 2015–2025 program devoted to the scientific exploration of Jupiter and its icy moons. Launched on April 14, 2023, from French Guiana, JUICE will perform multiple gravity assists, including an unprecedented lunar-Earth double gravity assist, in order to shape its trajectory to Jupiter, where it will arrive in July 2031. Thanks to a suite of 10 scientific instruments, JUICE will carry out a comprehensive investigation of the jovian system, with special focus on Ganymede. Among these experiments is the Gravity and Geophysics of Jupiter and the Galilean Moons (3GM) radio science and planetary geodesy experiment, supported by the onboard High Accuracy Accelerometer (HAA). The HAA, a three-axis spring mass accelerometer, measures the non-gravitational perturbations acting on the spacecraft, that need to be measured in order to fully exploit the highly accurate range and range rate measurements of 3GM. This paper analyzes the HAA data collected in the very early phase of the mission, to monitor the initial deployment of the spacecraft's moving appendages. The vibration modes of the magnetometer boom and solar arrays were clearly detected during the appendages' deployment, as well as the latching of the Langmuir probe hinges. The detected resonance frequencies of the first and second magnetometer boom bending modes are equal to 0.44 and 0.46 Hz, respectively. The HAA data contributed to identifying the root-cause of the anomalous Radar for Icy Moon Exploration (RIME) antenna deployment. The strong external perturbations due to the actuators' activation have been used to characterize the spacecraft tranquillization time. Despite the significant increase in the spacecraft noise floor during deployment events, the full sensitivity of the instrument was regained within 10 min. This information can be used to plan the spacecraft operations during the scientific phase of the mission. • Mission Overview : The ESA Jupiter Icy Moons Explorer mission will study the Jupiter's icy moons with a focus on Ganymede. • HAA instrument : The HAA has a sensitivity of 10 −8 m/s 2 /Hz 0.5 in the measurement bandwidth of 10 −4 -10 −1 Hz. • Deployment operations : After JUICE's launch, the primary goal was to deploy the spacecraft's movable appendages. • Article focus : HAA data analysis collected during JUICE appendages deployments. • Results : HAA detected the main vibrating modes, enabling a comprehensive study of the spacecraft dynamic response.

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Publication Details

Journal
Acta Astronautica
Published
2024-09-23
DOI
https://doi.org/10.1016/j.actaastro.2024.09.047
Citations
1
Primary Topic
Inertial Sensor and Navigation
Type
article
Field-Weighted Citation Impact
1.30

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Monitoring JUICE deployment operations with high-accuracy accelerometer data

Chiara Grappasonni, Umberto De Filippis, L. Iess, Paolo Cappuccio et al.
1 citations
Acta Astronautica
Inertial Sensor and Navigation
1.30
article

Monitoring JUICE deployment operations with high-accuracy accelerometer data

Chiara Grappasonni, Umberto De Filippis, L. Iess, Paolo Cappuccio, A. Olivieri, Massimiliano Pecora, Mauro Di Benedetto
article en
1 citations

Abstract

The Jupiter Icy Moons Explorer (JUICE) mission is a cornerstone of ESA's Cosmic Vision 2015–2025 program devoted to the scientific exploration of Jupiter and its icy moons. Launched on April 14, 2023, from French Guiana, JUICE will perform multiple gravity assists, including an unprecedented lunar-Earth double gravity assist, in order to shape its trajectory to Jupiter, where it will arrive in July 2031. Thanks to a suite of 10 scientific instruments, JUICE will carry out a comprehensive investigation of the jovian system, with special focus on Ganymede. Among these experiments is the Gravity and Geophysics of Jupiter and the Galilean Moons (3GM) radio science and planetary geodesy experiment, supported by the onboard High Accuracy Accelerometer (HAA). The HAA, a three-axis spring mass accelerometer, measures the non-gravitational perturbations acting on the spacecraft, that need to be measured in order to fully exploit the highly accurate range and range rate measurements of 3GM. This paper analyzes the HAA data collected in the very early phase of the mission, to monitor the initial deployment of the spacecraft's moving appendages. The vibration modes of the magnetometer boom and solar arrays were clearly detected during the appendages' deployment, as well as the latching of the Langmuir probe hinges. The detected resonance frequencies of the first and second magnetometer boom bending modes are equal to 0.44 and 0.46 Hz, respectively. The HAA data contributed to identifying the root-cause of the anomalous Radar for Icy Moon Exploration (RIME) antenna deployment. The strong external perturbations due to the actuators' activation have been used to characterize the spacecraft tranquillization time. Despite the significant increase in the spacecraft noise floor during deployment events, the full sensitivity of the instrument was regained within 10 min. This information can be used to plan the spacecraft operations during the scientific phase of the mission. • Mission Overview : The ESA Jupiter Icy Moons Explorer mission will study the Jupiter's icy moons with a focus on Ganymede. • HAA instrument : The HAA has a sensitivity of 10 −8 m/s 2 /Hz 0.5 in the measurement bandwidth of 10 −4 -10 −1 Hz. • Deployment operations : After JUICE's launch, the primary goal was to deploy the spacecraft's movable appendages. • Article focus : HAA data analysis collected during JUICE appendages deployments. • Results : HAA detected the main vibrating modes, enabling a comprehensive study of the spacecraft dynamic response.

Acta AstronauticaVol. 225
Leonardo (United States) (US), Agenzia Spaziale Italiana (IT), European Space Astronomy Centre (ES), Sapienza University of Rome (IT)
Agenzia Spaziale Italiana
Affordable and clean energy
Openalex Percentile: Top 13%
Inertial Sensor and Navigation
1.30
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