# Science Objectives of the Ganymede Laser Altimeter (GALA) for the JUICE   Mission

**Authors:** Jun Kimura, Hauke Hussmann, Shunichi Kamata, Koji Matsumoto, Jurgen, Oberst, Gregor Steinbrugge, Alexander Stark, Klaus Gwinner, Shoko Oshigami,, Noriyuki Namiki, Kay Lingenauber, Keigo Enya, Kiyoshi Kuramoto, Sho Sasaki

arXiv: 1803.01511 · 2018-03-19

## TL;DR

The Ganymede Laser Altimeter (GALA) on the JUICE mission will be the first to measure the topography, surface properties, and subsurface ocean presence of Jupiter's icy moons, advancing planetary science.

## Contribution

GALA introduces novel laser altimetry techniques for icy moons, enabling detailed surface and subsurface analysis for the first time.

## Key findings

- First laser altimeter for icy bodies.
- Enhanced understanding of surface features and tectonics.
- Potential detection of subsurface oceans.

## Abstract

Laser altimetry is a powerful tool for addressing the major objectives of planetary physics and geodesy, and have been applied in planetary explorations of the Moon, Mars, Mercury, and the asteroids Eros, and Itokawa. The JUpiter Icy Moons Explorer (JUICE), led by European Space Agency (ESA), has started development to explore the emergence of habitable worlds around gas giants. The Ganymede Laser Altimeter (GALA) will be the first laser altimeter for icy bodies, and will measure the shape and topography of the large icy moons of Jupiter, (globally for Ganymede, and using flyby ground-tracks for Europa and Callisto). Such information is crucial for understanding the formation of surface features and can tremendously improve our understanding of the icy tectonics. In addition, the GALA will infer the presence or absence of a subsurface ocean by measuring the tidal and rotational responses. Furthermore, it also improves the accuracy of gravity field measurements reflecting the interior structure, collaborating with the radio science experiment. In addition to range measurements, the signal strength and the waveform of the laser pulses reflected from the moon's surface contain information about surface reflectance at the laser wavelength and small scale roughness. Therefore we can infer the degrees of chemical and physical alterations, e.g., erosion, space weathering, compaction and deposition of exogenous materials, through GALA measurements without being affected by illumination conditions. JUICE spacecraft carries ten science payloads including GALA. They work closely together in a synergistic way with GALA being one of the key instruments for understanding the evolution of the icy satellites Ganymede, Europa, and Callisto.

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1803.01511/full.md

## References

50 references — full list in the complete paper: https://tomesphere.com/paper/1803.01511/full.md

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Source: https://tomesphere.com/paper/1803.01511