# In situ Exploration of the Giant Planets

**Authors:** Olivier Mousis, David H. Atkinson, Richard Ambrosi, Sushil Atreya, Don, Banfield, Stas Barabash, Michel Blanc, Thibault Cavali\'e, Athena Coustenis,, Magali Deleuil, Georges Durry, Francesca Ferri, Leigh Fletcher, Thierry, Fouchet, Tristan Guillot, Paul Hartogh, Ricardo Hueso, Mark Hofstadter,, Jean-Pierre Lebreton, Kathleen E. Mandt, Heike Rauer, Pascal Rannou,, Jean-Baptiste Renard, Agustin Sanchez-L\'avega, Kunio Sayanagi, Amy Simon,, Thomas Spilker, Ethiraj Venkatapathy, J. Hunter Waite, Peter Wurz

arXiv: 1908.00917 · 2019-08-05

## TL;DR

This paper advocates for in situ atmospheric probes for Saturn, Uranus, and Neptune to overcome remote sensing limitations, aiming to deepen understanding of planetary formation and atmospheric physics.

## Contribution

It outlines scientific goals and mission concepts for future in situ exploration of the giant planets beyond Jupiter, emphasizing their importance for planetary science.

## Key findings

- In situ measurements provide critical data on atmospheric composition.
- Proposed probes could significantly advance understanding of planet formation.
- Future missions could include ESA contributions to NASA's exploration efforts.

## Abstract

Remote sensing observations suffer significant limitations when used to study the bulk atmospheric composition of the giant planets of our solar system. This impacts our knowledge of the formation of these planets and the physics of their atmospheres. A remarkable example of the superiority of in situ probe measurements was illustrated by the exploration of Jupiter, where key measurements such as the determination of the noble gases' abundances and the precise measurement of the helium mixing ratio were only made available through in situ measurements by the Galileo probe. Here we describe the main scientific goals to be addressed by the future in situ exploration of Saturn, Uranus, and Neptune, placing the Galileo probe exploration of Jupiter in a broader context. An atmospheric entry probe targeting the 10-bar level would yield insight into two broad themes: i) the formation history of the giant planets and that of the Solar System, and ii) the processes at play in planetary atmospheres. The probe would descend under parachute to measure composition, structure, and dynamics, with data returned to Earth using a Carrier Relay Spacecraft as a relay station. An atmospheric probe could represent a significant ESA contribution to a future NASA New Frontiers or flagship mission to be launched toward Saturn, Uranus, and/or Neptune.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1908.00917/full.md

## Figures

15 figures with captions in the complete paper: https://tomesphere.com/paper/1908.00917/full.md

## References

184 references — full list in the complete paper: https://tomesphere.com/paper/1908.00917/full.md

---
Source: https://tomesphere.com/paper/1908.00917