Interior and evolution of the giant planets

Y Miguel, A Vazan - Remote Sensing, 2023 - mdpi.com
The giant planets were the first to form and hold the key to unveiling the solar system's
formation history in their interiors and atmospheres. Furthermore, the unique conditions …

Multiple probe measurements at Uranus motivated by spatial variability

MH Wong, N Rowe-Gurney, S Markham… - Space Science …, 2024 - Springer
A major motivation for multiple atmospheric probe measurements at Uranus is the
understanding of dynamic processes that create and maintain spatial variation in thermal …

Phase separation of planetary ices explains nondipolar magnetic fields of Uranus and Neptune

B Militzer - Proceedings of the National Academy of Sciences, 2024 - pnas.org
The Voyager spacecraft discovered that the ice giants Uranus and Neptune have nondipolar
magnetic fields, defying expectations that a thick interior layer of planetary ices would …

Ring seismology of the ice giants uranus and neptune

JA A'Hearn, MM Hedman, CR Mankovich… - The Planetary …, 2022 - iopscience.iop.org
We assess the prospect of using ring seismology to probe the interiors of the ice giants
Uranus and Neptune. We do this by calculating normal-mode spectra for different interior …

The deep oxygen abundance in solar system giant planets, with a new derivation for Saturn

T Cavalié, J Lunine, O Mousis, R Hueso - Space Science Reviews, 2024 - Springer
Deep elemental composition is a challenging measurement to achieve in the giant planets
of the solar system. Yet, knowledge of the deep composition offers important insights in the …

The interior of Uranus-Thermal profile, bulk composition, and the distribution of rock, water, and hydrogen and helium

L Morf, S Müller, R Helled - Astronomy & Astrophysics, 2024 - aanda.org
We present improved empirical density profiles of Uranus and interpret them in terms of their
temperature and composition using a new random algorithm. The algorithm to determine the …

Saturn's seismic rotation revisited

CR Mankovich, JW Dewberry… - The Planetary Science …, 2023 - iopscience.iop.org
Normal mode seismology is a promising means of measuring rotation in gas giant interiors,
and ring seismology presents a singular opportunity to do so at Saturn. We calculate …

The Uranus system from occultation observations (1977–2006): Rings, pole direction, gravity field, and masses of Cressida, Cordelia, and Ophelia

RG French, MM Hedman, PD Nicholson, PY Longaretti… - Icarus, 2024 - Elsevier
From an analysis of 31 Earth-based stellar occultations and three Voyager 2 occultations
spanning 1977–2006 (French et al. 2023a), we determine the keplerian orbital elements of …

Thermal and Tidal Evolution of Ice Giants with Growing Frozen Cores: The Case of Neptune

DA James, L Stixrude - Space Science Reviews, 2024 - Springer
The contrasting internal luminosity of Uranus and Neptune present a challenge to our
understanding of the origin and evolution of these bodies, as well as extra-solar ice giants …

The miscibility of hydrogen and water in planetary atmospheres and interiors

A Gupta, L Stixrude, HE Schlichting - arXiv preprint arXiv:2407.04685, 2024 - arxiv.org
Many planets in the solar system and across the galaxy have hydrogen-rich atmospheres
overlying more heavy element-rich interiors with which they interact for billions of years …