4.7 Review

Interior and Evolution of the Giant Planets

相关参考文献

注意:仅列出部分参考文献,下载原文获取全部文献信息。
Article Astronomy & Astrophysics

Accounting for non-ideal mixing effects in the hydrogen-helium equation of state

S. Howard et al.

Summary: This paper proposes a simple method to consider the interactions between hydrogen and helium in the interior and evolution models of giant planets. It is found that non-ideal mixing effects have significant impacts on the interior models of giant planets and the mass-radius relation of exoplanets. The study shows that the density and entropy can vary up to 15% when non-ideal mixing is considered.

ASTRONOMY & ASTROPHYSICS (2023)

Article Astronomy & Astrophysics

Zonal Winds of Uranus and Neptune: Gravitational Harmonics, Dynamic Self-gravity, Shape, and Rotation

Deniz Soyuer et al.

Summary: This study investigates the zonal wind speeds in Uranus and Neptune and finds that they diminish rapidly. The researchers create structure models of the planets and consider the density perturbations caused by zonal winds and their dynamic self-gravity. They discover that the maximum scale height of the winds is about 2%-3% of the planetary radii, and the winds also impact the shape of the planets. These findings could be used to infer information about the decay of zonal winds and the bulk rotation periods of Uranus and Neptune through future observations.

ASTRONOMICAL JOURNAL (2023)

Article Astronomy & Astrophysics

A New Perspective on the Interiors of Ice-rich Planets: Ice-Rock Mixture Instead of Ice on Top of Rock

Allona Vazan et al.

Summary: The high ice content affects the structure of ice-rich planets, where ice and rock often remain mixed in the interior. Mass loss can cause separation of water and rock, resulting in the formation of a volatile atmosphere.

ASTROPHYSICAL JOURNAL (2022)

Article Astronomy & Astrophysics

Uranus and Neptune are key to understand planets with hydrogen atmospheres

Tristan Guillot

Summary: Uranus and Neptune, the last unexplored planets in the Solar System, are crucial in understanding the atmospheric dynamics and structure of planets with hydrogen atmospheres. Investigating the active atmospheres, temperature, and methane abundance on these planets can provide insights into convection organization in a surface-less atmosphere with heavier condensates, which is essential for not only understanding Uranus and Neptune, but also Jupiter, Saturn, and other exoplanets with hydrogen atmospheres.

EXPERIMENTAL ASTRONOMY (2022)

Article Physics, Multidisciplinary

Superionic Silica-Water and Silica-Hydrogen Compounds in the Deep Interiors of Uranus and Neptune

Hao Gao et al.

Summary: Research shows that silica-water and silica-hydrogen compounds can exist under high pressures. These compounds exhibit superionic behavior under specific conditions within giant planets, shedding light on the formation and evolution of their cores.

PHYSICAL REVIEW LETTERS (2022)

Article Geochemistry & Geophysics

A New Model of Jupiter's Magnetic Field at the Completion of Juno's Prime Mission

J. E. P. Connerney et al.

Summary: A spherical harmonic model of Jupiter's magnetic field is obtained using data from the Juno spacecraft. This model provides a detailed view of the planetary dynamo and shows evidence of advection of the magnetic field by deep zonal winds near the Great Blue Spot.

JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS (2022)

Article Astronomy & Astrophysics

Jupiter's inhomogeneous envelope

Y. Miguel et al.

Summary: This paper presents a Bayesian statistical analysis of Jupiter's interior models, revealing a heavy-element enrichment in the planet's envelope compared to the outer layers. This finding has important implications for the formation of giant planets in our Solar System and beyond.

ASTRONOMY & ASTROPHYSICS (2022)

Article Astronomy & Astrophysics

Possible In Situ Formation of Uranus and Neptune via Pebble Accretion

Claudio Valletta et al.

Summary: This paper simulates the in situ formation of Uranus and Neptune and suggests that they could have formed at their current locations within a short period of time. The simulations also indicate the possibility of additional accumulation of heavy elements through planetesimal accretion and/or giant impacts after their initial formation.

ASTROPHYSICAL JOURNAL (2022)

Article Astronomy & Astrophysics

Ice giant system exploration within ESA's Voyage 2050

Leigh N. Fletcher et al.

Summary: The distant Ice Giants Uranus and Neptune are the least explored environments in our Solar System, with an international partnership mission proposed for the early 2030s. This mission could shape the paradigm for planetary formation throughout our galaxy.

EXPERIMENTAL ASTRONOMY (2022)

Article Geosciences, Multidisciplinary

A Dynamo Simulation Generating Saturn-Like Small Magnetic Dipole Tilts

Rakesh Kumar Yadav et al.

Summary: Saturn's magnetic field is highly axisymmetric, with a very small tilt angle of the magnetic dipole component. Numerical simulations suggest that small dipole tilt values can be realized by introducing spatial heat-flux variation and stably stratified layers on top of an active dynamo layer. This study presents a simplified model that achieves extremely small dipole tilt values without these ad hoc ingredients.

GEOPHYSICAL RESEARCH LETTERS (2022)

Article Astronomy & Astrophysics

Benchmarking the ab initio hydrogen equation of state for the interior structure of Jupiter

S. Mazevet et al.

Summary: This study evaluates the effectiveness of currently available ab initio equations of state (EOSs) in predicting the interior structure of Jupiter and provides suggestions for improvement. By adjusting the free energy parameterization, it identifies the source of discrepancies in previous reports on the internal structure of Jupiter and highlights areas that require special attention when constructing EOSs for giant planets.

ASTRONOMY & ASTROPHYSICS (2022)

Article Astronomy & Astrophysics

Random models for exploring planet compositions I: Uranus as an example

Joshua Podolak et al.

Summary: Modeling the interior of a planet is challenging due to the limited number of measured parameters, thus unable to constrain multiple variables describing the interior structure and composition. In order to better understand the necessary cosmogonic constraints, researchers have developed a code for generating random, monotonic, density distributions consistent with given mass, radius, and moment of inertia requirements, which has been applied to Uranus for validation.

ICARUS (2022)

Article Multidisciplinary Sciences

Miscibility of rock and ice in the interiors of water worlds

Tanja Kovacevic et al.

Summary: Through simulations, we have found that water and enstatite can be completely miscible under extreme conditions, leading to the formation of a mixed layer of rock and water in water worlds.

SCIENTIFIC REPORTS (2022)

Article Astronomy & Astrophysics

Juno Spacecraft Measurements of Jupiter's Gravity Imply a Dilute Core

Burkhard Militzer et al.

Summary: The Juno spacecraft's measurement of Jupiter's gravity field and its harmonics has provided new insights into the planet's interior structure. The study suggests that the small values of certain harmonics can be explained by assuming the presence of a dilute core of heavy elements distributed throughout the planet, along with a new equation of state and wind profiles.

PLANETARY SCIENCE JOURNAL (2022)

Article Astronomy & Astrophysics

The Promise and Limitations of Precision Gravity: Application to the Interior Structure of Uranus and Neptune

Naor Movshovitz et al.

Summary: This study investigates the constraining power of a high-precision measurement of the gravity field for Uranus and Neptune. It assesses the possible deliverables and limitations of such a mission in revealing the structure of the planets and the relative importance of different factors in constraining planetary structure. The study explores various interior density structures that are consistent with hypothetical gravity data by sampling parameterized density profiles. It concludes that while density profiles can be well constrained, uncertainties still exist regarding the relative roles of different components in the deep interior.

PLANETARY SCIENCE JOURNAL (2022)

Article Astronomy & Astrophysics

Mixing of Condensable Constituents with H-He during the Formation and Evolution of Jupiter

David J. J. Stevenson et al.

Summary: Simulations of Jupiter's formation show that the mixing of H-He with denser material entering the planet as solids plays an important role in shaping the planet's composition and internal structure. The simulations reveal the existence of compositional gradients and a hot interior where much of the accretion energy remains trapped.

PLANETARY SCIENCE JOURNAL (2022)

Article Astronomy & Astrophysics

Jupiter's Temperature Structure: A Reassessment of the Voyager Radio Occultation Measurements

Pranika Gupta et al.

Summary: The study electronically digitized all available temperature profiles from Voyager spacecraft to find corrected temperature values at the 1-bar level for Jupiter, showing a difference of up to 4K compared to previously published values. This suggests spatial variability in Jupiter's tropospheric temperatures of up to 7K between latitudes 7 degrees N and 12 degrees S.

PLANETARY SCIENCE JOURNAL (2022)

Article Astronomy & Astrophysics

The Possible Formation of Jupiter from Supersolar Gas

Artyom Aguichine et al.

Summary: This study aims to determine the radial and temporal evolution of Jupiter's atmospheric composition to assess whether it was acquired via the direct accretion of supersolar gases. The model shows that Jupiter's composition can be explained by accreting gases from the protosolar nebula or a mixture of vapors and solids.

PLANETARY SCIENCE JOURNAL (2022)

Article Astronomy & Astrophysics

Combined magnetic and gravity measurements probe the deep zonal flows of the gas giants

E. Galanti et al.

Summary: Recent measurements from the Cassini mission at Saturn and the Juno mission at Jupiter have provided unprecedented accuracy on the gravity and magnetic fields of the gas giants. By combining gravity measurements with magnetic field observations, researchers were able to determine the vertical decay profile of the observed zonal flows on Saturn and Jupiter. The results show that the cloud-level winds extend with little decay until a certain depth, where they rapidly reduce in strength, indicating a possible interaction with the magnetic field in the semiconducting region.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

How planets grow by pebble accretion: III. Emergence of an interior composition gradient

Chris W. Ormel et al.

Summary: During planet formation, pebbles sublimate in the atmosphere leading to a gradual decrease in metallicity in the outer layers of the planet. Pebbles act as the dominant source of opacity, preventing rapid cooling and aiding in the survival of mini-Neptunes in gas-rich disks. Atmospheric recycling is considered the most likely mechanism to stall the growth of planet envelopes.

ASTRONOMY & ASTROPHYSICS (2021)

Article Astronomy & Astrophysics

Latitudinal variation of methane mole fraction above clouds in Neptune's atmosphere from VLT/MUSE-NFM: Limb-darkening reanalysis

Patrick G. J. Irwin et al.

Summary: A reanalysis of visible/near-infrared observations of Neptune made in 2018 with the MUSE instrument at the VLT revealed that previous analysis underestimated retrieval errors and introduced spurious latitudinal variability. The reanalysis incorporated limb-darkening effects and found that a background cloud model can effectively approximate the observed reflectivity spectrum. The study also concluded that the methane mole fraction varies with latitude and confirmed previous findings.

ICARUS (2021)

Article Astronomy & Astrophysics

Thermal evolution of Uranus and Neptune: II. Deep thermal boundary layer

Ludwig Scheibe et al.

Summary: Thermal evolution models of Uranus and Neptune suggest that their luminosities are inconsistent with the classical assumption of an adiabatic interior, with the influence of a thermally conductive boundary layer being a significant factor. Even a thin conductive layer of a few kilometers can greatly affect planetary cooling, resulting in either brighter or fainter appearances compared to the adiabatic case. The models also indicate that Uranus may have been in equilibrium with solar flux for a longer period of time.

ASTRONOMY & ASTROPHYSICS (2021)

Article Astronomy & Astrophysics

Atomic-scale mixing between MgO and H2O in the deep interiors of water-rich planets

Taehyun Kim et al.

Summary: This study reports experimental results on two rock-forming minerals in water at the expected pressure and temperature conditions for water-rich planets. The data indicate selective leaching of MgO, peaking between 20 and 40 GPa and above 1,500 K. The chemical reaction at the deep water-rock interface may lead to high concentrations of MgO in the H2O layer of water-rich planets.

NATURE ASTRONOMY (2021)

Article Astronomy & Astrophysics

The Nature and Composition of Jupiter's Building Blocks Derived from the Water Abundance Measurements by the Juno Spacecraft

Olivier Mousis et al.

Summary: This study uses data from the Juno spacecraft's microwave radiometer and other measurements of elemental abundances in Jupiter to derive the formation conditions, initial composition, and adjustment process of icy solids in Jupiter's envelope. The total mass of volatiles needed in Jupiter's envelope to match observed enrichments ranges from approximately 4.3-39 M (circle plus), depending on the crystallization scenario considered in the protosolar nebula. The mass of heavy elements derived from the fits is found to be compatible with the envelope's metallicity calculated from current interior models.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Multidisciplinary Sciences

Evidence of hydrogen-helium immiscibility at Jupiter-interior conditions

S. Brygoo et al.

Summary: The study reveals the phase behavior of H-He mixtures under Jupiter interior conditions through laser-driven shock compression of H-2-He samples, identifying a region of immiscibility along the Hugoniot. The experimental findings suggest that phase separation affects a large fraction of the interior of Jupiter, about 15% of its radius. This provides microphysical support for models of Jupiter with a layered interior.

NATURE (2021)

Article Astronomy & Astrophysics

A diffuse core in Saturn revealed by ring seismology

Christopher R. Mankovich et al.

Summary: Historically, the best constraints on the internal structures of giant planets have come from measurements of their gravity fields, which are mostly sensitive to the planet's outer regions. However, studies of Saturn's rings have detected waves driven by pulsation modes within the planet, offering independent seismic probes of Saturn's interior. These observations reveal gravity-mode pulsations that indicate a stable region against convection in Saturn's deep interior.

NATURE ASTRONOMY (2021)

Article Astronomy & Astrophysics

Constraining the Effect of Convective Inhibition on the Thermal Evolution of Uranus and Neptune

Steve Markham et al.

Summary: This study examines the effects of condensation on the thermal evolution of Uranus and Neptune, finding that methane condensation can speed up the cooldown time by up to 15%, while water condensation can slow it down by up to 15%. The research also discusses convective inhibition and the importance of considering it when modeling planetary interiors.

PLANETARY SCIENCE JOURNAL (2021)

Article Astronomy & Astrophysics

Thermodynamically Governed Interior Models of Uranus and Neptune

Elizabeth Bailey et al.

Summary: Interior models of Uranus and Neptune suggest possible hydrogen-water immiscibility due to gravitational and magnetic reasoning. The disagreement in ab initio models highlights the difficulty in accurately modeling hydrogen and water from first-principles quantum mechanics. This immiscibility could impact the heat flows and cooling rates of the ice giants.

PLANETARY SCIENCE JOURNAL (2021)

Article Astronomy & Astrophysics

The Role of Early Giant-planet Instability in Terrestrial Planet Formation

David Nesvorny et al.

Summary: The terrestrial planets are believed to have formed by violent collisions of tens of lunar- to Mars-size protoplanets within 200 million years after the dispersal of the protoplanetary gas disk. The rapid formation and radial migration of the solar system giant planets may have influenced the formation of the terrestrial planets.

ASTRONOMICAL JOURNAL (2021)

Article Astronomy & Astrophysics

Explaining the low luminosity of Uranus: a self-consistent thermal and structural evolution

Allona Vazan et al.

ASTRONOMY & ASTROPHYSICS (2020)

Article Astronomy & Astrophysics

Jupiter's heavy-element enrichment expected from formation models

Julia Venturini et al.

ASTRONOMY & ASTROPHYSICS (2020)

Article Geosciences, Multidisciplinary

Jupiter's Gravity Field Halfway Through the Juno Mission

D. Durante et al.

GEOPHYSICAL RESEARCH LETTERS (2020)

Article Astronomy & Astrophysics

The water abundance in Jupiter's equatorial zone

Cheng Li et al.

NATURE ASTRONOMY (2020)

Article Astronomy & Astrophysics

The challenge of forming a fuzzy core in Jupiter

Simon Mueller et al.

ASTRONOMY & ASTROPHYSICS (2020)

Article Astronomy & Astrophysics

Understanding Saturn's interior from the Cassini Grand Finale gravity measurements

Dongdong Ni

ASTRONOMY & ASTROPHYSICS (2020)

Article Multidisciplinary Sciences

Large H2O solubility in dense silica and its implications for the interiors of water-rich planets

Carole Nisr et al.

PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA (2020)

Review Astronomy & Astrophysics

The Deep Composition of Uranus and Neptune from In Situ Exploration and Thermochemical Modeling

Thibault Cavalie et al.

SPACE SCIENCE REVIEWS (2020)

Article Geochemistry & Geophysics

The Range of Jupiter's Flow Structures that Fit the Juno Asymmetric Gravity Measurements

Keren Duer et al.

JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS (2020)

Article Astronomy & Astrophysics

Constraining the depth of the winds on Uranus and Neptune via Ohmic dissipation

Deniz Soyuer et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

Review Astronomy & Astrophysics

Ice Giant Systems: The scientific potential of orbital missions to Uranus and Neptune

Leigh N. Fletcher et al.

PLANETARY AND SPACE SCIENCE (2020)

Article Astronomy & Astrophysics

Evidence for a Dichotomy in the Interior Structures of Jupiter and Saturn from Helium Phase Separation

Christopher R. Mankovich et al.

ASTROPHYSICAL JOURNAL (2020)

Article Astronomy & Astrophysics

Giant Planet Formation Models with a Self-consistent Treatment of the Heavy Elements

Claudio Valletta et al.

ASTROPHYSICAL JOURNAL (2020)

Article Geosciences, Multidisciplinary

Saturn's Deep Atmosnheric Flows Revealed by the Cassini Grand Finale Gravity Measurements

E. Galanti et al.

GEOPHYSICAL RESEARCH LETTERS (2019)

Article Astronomy & Astrophysics

A water budget dichotomy of rocky protoplanets from 26Al-heating

Tim Lichtenberg et al.

NATURE ASTRONOMY (2019)

Article Astronomy & Astrophysics

Effect of non-adiabatic thermal profiles on the inferred compositions of Uranus and Neptune

Morris Podolak et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2019)

Article Astronomy & Astrophysics

Uranus and Neptune missions: A study in advance of the next Planetary Science Decadal Survey

Mark Hofstadter et al.

PLANETARY AND SPACE SCIENCE (2019)

Article Astronomy & Astrophysics

Constraining the initial planetary population in the gravitational instability model

J. Humphries et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2019)

Article Astronomy & Astrophysics

The fate of planetary cores in giant and ice-giant planets

S. Mazevet et al.

ASTRONOMY & ASTROPHYSICS (2019)

Article Astronomy & Astrophysics

Ab initio based equation of state of dense water for planetary and exoplanetary modeling

S. Mazevet et al.

ASTRONOMY & ASTROPHYSICS (2019)

Article Astronomy & Astrophysics

Thermal evolution of Uranus and Neptune I. Adiabatic models

Ludwig Scheibe et al.

ASTRONOMY & ASTROPHYSICS (2019)

Article Astronomy & Astrophysics

Understanding Jupiter's deep interior: the effect of a dilute core

Dongdong Ni

ASTRONOMY & ASTROPHYSICS (2019)

Article Astronomy & Astrophysics

Jupiter formed as a pebble pile around the N2 ice line

A. D. Bosman et al.

ASTRONOMY & ASTROPHYSICS (2019)

Article Multidisciplinary Sciences

Measurement and implications of Saturn's gravity field and ring mass

L. Iess et al.

SCIENCE (2019)

Article Astronomy & Astrophysics

Analysis of Jupiter's Deep Jets Combining Juno Gravity and Time-varying Magnetic Field Measurements

Keren Duer et al.

ASTROPHYSICAL JOURNAL LETTERS (2019)

Article Astronomy & Astrophysics

Models of Saturn's Interior Constructed with an Accelerated Concentric Maclaurin Spheroid Method

B. Militzer et al.

ASTROPHYSICAL JOURNAL (2019)

Article Astronomy & Astrophysics

Jupiter's Composition Suggests its Core Assembled Exterior to the N2 Snowline

Karin Oberg et al.

ASTRONOMICAL JOURNAL (2019)

Article Astronomy & Astrophysics

A New Equation of State for Dense Hydrogen-Helium Mixtures

G. Chabrier et al.

ASTROPHYSICAL JOURNAL (2019)

Article Astronomy & Astrophysics

New Models of Jupiter in the Context of Juno and Galileo

Florian Debras et al.

ASTROPHYSICAL JOURNAL (2019)

Article Astronomy & Astrophysics

Cassini Ring Seismology as a Probe of Saturn's Interior. I. Rigid Rotation

Christopher Mankovich et al.

ASTROPHYSICAL JOURNAL (2019)

Article Astronomy & Astrophysics

First ALMA Millimeter-wavelength Maps of Jupiter, with a Multiwavelength Study of Convection

Imke de Pater et al.

ASTRONOMICAL JOURNAL (2019)

Article Astronomy & Astrophysics

Jupiter's evolution with primordial composition gradients

Allona Vazan et al.

ASTRONOMY & ASTROPHYSICS (2018)

Article Astronomy & Astrophysics

How cores grow by pebble accretion I. Direct core growth

M. G. Brouwers et al.

ASTRONOMY & ASTROPHYSICS (2018)

Article Geosciences, Multidisciplinary

A New Model of Jupiter's Magnetic Field From Juno's First Nine Orbits

J. E. P. Connerney et al.

GEOPHYSICAL RESEARCH LETTERS (2018)

Article Multidisciplinary Sciences

Measurement of Jupiter's asymmetric gravity field

L. Iess et al.

NATURE (2018)

Article Astronomy & Astrophysics

Jupiter's evolution with primordial composition gradients

Allona Vazan et al.

ASTRONOMY & ASTROPHYSICS (2018)

Article Astronomy & Astrophysics

How cores grow by pebble accretion I. Direct core growth

M. G. Brouwers et al.

ASTRONOMY & ASTROPHYSICS (2018)

Article Multidisciplinary Sciences

A complex dynamo inferred from the hemispheric dichotomy of Jupiter's magnetic field

Kimberly M. Moore et al.

NATURE (2018)

Article Multidisciplinary Sciences

Jupiter's atmospheric jet streams extend thousands of kilometres deep

Y. Kaspi et al.

NATURE (2018)

Article Multidisciplinary Sciences

A suppression of differential rotation in Jupiter's deep interior

T. Guillot et al.

NATURE (2018)

Article Astronomy & Astrophysics

The formation of Jupiter by hybrid pebble-planetesimal accretion

Yann Alibert et al.

NATURE ASTRONOMY (2018)

Article Astronomy & Astrophysics

New Formation Models for the Kepler-36 System

Peter Bodenheimer et al.

ASTROPHYSICAL JOURNAL (2018)

Article Geosciences, Multidisciplinary

Comparing Jupiter interior structure models to Juno gravity measurements and the role of a dilute core

S. M. Wahl et al.

GEOPHYSICAL RESEARCH LETTERS (2017)

Article Multidisciplinary Sciences

Age of Jupiter inferred from the distinct genetics and formation times of meteorites

Thomas S. Kruijer et al.

PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA (2017)

Article Astronomy & Astrophysics

Acceleration of Cooling of Ice Giants by Condensation in Early Atmospheres

Kenji Kurosaki et al.

ASTRONOMICAL JOURNAL (2017)

Article Astronomy & Astrophysics

The Fuzziness of Giant Planets' Cores

Ravit Helled et al.

ASTROPHYSICAL JOURNAL LETTERS (2017)

Article Astronomy & Astrophysics

Jupiter's Formation and Its Primordial Internal Structure

Michael Lozovsky et al.

ASTROPHYSICAL JOURNAL (2017)

Article Astronomy & Astrophysics

Jupiter internal structure: the effect of different equations of state

Y. Miguel et al.

ASTRONOMY & ASTROPHYSICS (2016)

Article Astronomy & Astrophysics

Uranus evolution models with simple thermal boundary layers

N. Nettelmann et al.

ICARUS (2016)

Article Astronomy & Astrophysics

Jupiter internal structure: the effect of different equations of state

Y. Miguel et al.

ASTRONOMY & ASTROPHYSICS (2016)

Article Astronomy & Astrophysics

A PRELIMINARY JUPITER MODEL

W. B. Hubbard et al.

ASTROPHYSICAL JOURNAL (2016)

Article Astronomy & Astrophysics

THE ASTEROID BELT AS A RELIC FROM A CHAOTIC EARLY SOLAR SYSTEM

Andre Izidoro et al.

ASTROPHYSICAL JOURNAL (2016)

Article Astronomy & Astrophysics

THE EVOLUTION AND INTERNAL STRUCTURE OF JUPITER AND SATURN WITH COMPOSITIONAL GRADIENTS

A. Vazan et al.

ASTROPHYSICAL JOURNAL (2016)

Article Astronomy & Astrophysics

BAYESIAN EVOLUTION MODELS FOR JUPITER WITH HELIUM RAIN AND DOUBLE-DIFFUSIVE CONVECTION

Christopher Mankovich et al.

ASTROPHYSICAL JOURNAL (2016)

Article Astronomy & Astrophysics

The growth of planets by pebble accretion in evolving protoplanetary discs

Bertram Bitsch et al.

ASTRONOMY & ASTROPHYSICS (2015)

Article Astronomy & Astrophysics

The growth of planets by pebble accretion in evolving protoplanetary discs

Bertram Bitsch et al.

ASTRONOMY & ASTROPHYSICS (2015)

Article Astronomy & Astrophysics

CONVECTION AND MIXING IN GIANT PLANET EVOLUTION

A. Vazan et al.

ASTROPHYSICAL JOURNAL (2015)

Article Astronomy & Astrophysics

Forming the cores of giant planets from the radial pebble flux in protoplanetary discs

M. Lambrechts et al.

ASTRONOMY & ASTROPHYSICS (2014)

Article Astronomy & Astrophysics

AB INITIO EQUATIONS OF STATE FOR HYDROGEN (H-REOS.3) AND HELIUM (He-REOS.3) AND THEIR IMPLICATIONS FOR THE INTERIOR OF BROWN DWARFS

Andreas Becker et al.

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2014)

Article Geosciences, Multidisciplinary

Inferring the depth of the zonal jets on Jupiter and Saturn from odd gravity harmonics

Yohai Kaspi

GEOPHYSICAL RESEARCH LETTERS (2013)

Article Multidisciplinary Sciences

Atmospheric confinement of jet streams on Uranus and Neptune

Yohai Kaspi et al.

NATURE (2013)

Article Geosciences, Multidisciplinary

Layered convection as the origin of Saturn's luminosity anomaly

Jeremy Leconte et al.

NATURE GEOSCIENCE (2013)

Article Materials Science, Multidisciplinary

Hydrogen-helium demixing from first principles: From diamond anvil cells to planetary interiors

Miguel A. Morales et al.

PHYSICAL REVIEW B (2013)

Article Astronomy & Astrophysics

Rapid growth of gas-giant cores by pebble accretion

M. Lambrechts et al.

ASTRONOMY & ASTROPHYSICS (2012)

Article Astronomy & Astrophysics

A new vision of giant planet interiors: Impact of double diffusive convection

J. Leconte et al.

ASTRONOMY & ASTROPHYSICS (2012)

Article Astronomy & Astrophysics

SOLUBILITY OF WATER ICE IN METALLIC HYDROGEN: CONSEQUENCES FOR CORE EROSION IN GAS GIANT PLANETS

H. F. Wilson et al.

ASTROPHYSICAL JOURNAL (2012)

Article Astronomy & Astrophysics

JUPITER MODELS WITH IMPROVED AB INITIO HYDROGEN EQUATION OF STATE (H-REOS.2)

N. Nettelmann et al.

ASTROPHYSICAL JOURNAL (2012)

Article Materials Science, Multidisciplinary

Extended data set for the equation of state of warm dense hydrogen isotopes

P. Loubeyre et al.

PHYSICAL REVIEW B (2012)

Article Physics, Multidisciplinary

Rocky Core Solubility in Jupiter and Giant Exoplanets

Hugh F. Wilson et al.

PHYSICAL REVIEW LETTERS (2012)

Article Astronomy & Astrophysics

INTERIOR MODELS OF URANUS AND NEPTUNE

Ravit Helled et al.

ASTROPHYSICAL JOURNAL (2011)

Article Astronomy & Astrophysics

SELF-CONSISTENT MODEL ATMOSPHERES AND THE COOLING OF THE SOLAR SYSTEM'S GIANT PLANETS

J. J. Fortney et al.

ASTROPHYSICAL JOURNAL (2011)

Article Astronomy & Astrophysics

The haze and methane distributions on Neptune from HST-STIS spectroscopy

Erich Karkoschka et al.

ICARUS (2011)

Article Astronomy & Astrophysics

The phase diagram of water and the magnetic fields of Uranus and Neptune

Ronald Redmer et al.

ICARUS (2011)

Article Astronomy & Astrophysics

Gas giant formation with small cores triggered by envelope pollution by icy planetesimals

Y. Hori et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2011)

Article Materials Science, Multidisciplinary

Laser-shock compression and Hugoniot measurements of liquid hydrogen to 55 GPa

T. Sano et al.

PHYSICAL REVIEW B (2011)

Article Astronomy & Astrophysics

EVIDENCE FROM THE ASTEROID BELT FOR A VIOLENT PAST EVOLUTION OF JUPITER'S ORBIT

Alessandro Morbidelli et al.

ASTRONOMICAL JOURNAL (2010)

Review Astronomy & Astrophysics

The Interior Structure, Composition, and Evolution of Giant Planets

Jonathan J. Fortney et al.

SPACE SCIENCE REVIEWS (2010)

Review Astronomy & Astrophysics

The Chemical Composition of the Sun

Martin Asplund et al.

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 47 (2009)

Article Astronomy & Astrophysics

THE ORBITS OF THE NEPTUNIAN SATELLITES AND THE ORIENTATION OF THE POLE OF NEPTUNE

R. A. Jacobson

ASTRONOMICAL JOURNAL (2009)

Article Astronomy & Astrophysics

DETERMINATION OF THE MINIMUM MASSES OF HEAVY ELEMENTS IN THE ENVELOPES OF JUPITER AND SATURN

Olivier Mousis et al.

ASTROPHYSICAL JOURNAL (2009)

Article Materials Science, Multidisciplinary

Laser-driven single shock compression of fluid deuterium from 45 to 220 GPa

D. G. Hicks et al.

PHYSICAL REVIEW B (2009)

Article Materials Science, Multidisciplinary

Equation of state and phase diagram of water at ultrahigh pressures as in planetary interiors

Martin French et al.

PHYSICAL REVIEW B (2009)

Article Materials Science, Multidisciplinary

Path integral Monte Carlo and density functional molecular dynamics simulations of hot, dense helium

B. Militzer

PHYSICAL REVIEW B (2009)

Article Astronomy & Astrophysics

Ab initio equation of state data for hydrogen, helium, and water and the internal structure of Jupiter

Nadine Nettelmann et al.

ASTROPHYSICAL JOURNAL (2008)

Article Astronomy & Astrophysics

The gravity field of the Saturnian system from satellite observations and spacecraft tracking data

R. A. Jacobson et al.

ASTRONOMICAL JOURNAL (2006)

Article Astronomy & Astrophysics

Numerical dynamo models of Uranus' and Neptune's magnetic fields

Sabine Stanley et al.

ICARUS (2006)

Article Astronomy & Astrophysics

The composition of Jupiter: sign of a (relatively) late formation in a chemically evolved protosolar disc

T Guillot et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2006)

Article Multidisciplinary Sciences

Origin of the orbital architecture of the giant planets of the Solar System

K Tsiganis et al.

NATURE (2005)

Article Astronomy & Astrophysics

Models of giant planet formation with migration and disc evolution

Y Alibert et al.

ASTRONOMY & ASTROPHYSICS (2005)

Article Astronomy & Astrophysics

Shock compression of deuterium and the interiors of Jupiter and Saturn

D Saumon et al.

ASTROPHYSICAL JOURNAL (2004)

Article Astronomy & Astrophysics

Solar system abundances and condensation temperatures of the elements

K Lodders

ASTROPHYSICAL JOURNAL (2003)

Article Astronomy & Astrophysics

Phase separation in giant planets: inhomogeneous evolution of Saturn

JJ Fortney et al.

ICARUS (2003)

Article Astronomy & Astrophysics

Further investigations of random models of Uranus and Neptune

M Podolak et al.

PLANETARY AND SPACE SCIENCE (2000)