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The Water–Ammonia Phase Diagram up to 300 MPa: Application to Icy Satellites
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Large Ocean Worlds with High-Pressure Ices
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The composition of the Earth
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Abundances of the elements: Meteoritic and solar
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Some properties of the pressure—entropy diagram
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Is the mantle chemically stratified? Insights from sound velocity modeling and isotope evolution of an early magma ocean
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Constraining the equation of state of fluid H2O to 80 GPa using the melting curve, bulk modulus, and thermal expansivity of Ice VII
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July 2004 |
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Impacts onto H2O ice: Scaling laws for melting, vaporization, excavation, and final crater size
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August 2011 |
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Coherent thermodynamic model for solid, liquid and gas phases of elements and simple compounds in wide ranges of pressure and temperature
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June 2018 |
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Superionic Phases of the 1:1 Water–Ammonia Mixture
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October 2015 |
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The Freezing Point Curve of the System Water-Ammonia
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August 1924 |
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Holistic Approach for Studying Planetary Hydrospheres: Gibbs Representation of Ices Thermodynamics, Elasticity, and the Water Phase Diagram to 2,300 MPa
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Silicate Melting and Vaporization During Rocky Planet Formation
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The ammonia-water phase diagram and its implications for icy satellites
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January 1987 |
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Elasticity and constitution of the Earth's interior
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June 1952 |
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Abrupt climate transition of icy worlds from snowball to moist or runaway greenhouse
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Experimental evidence for superionic water ice using shock compression
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February 2018 |
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Nanosecond X-ray diffraction of shock-compressed superionic water ice
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May 2019 |
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Ab initio based equation of state of dense water for planetary and exoplanetary modeling
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January 2019 |
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Planetary evolution with atmospheric photoevaporation
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June 2020 |
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Revisited mass-radius relations for exoplanets below 120 M ⊕
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February 2020 |
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AQUA: a collection of H 2 O equations of state for planetary models
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November 2020 |
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The nature of the radius valley
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October 2020 |
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A planetary system with two transiting mini-Neptunes near the radius valley transition around the bright M dwarf TOI-776
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January 2021 |
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Six transiting planets and a chain of Laplace resonances in TOI-178
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May 2021 |
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Star-planet interactions
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July 2021 |
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A sub-Neptune and a non-transiting Neptune-mass companion unveiled by ESPRESSO around the bright late-F dwarf HD 5278 (TOI-130)
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April 2021 |
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Thermodynamic model for water and high-pressure ices up to 2.2GPa and down to the metastable domain
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September 2007 |
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Dissociative melting of ice VII at high pressure
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March 2009 |
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Thermodynamic data and modeling of the water and ammonia-water phase diagrams up to 2.2 GPa for planetary geophysics
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October 2010 |
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Equation of state and phase diagram of ammonia at high pressures from ab initio simulations
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June 2013 |
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Equations of state of ice VI and ice VII at high pressure and high temperature
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September 2014 |
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Free energy models for ice VII and liquid water derived from pressure, entropy, and heat capacity relations
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August 2017 |
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Proton dynamics and the phase diagram of dense water ice
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June 2018 |
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A Helmholtz Free Energy Formulation of the Thermodynamic Properties of the Mixture {Water + Ammonia}
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The thermodynamics of melting of simple substances
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May 1975 |
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Growth model interpretation of planet size distribution
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April 2019 |
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Large H 2 O solubility in dense silica and its implications for the interiors of water-rich planets
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April 2020 |
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The 142 Nd/ 144 Nd variations in mantle-derived rocks provide constraints on the stirring rate of the mantle from the Hadean to the present
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June 2020 |
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Radius and Structure Models of the First Super‐Earth Planet
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February 2007 |
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Detailed Models of Super‐Earths: How Well Can We Infer Bulk Properties?
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August 2007 |
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A Detailed Model Grid for Solid Planets from 0.1 through 100 Earth Masses
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March 2013 |
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The NASA Exoplanet Archive: Data and Tools for Exoplanet Research
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August 2013 |
The K2 Mission: Characterization and Early Results
- Howell, Steve B.; Sobeck, Charlie; Haas, Michael
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Publications of the Astronomical Society of the Pacific, Vol. 126, Issue 938
https://doi.org/10.1086/676406
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April 2014 |
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Ab Initio Equation of State for Hydrogen-Helium Mixtures with Recalibration of the Giant-Planet Mass-Radius Relation
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August 2013 |
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STRUCTURE AND DYNAMICS OF COLD WATER SUPER-EARTHS: THE CASE OF OCCLUDED CH 4 AND ITS OUTGASSING
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August 2014 |
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AB INITIO EQUATIONS OF STATE FOR HYDROGEN (H-REOS.3) AND HELIUM (He-REOS.3) AND THEIR IMPLICATIONS FOR THE INTERIOR OF BROWN DWARFS
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January 2014 |
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Thermodynamically based melting-curve equation
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January 1995 |
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Formation of planetary populations – III. Core composition and atmospheric evaporation
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July 2020 |
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Signatures of the core-powered mass-loss mechanism in the exoplanet population: dependence on stellar properties and observational predictions
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February 2020 |
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An unusually low density ultra-short period super-Earth and three mini-Neptunes around the old star TOI-561
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December 2020 |
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Caught in the act: core-powered mass-loss predictions for observing atmospheric escape
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April 2021 |
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Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valley
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August 2021 |
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A variable polytrope index applied to planet and material models
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July 2015 |
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Survival function analysis of planet size distribution with Gaia Data Release 2 updates
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July 2018 |
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An asteroseismic view of the radius valley: stripped cores, not born rocky
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July 2018 |
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Core-powered mass-loss and the radius distribution of small exoplanets
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February 2018 |
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The Ice Cap Zone: A Unique Habitable Zone for Ocean Worlds
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March 2018 |
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Sculpting the valley in the radius distribution of small exoplanets as a by-product of planet formation: the core-powered mass-loss mechanism
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May 2019 |
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Examining the radius valley: a machine-learning approach
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May 2019 |
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Effects of magnetic fields on the location of the evaporation valley for low-mass exoplanets
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September 2019 |
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Testing exoplanet evaporation with multitransiting systems
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December 2019 |
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EUV irradiation of exoplanet atmospheres occurs on Gyr time-scales
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November 2020 |
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Finite Elastic Strain of Cubic Crystals
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June 1947 |
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Isentropic compression of hydrogen: Probing conditions deep in planetary interiors
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July 2013 |
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Ionic and superionic phases in ammonia dihydrate N H 3 · 2 H 2 O under high pressure
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April 2017 |
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Bulk moduli and equations of state of ice VII and ice VIII
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May 2017 |
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Superionic-Superionic Phase Transitions in Body-Centered Cubic H 2 O Ice
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September 2016 |
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Metallization of Shock-Compressed Liquid Ammonia
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January 2021 |
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Dynamic Ionization of Water under Extreme Conditions
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April 2005 |
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Homogeneous studies of transiting extrasolar planets - IV. Thirty systems with space-based light curves: Studies of transiting extrasolar planets - IV
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September 2011 |
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Transiting Exoplanet Survey Satellite
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October 2014 |
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Kepler Planet-Detection Mission: Introduction and First Results
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January 2010 |
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Superionic and Metallic States of Water and Ammonia at Giant Planet Conditions
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January 1999 |
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How to Characterize Habitable Worlds and Signs of Life
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August 2017 |
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The Chemical Composition of the Sun
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September 2009 |
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Nucleosynthesis
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December 1984 |
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Water, in the Liquid and Five Solid Forms, under Pressure
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January 1912 |
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March 2016 |
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The California- Kepler Survey. III. A Gap in the Radius Distribution of Small Planets
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August 2017 |
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The California- Kepler Survey. IV. Metal-rich Stars Host a Greater Diversity of Planets
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January 2018 |
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Material Properties for the Interiors of Massive Giant Planets and Brown Dwarfs
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September 2018 |
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The California- Kepler Survey. VII. Precise Planet Radii Leveraging Gaia DR2 Reveal the Stellar Mass Dependence of the Planet Radius Gap
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November 2018 |
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Evolution of the Radius Valley around Low-mass Stars from Kepler and K2
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April 2020 |
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A Pair of TESS Planets Spanning the Radius Valley around the Nearby Mid-M Dwarf LTT 3780
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June 2020 |
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TOI-1235 b: A Keystone Super-Earth for Testing Radius Valley Emergence Models around Early M Dwarfs
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June 2020 |
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The Gaia–Kepler Stellar Properties Catalog. II. Planet Radius Demographics as a Function of Stellar Mass and Age
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August 2020 |
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Transits of Known Planets Orbiting a Naked-eye Star
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August 2020 |
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TOI 122b and TOI 237b: Two Small Warm Planets Orbiting Inactive M Dwarfs Found by TESS
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December 2020 |
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The TESS-Keck Survey. II. An Ultra-short-period Rocky Planet and Its Siblings Transiting the Galactic Thick-disk Star TOI-561
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January 2021 |
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Evolution of the Exoplanet Size Distribution: Forming Large Super-Earths Over Billions of Years
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May 2021 |
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K2-79b and K2-222b: Mass Measurements of Two Small Exoplanets with Periods beyond 10 days that Overlap with Periodic Magnetic Activity Signals
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January 2022 |
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The Abundance of Atmospheric CO2in Ocean Exoplanets: a Novel CO2Deposition Mechanism
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March 2017 |
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H-atmospheres of Icy Super-Earths Formed In Situ in the Outer Solar System: An Application to a Possible Planet Nine
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April 2017 |
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Planetary Ices and the Linear Mixing Approximation
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October 2017 |
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A New Desalination Pump Helps Define the pH of Ocean Worlds
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April 2018 |
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Revised Radii of Kepler Stars and Planets Using Gaia Data Release 2
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October 2018 |
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A New Equation of State for Dense Hydrogen–Helium Mixtures
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February 2019 |
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Mass and Mass Scalings of Super-Earths
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March 2019 |
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A Spectroscopic Analysis of the California-Kepler Survey Sample. I. Stellar Parameters, Planetary Radii, and a Slope in the Radius Gap
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April 2019 |
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The Sub-Neptune Desert and Its Dependence on Stellar Type: Controlled by Lifetime X-Ray Irradiation
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April 2019 |
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The Equation of State of MH-III: A Possible Deep CH 4 Reservoir in Titan, Super-Titan Exoplanets, and Moons
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September 2019 |
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Atmosphere Origins for Exoplanet Sub-Neptunes
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March 2020 |
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Primordial Radius Gap and Potentially Broad Core Mass Distributions of Super-Earths and Sub-Neptunes
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February 2021 |
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Planetary Candidates Observed by Kepler . VIII. A Fully Automated Catalog with Measured Completeness and Reliability Based on Data Release 25
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April 2018 |
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Scaling K2. I. Revised Parameters for 222,088 K2 Stars and a K2 Planet Radius Valley at 1.9 R ⊕
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Superabundance of Exoplanet Sub-Neptunes Explained by Fugacity Crisis
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December 2019 |
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Irradiated Ocean Planets Bridge Super-Earth and Sub-Neptune Populations
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June 2020 |
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Bridging the Planet Radius Valley: Stellar Clustering as a Key Driver for Turning Sub-Neptunes into Super-Earths
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Water on Hot Rocky Exoplanets
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March 2021 |
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Exoplanet Radius Gap Dependence on Host Star Type
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December 2017 |