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Astrochemistry and compositions of planetary systems
Planets form and obtain their compositions in disks of gas and dust around young stars. The
chemical compositions of these planet-forming disks regulate all aspects of planetary …
chemical compositions of these planet-forming disks regulate all aspects of planetary …
Atmospheres of rocky exoplanets
Rocky planets are common around other stars, but their atmospheric properties remain
largely unconstrained. Thanks to a wealth of recent planet discoveries and upcoming …
largely unconstrained. Thanks to a wealth of recent planet discoveries and upcoming …
The California-Kepler survey. III. A gap in the radius distribution of small planets
The size of a planet is an observable property directly connected to the physics of its
formation and evolution. We used precise radius measurements from the California-Kepler …
formation and evolution. We used precise radius measurements from the California-Kepler …
The California-Kepler survey. VII. Precise planet radii leveraging Gaia DR2 reveal the stellar mass dependence of the planet radius gap
The distribution of planet sizes encodes details of planet formation and evolution. We
present the most precise planet size distribution to date based on Gaia parallaxes, Kepler …
present the most precise planet size distribution to date based on Gaia parallaxes, Kepler …
Formation of planetary systems by pebble accretion and migration-How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode
Super-Earths–planets with sizes between the Earth and Neptune–are found in tighter orbits
than that of the Earth around more than one third of main sequence stars. It has been …
than that of the Earth around more than one third of main sequence stars. It has been …
Compositional imprints in density–distance–time: a rocky composition for close-in low-mass exoplanets from the location of the valley of evaporation
We use an end-to-end model of planet formation, thermodynamic evolution, and
atmospheric escape to investigate how the statistical imprints of evaporation depend on the …
atmospheric escape to investigate how the statistical imprints of evaporation depend on the …
Evolution of the radius valley around low-mass stars from Kepler and K2
We present calculations of the occurrence rate of small close-in planets around low-mass
dwarf stars using the known planet populations from the Kepler and K2 missions. Applying …
dwarf stars using the known planet populations from the Kepler and K2 missions. Applying …
Make super-Earths, not Jupiters: Accreting nebular gas onto solid cores at 0.1 AU and beyond
Close-in super-Earths having radii 1–4 R⊕ may possess hydrogen atmospheres comprising
a few percent by mass of their rocky cores. We determine the conditions under which such …
a few percent by mass of their rocky cores. We determine the conditions under which such …
Magma ocean, water, and the early atmosphere of Venus
The current state and surface conditions of the Earth and its twin planet Venus are drastically
different. Whether these differences are directly inherited from the earliest stages of …
different. Whether these differences are directly inherited from the earliest stages of …
Silicon isotope constraints on terrestrial planet accretion
Understanding the nature and origin of the precursor material to terrestrial planets is key to
deciphering the mechanisms and timescales of planet formation. Nucleosynthetic variability …
deciphering the mechanisms and timescales of planet formation. Nucleosynthetic variability …