Vanadium oxide and a sharp onset of cold-trapping on a giant exoplanet [PDF]
The abundance of refractory elements in giant planets can provide key insights into their formation histories^ 1 . Owing to the low temperatures of the Solar System giants, refractory elements condense below the cloud deck, limiting sensing capabilities ...
S. Pelletier +17 more
semanticscholar +1 more source
True Polar Wander of Lava Worlds
As one of the most detectable types of terrestrial planets, lava worlds are highly prioritized targets for exoplanet atmosphere characterization since their atmospheres may reveal what they are made of and how.
Wanying Kang, Francis Nimmo, Feng Ding
doaj +1 more source
Evolution of exoplanets and their parent stars [PDF]
Studying exoplanets with their parent stars is crucial to understand their population, formation and history. We review some of the key questions regarding their evolution with particular emphasis on giant gaseous exoplanets orbiting close to solar-type stars.
Guillot, Tristan +4 more
openaire +3 more sources
A Geologic Si‐O‐C Pathway to Incorporate Carbon in Silicates
This book is Open Access. A digital copy can be downloaded for free from Wiley Online Library.
Explores the behavior of carbon in minerals, melts, and fluids under extreme conditions
Carbon trapped in diamonds and carbonate-bearing rocks in subduction zones are examples of the continuing exchange of substantial carbon ...
Alexandra Navrotsky +2 more
wiley +2 more sources
ExoMDN: Rapid characterization of exoplanet interior structures with Mixture Density Networks [PDF]
Characterizing the interior structure of exoplanets is essential for understanding their diversity, formation, and evolution. As the interior of exoplanets is inaccessible to observations, an inverse problem must be solved, where numerical structure ...
Philipp Baumeister, N. Tosi
semanticscholar +1 more source
Exoplanet interior retrievals: core masses and metallicities from atmospheric abundances [PDF]
The mass and distribution of metals in the interiors of exoplanets are essential for constraining their formation and evolution processes. Never the less, with only masses and radii measured, the determination of exoplanet interior structures is ...
Sanne Bloot +3 more
semanticscholar +1 more source
Warm giant exoplanet characterisation: current state, challenges and outlook [PDF]
The characterisation of giant exoplanets is crucial to constrain giant planet formation and evolution theory and for putting the solar-system’s giant planets in perspective. Typically, mass-radius (M-R) measurements of moderately irradiated warm Jupiters
S. Müller, R. Helled
semanticscholar +1 more source
Thermal and Orbital Evolution of Low-mass Exoplanets [PDF]
Abstract The thermal, orbital, and rotational dynamics of tidally loaded exoplanets are interconnected by intricate feedback. The rheological structure of the planet determines its susceptibility to tidal deformation and, as a consequence, participates in shaping its orbit.
Michaela Walterová, Marie Běhounková
openaire +2 more sources
Surrounded by Giants: Habitable Zone Stability Within the HD 141399 System
The search for exoplanets has revealed a diversity of planetary system architectures, the vast majority of which diverge significantly from the template of the solar system.
Stephen R. Kane
doaj +1 more source
Extreme weather variability on hot rocky exoplanet 55 Cancri e explained by magma temperature–cloud feedback [PDF]
Kaitlyn Loftus +2 more
exaly +2 more sources

