Astrochemistry and compositions of planetary systems
KI Öberg, EA Bergin - Physics Reports, 2021 - Elsevier
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 …
[HTML][HTML] Revelations on Jupiter's formation, evolution and interior: Challenges from Juno results
The Juno mission has revolutionized and challenged our understanding of Jupiter. As Juno
transitioned into its extended mission, we review the major findings of Jupiter's internal …
transitioned into its extended mission, we review the major findings of Jupiter's internal …
Early Release Science of the exoplanet WASP-39b with JWST NIRCam
Measuring the metallicity and carbon-to-oxygen (C/O) ratio in exoplanet atmospheres is a
fundamental step towards constraining the dominant chemical processes at work and, if in …
fundamental step towards constraining the dominant chemical processes at work and, if in …
A solar C/O and sub-solar metallicity in a hot Jupiter atmosphere
Measurements of the atmospheric carbon (C) and oxygen (O) relative to hydrogen (H) in hot
Jupiters (relative to their host stars) provide insight into their formation location and …
Jupiters (relative to their host stars) provide insight into their formation location and …
Temperature-pressure phase diagram of confined monolayer water/ice at first-principles accuracy with a machine-learning force field
Understanding the phase behaviour of nanoconfined water films is of fundamental
importance in broad fields of science and engineering. However, the phase behaviour of the …
importance in broad fields of science and engineering. However, the phase behaviour of the …
Planet formation theory in the era of ALMA and Kepler: from pebbles to exoplanets
J Drazkowska, B Bitsch, M Lambrechts… - arXiv preprint arXiv …, 2022 - arxiv.org
Our understanding of planet formation has been rapidly evolving in recent years. The
classical planet formation theory, developed when the only known planetary system was our …
classical planet formation theory, developed when the only known planetary system was our …
A comparative study of atmospheric chemistry with VULCAN
We present an update of the open-source photochemical kinetics code VULCAN to include
C–H–N–O–S networks and photochemistry. The additional new features are advection …
C–H–N–O–S networks and photochemistry. The additional new features are advection …
Where is the water? Jupiter-like C/H ratio but strong H2O depletion found on τ Boötis b using SPIRou
S Pelletier, B Benneke, A Darveau-Bernier… - The Astronomical …, 2021 - iopscience.iop.org
The present-day envelope of gaseous planets is a relic of how these giant planets originated
and evolved. Measuring their elemental composition therefore presents a powerful …
and evolved. Measuring their elemental composition therefore presents a powerful …
Water activity in Venus's uninhabitable clouds and other planetary atmospheres
The recent suggestion of phosphine in Venus's atmosphere has regenerated interest in the
idea of life in clouds. However, such analyses usually neglect the role of water activity, which …
idea of life in clouds. However, such analyses usually neglect the role of water activity, which …
Jupiter's inhomogeneous envelope
Context. While Jupiter's massive gas envelope consists mainly of hydrogen and helium, the
key to understanding Jupiter's formation and evolution lies in the distribution of the …
key to understanding Jupiter's formation and evolution lies in the distribution of the …