Results 31 to 40 of about 16,468 (216)
Sulfur-driven haze formation in warm CO2-rich exoplanet atmospheres [PDF]
Sulfur gases significantly affect the photochemistry of planetary atmospheres in our Solar System, and are expected to be important components in exoplanet atmospheres. However, sulfur photochemistry in the context of exoplanets is poorly understood due to a lack of chemical-kinetics information for sulfur species under relevant conditions.
Chao He +10 more
openalex +7 more sources
Set to Music, Exoplanets Reveal Insights on Their Formation
Sonification hints at how some Kepler planets may have been configured in the late stages of their development.
Nola Redd
openalex +2 more sources
Lithium abundances in exoplanet host stars as test of planetary formation scenarii [PDF]
Following the observations of Israelian et al. 2004, we compare different evolutionary models in order to study the lithium destruction processes and the planetary formation scenarii.
M. Castro, O. Richard, S. Vauclair
openalex +8 more sources
Atmospheric signatures of giant exoplanet formation by pebble accretion [PDF]
Atmospheric chemical abundances of giant planets lead to important constraints on planetary formation and migration. Studies have shown that giant planets that migrate through the protoplanetary disc can accrete substantial amounts of oxygen-rich planetesimals, leading to supersolar metallicities in the envelope and solar or subsolar C/O ratios. Pebble
Madhusudhan, Nikku +3 more
openaire +4 more sources
Planet Formation Theory in the Era of ALMA and Kepler: from Pebbles to Exoplanets [PDF]
38 pages, 13 figures, review chapter accepted to Protostars and Planets VII, editors: Shu-ichiro Inutsuka, Yuri Aikawa, Takayuki Muto, Kengo Tomida, and Motohide Tamura, corrected label in Fig ...
Drazkowska, Joanna +9 more
openaire +3 more sources
THE FORMATION OF URANUS AND NEPTUNE: CHALLENGES AND IMPLICATIONS FOR INTERMEDIATE-MASS EXOPLANETS [PDF]
In this paper we investigate the formation of Uranus and Neptune, according to the core-nucleated accretion model, considering formation locations ranging from 12 to 30 AU from the Sun, and with various disk solid-surface densities and core accretion rates.
Ravit Helled, Peter Bodenheimer
openaire +3 more sources
A giant exoplanet orbiting a very-low-mass star challenges planet formation models [PDF]
A small star hosts a big planet M dwarfs, the most common type of star, are low-mass objects that emit most of their faint light in the near-infrared, making it difficult to detect any orbiting exoplanets. Morales et al.
J. C. Morales +99 more
openalex +11 more sources
Accreting protoplanets are windows into planet formation processes, and high-contrast differential imaging is an effective way to identify them. We report results from the Giant Accreting Protoplanet Survey (GAPlanetS), which collected H α differential ...
Katherine B. Follette +23 more
doaj +1 more source
Ranges of Atmospheric Mass and Composition of Super Earth Exoplanets [PDF]
Terrestrial-like exoplanets may obtain atmospheres from three primary sources: Capture of nebular gases, degassing during accretion, and degassing from subsequent tectonic activity.
Burbine T. H. +5 more
core +1 more source
SPECULOOS exoplanet search and its prototype on TRAPPIST [PDF]
One of the most significant goals of modern science is establishing whether life exists around other suns. The most direct path towards its achievement is the detection and atmospheric characterization of terrestrial exoplanets with potentially habitable
A Burrows +78 more
core +1 more source

