Results 31 to 40 of about 4,598,556 (263)

Early Release Science of the exoplanet WASP-39b with JWST NIRSpec G395H [PDF]

open access: yesNature, 2022
Measuring the abundances of carbon and oxygen in exoplanet atmospheres is considered a crucial avenue for unlocking the formation and evolution of exoplanetary systems^ 1 , 2 .
L. Alderson   +91 more
semanticscholar   +1 more source

Let’s Sweep: The Effect of Evolving J 2 on the Resonant Structure of a Three-planet System

open access: yesThe Astrophysical Journal, 2023
Short and ultrashort period planets are peculiar types of exoplanets with periods as short as a few days or less. Although it is challenging to detect them, already several have been observed, with many additional candidates.
Thea H. Faridani   +3 more
doaj   +1 more source

Identification of carbon dioxide in an exoplanet atmosphere [PDF]

open access: yesNature, 2022
Carbon dioxide (CO_2) is a key chemical species that is found in a wide range of planetary atmospheres. In the context of exoplanets, CO_2 is an indicator of the metal enrichment (that is, elements heavier than helium, also called ‘metallicity’)^ 1 – 3 ,
The Jwst Transiting Exoplanet Community Early Release Ahrer   +363 more
semanticscholar   +1 more source

A Geologic Si‐O‐C Pathway to Incorporate Carbon in Silicates

open access: yesGeophysical Monograph Series, Page 47-54., 2020

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

Early Release Science of the exoplanet WASP-39b with JWST NIRCam [PDF]

open access: yesNature, 2022
Time-series observations from the JWST of the transiting exoplanet WASP-39b show gaseous water in the planet’s atmosphere and place an upper limit on the abundance of methane.
E. Ahrer   +98 more
semanticscholar   +1 more source

A Comparison of the Composition of Planets in Single-planet and Multiplanet Systems Orbiting M dwarfs

open access: yesThe Astronomical Journal, 2023
We investigate and compare the composition of M-dwarf planets in systems with only one known planet (“singles”) to those residing in multiplanet systems (“multis”) and the fundamental properties of their host stars.
Romy Rodríguez Martínez   +6 more
doaj   +1 more source

ELemental abundances of Planets and brown dwarfs Imaged around Stars (ELPIS). I. Potential Metal Enrichment of the Exoplanet AF Lep b and a Novel Retrieval Approach for Cloudy Self-luminous Atmospheres [PDF]

open access: yesAstronomical Journal, 2023
AF Lep A+b is a remarkable planetary system hosting a gas-giant planet that has the lowest dynamical mass among directly imaged exoplanets. We present an in-depth analysis of the atmospheric composition of the star and planet to probe the planet’s ...
Z. Zhang 张   +12 more
semanticscholar   +1 more source

RESONANCES OF MULTIPLE EXOPLANETS AND IMPLICATIONS FOR THEIR FORMATION [PDF]

open access: yesThe Astrophysical Journal, 2014
5 pages, 5 figures, accepted for publication in ApJ ...
Xiaojia Zhang   +4 more
openaire   +4 more sources

Interpreting the Atmospheric Composition of Exoplanets: Sensitivity to Planet Formation Assumptions [PDF]

open access: yesThe Astrophysical Journal, 2022
Abstract Constraining planet formation based on the atmospheric composition of exoplanets is a fundamental goal of the exoplanet community. Existing studies commonly try to constrain atmospheric abundances, or to analyze what abundance patterns a given description of planet formation predicts.
Paul Mollière   +15 more
openaire   +5 more sources

Exoplanet interior retrievals: core masses and metallicities from atmospheric abundances [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2023
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

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