Results 41 to 50 of about 46,669 (261)
Nightside condensation of iron in an ultra-hot giant exoplanet [PDF]
Ultrahot giant exoplanets receive thousands of times Earth’s insolation1,2. Their high-temperature atmospheres (greater than 2,000 kelvin) are ideal laboratories for studying extreme planetary climates and chemistry3–5. Daysides are predicted to be cloud-
D. Ehrenreich +96 more
semanticscholar +1 more source
Chemical Abundances for 25 JWST Exoplanet Host Stars with KeckSpec [PDF]
Using a data-driven machine learning tool we report T eff, log(g) , vsin(i) , and elemental abundances for 15 elements (C, N, O, Na, Mg, Al, Si, Ca, Ti, V, Cr, Mn, Fe, Ni, Y) for a sample of 25 exoplanet host stars targeted by JWST's first year of ...
A. Polanski +4 more
semanticscholar +1 more source
Exoplanet imaging data challenge: benchmarking the various image processing methods for exoplanet detection [PDF]
The Exoplanet Imaging Data Challenge is a community-wide effort meant to offer a platform for a fair and common comparison of image processing methods designed for exoplanet direct detection. For this purpose, it gathers on a dedicated repository (Zenodo)
Desgrange, Célia +81 more
core +1 more source
Efficient metal emissions in the upper atmospheres of close-in exoplanets
Atmospheric escape is a key process controlling the long term evolution of planets. Radiative cooling competes for energy against atmospheric escape in planetary upper atmospheres.
Lei Liu, Feng Tian
doaj +1 more source
In the search for life on other planets, the presence of photosynthetic surface vegetation may be detectable from the colors of light it reflects. On the modern Earth, this spectral reflectance is characterized by a steep increase in reflectance between ...
Owen R. Lehmer +5 more
doaj +1 more source
Silicate clouds and a circumplanetary disk in the YSES-1 exoplanet system [PDF]
Young exoplanets provide an important link between understanding planet formation and atmospheric evolution1. Direct imaging spectroscopy allows us to infer the properties of young, wide-orbit, giant planets with high signal-to-noise ratio.
K. Hoch +28 more
semanticscholar +1 more source
The growing database of exoplanets has shown us the statistical characteristics of various exoplanet populations, providing insight towards their origins.
Jonathan H. Jiang +4 more
doaj +1 more source
Effect of Laboratory Reagents for Cleaning Modern Contamination on the δ<sup>15</sup>N Integrity of Nitrogen-Poor Samples. [PDF]
ABSTRACT Rationale Nitrogen isotope values have been widely used for tracing ancient biogeochemical processes, but contaminant‐sensitive materials, such as Precambrian sedimentary rocks, meteorites, or returned extraterrestrial samples, often have low nitrogen levels and are thus vulnerable to modern organic contamination.
Bubphamanee K, Schauer A, Buick R.
europepmc +2 more sources
A high internal heat flux and large core in a warm Neptune exoplanet [PDF]
Interactions between exoplanetary atmospheres and internal properties have long been proposed to be drivers of the inflation mechanisms of gaseous planets and apparent atmospheric chemical disequilibrium conditions1.
L. Welbanks +18 more
semanticscholar +1 more source
Early Release Science of the exoplanet WASP-39b with JWST NIRSpec G395H [PDF]
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

