Results 91 to 100 of about 2,900,879 (209)
TOI-836 is a ∼2–3 Gyr K dwarf with an inner super Earth ( R = 1.7 R _⊕ , P = 3.8 days) and an outer mini-Neptune ( R = 2.6 R _⊕ , P = 8.6 days). JWST/NIRSpec 2.8–5.2 μ m transmission spectra are flat for both planets.
Michael Zhang +15 more
doaj +1 more source
Predicting Nitrogen Isotope Fractionation in Nitrate Deposition on Early Mars
Abstract Noachian and early Hesperian Mars were likely warm and wet, with an atmosphere abundant in molecular nitrogen. The recent discovery of nitrate deposits in the Yellowknife Bay mudstones at Gale Crater confirm the existence of nitrogen oxides (NOX) on Noachian Mars. The processes responsible for the production of these nitrates would fractionate
J. Shawcross +4 more
wiley +1 more source
Evolution of Atmospheric Composition in Giant Exoplanets with Diluted Cores
Transmission spectroscopy has reported sub-solar C/O ratios (
Matsuo, Hiroki +2 more
openaire +1 more source
On the Detection of Low‐Frequency Planetary Radio Emission With an Orbiting Interferometer
Abstract The magnetized planets of the outer Solar System produce kilometric radio emissions at very low frequencies (<1 ${< } 1\,$MHz). They reveal the planetary magnetic dynamics and their interaction with the solar wind. Those radio emissions can also serve as a proxy for interplanetary space weather monitoring.
E. Rouillé +4 more
wiley +1 more source
Overcast Mornings and Clear Evenings in Hot Jupiter Exoplanet Atmospheres
Aerosols are an old topic in the young field of exoplanet atmospheres. Understanding what they are, how they form, and where they go has long provided a fertile playground for theorists.
Guangwei Fu +12 more
doaj +1 more source
Advancing Heliophysics and Space Weather Modeling Through Open Science
Abstract We present a community‐wide effort to develop a strategy and action plan to advance heliophysics and space weather modeling through open science. While open science has the potential to enhance the quality and pace of scientific discovery, its application to scientific modeling requires more careful consideration regarding open data and open ...
C. Corti +87 more
wiley +1 more source
The Compositions of the HR 8799 Planets Reflect Accretion of Both Solids and Metal-enriched Gas
With four giant planets ( m ∼ 5 M _Jup −10 M _Jup , T _eff ∼ 900–1200 K) orbiting between 15 and 70 au, HR 8799 provides an unparalleled test bed for studying giant planet formation and probing compositional trends across the protoplanetary disk.
Jerry W. Xuan +26 more
doaj +1 more source
The Role of Planetary Rotation in Polar Cusp Localization
Abstract Juno observations have revealed that Jupiter's polar cusps are displaced toward dusk and even the nightside, contradicting the Earth‐derived paradigm that is confined to narrower ranges near noon. These findings underscore the overlooked influence of planetary rotation on magnetospheric dynamics, exposing a critical gap in current theoretical ...
Junjie Chen +9 more
wiley +1 more source
Changes in atmospheric composition
S.181-198This group report summarizes evidences for changes in atmospheric composition during various periods of earth history as documented in sedimentary rocks, ice cores, lake and marine sediments, tree rings, moisture records, and ...
Stuiver, M. +13 more
core +1 more source
Characterization of Rocky Exoplanet Atmospheres from Lyα Transit Observations
Ly α transit observations are a powerful tool for probing hydrogen escape from exoplanets, but to date all Ly α transits of rocky exoplanets have yielded nondetections.
Grace Bischof +3 more
doaj +1 more source

