Results 91 to 100 of about 6,508 (165)
Atmospheric Waves Driving Variability and Cloud Modulation on a Planetary-mass Object
Planetary-mass objects and brown dwarfs at the transition ( T _eff ∼ 1300 K) from relatively red L dwarfs to bluer mid-T dwarfs show enhanced spectrophotometric variability.
Michael K. Plummer +4 more
doaj +1 more source
Recent studies revealed viewing-angle-dependent color and spectral trends in brown dwarfs, as well as long-term photometric variability (∼100 hr). The origins of these trends are yet unexplained.
Nguyen Fuda, Dániel Apai
doaj +1 more source
Planetary Habitability Under the Light of a Rapidly Changing Star
Planetary atmospheric energy budgets primarily depend on stellar incident flux. However, stellar variability can have major consequences for the evolution of planetary climates. In this work, we evaluate how stellar variability influences the equilibrium
Tara Fetherolf +5 more
doaj +1 more source
Fully fluorinated non-carbon compounds NF3 and SF6 as ideal technosignature gases. [PDF]
Seager S +5 more
europepmc +1 more source
Terrestrial exoplanets around M- and K-type stars are important targets for atmospheric characterization. Such planets are likely tidally locked with the order of spin–orbit resonances (SORs) depending on eccentricity. We explore the impact of SORs on 3D
Marrick Braam +5 more
doaj +1 more source
Analogous response of temperate terrestrial exoplanets and Earth's climate dynamics to greenhouse gas supplement. [PDF]
Hochman A, Komacek TD, De Luca P.
europepmc +1 more source
Atmospheric retrievals are widely used to constrain exoplanet properties from observed spectra. We investigate how the common nonphysical retrieval assumptions of vertically constant molecule abundances and cloud-free atmospheres affect our ...
Björn S. Konrad +3 more
doaj +1 more source
Revealing the atmospheres of highly irradiated exoplanets: from ultra-hot Jupiters to rocky worlds. [PDF]
Mansfield M.
europepmc +1 more source
Lessons from Hubble and Spitzer: 1D Self-consistent Model Grids for 19 Hot Jupiter Emission Spectra
We present a population-level analysis of the dayside thermal emission spectra of 19 planets observed with Hubble WFC3 and Spitzer IRAC 3.6 and 4.5 μ m, spanning equilibrium temperatures 1200–2700 K and 0.7–10.5 Jupiter masses.
Lindsey S. Wiser +6 more
doaj +1 more source
Photochemically produced SO<sub>2</sub> in the atmosphere of WASP-39b. [PDF]
Tsai SM +84 more
europepmc +1 more source

