Results 71 to 80 of about 6,508 (165)
On the Measurement of Ocean Acidity With Ambient Sound
Abstract The volume‐integrated pH of seawater can be determined from the frequency and depth dependence of wind‐generated ambient noise in the ocean. Over the 1–10 kHz frequency band, three main processes contribute to the acoustic attenuation in seawater: the chemical relaxation of boric acid and magnesium carbonate (<3 kHz, related to pH) and of ...
Ernst M. Uzhansky +2 more
wiley +1 more source
The disintegrating ultrashort period rocky exoplanet K2-22 b periodically emits dusty clouds in a dynamically chaotic process resulting in a variable transit depth from 0% to 1.3%.
Nick Tusay +14 more
doaj +1 more source
Hot Jupiters are typically considered to be tidally locked due to their short orbital periods. The extreme irradiation can result in atmospheric species becoming thermally ionized on the dayside, which then interact with the planet’s magnetic field by ...
Hayley Beltz +5 more
doaj +1 more source
A Large and Variable Leading Tail of Helium in a Hot Saturn Undergoing Runaway Inflation
Atmospheric escape shapes the fate of exoplanets, with statistical evidence for transformative mass loss imprinted across the mass–radius–insolation distribution.
Michael Gully-Santiago +16 more
doaj +1 more source
Multiple Patchy Cloud Layers in the Planetary-mass Object SIMP 0136+0933
Multiwavelength photometry of brown dwarfs and planetary-mass objects provides insight into their atmospheres and cloud layers. We present near-simultaneous J - and K _s -band multiwavelength observations of the highly variable T2.5 planetary-mass object,
Allison M. McCarthy +8 more
doaj +1 more source
Isolated planetary-mass objects share their mass range with planets but do not orbit a star. They lack the necessary mass to support fusion in their cores and thermally radiate their heat from formation as they cool, primarily at infrared wavelengths ...
Allison M. McCarthy +19 more
doaj +1 more source
A Search for Temporal Atmospheric Variability of Kepler Hot Jupiters
We perform a systematic search for atmospheric variability in short-period gas-giant planets (hot Jupiters) observed by the Kepler mission, by looking for temporal variability of their secondary eclipse depths.
Canis Li, Avi Shporer
doaj +1 more source
HET/HPF Observations of Helium in Warm, Hot, and Ultrahot Jupiters
The near-infrared helium triplet line is a powerful tool for studying atmospheric escape processes of close-in exoplanets, especially irradiated gas giants. Line profile fitting provides direct insight into the mechanisms driving atmospheric mass loss of
Jaume Orell-Miquel +7 more
doaj +1 more source
Effects of Transient Stellar Emissions on Planetary Climates of Tidally Locked Exo-Earths
Space weather events in exoplanetary environments sourced from transient host star emissions, including stellar flares, coronal mass ejections, and stellar proton events, can substantially influence a planet's habitability and atmospheric evolution ...
Howard Chen +3 more
doaj +1 more source
Time-resolved X-ray spectra of Proxima Centauri as seen by XMM-Newton
Context. Stellar soft X-ray ([1, 100] Å) and extreme ultraviolet (also EUV, [100, 920] Å; jointly, XUV) radiation affect the evolution and chemistry of exoplanet atmospheres. It is, however, uncertain to what extent the radiation’s short-term variability
Damonte A. +4 more
doaj +1 more source

