Results 51 to 60 of about 700,042 (263)
Measuring titanium isotope ratios in exoplanet atmospheres [PDF]
[abridged] Measurements of relative isotope abundances can provide unique insights into the formation and evolution histories of celestial bodies. The five stable isotopes of titanium are used to study the early history of the solar system and constrain ...
Dilovan B. Serindag+2 more
semanticscholar +1 more source
Nonthermal Atmospheric Escape on the Kepler-11 “Super-Earths” Driven by Stellar Wind Sputtering
Jeans escape or hydrodynamic escape is believed to dominate atmospheric loss for hot Jupiters. However, nonthermal mechanisms likely contribute substantially on hydrogen-rich “super-Earths” with relatively cold and extended atmospheres.
Hao Gu+4 more
doaj +1 more source
Disequilibrium Chemistry in Exoplanet Atmospheres Observed with the Hubble Space Telescope
Literature on the theory of exoplanet atmospheric disequilibrium chemistry is rich, although its observational counterpart has yet to emerge beyond the hints provided by a few targets in dedicated studies. We report results from an uniform data reduction
Gaël M. Roudier+5 more
openalex +2 more sources
Retrieving C and O Abundance of HR 8799 c by Combining High- and Low-resolution Data
The formation and evolution pathway for the directly imaged multiplanetary system HR 8799 remains mysterious. Accurate constraints on the chemical composition of the planetary atmosphere(s) are key to solving the mystery.
Ji Wang+31 more
doaj +1 more source
Chemical modeling of exoplanet atmospheres [PDF]
The past twenty years have revealed the diversity of planets that exist in the Universe. It turned out that most of exoplanets are different from the planets of our Solar System and thus, everything about them needs to be explored. Thanks to current observational technologies, we are able to determine some information about the atmospheric composition,
Marcelino Agúndez+2 more
openaire +5 more sources
Exoplanet secondary atmosphere loss and revival [PDF]
SignificanceEarth and Venus have significant atmospheres, but Mercury does not. Thousands of exoplanets are known, but we know almost nothing about rocky exoplanet atmospheres. Many rocky exoplanets were formed by a sub-Neptune-to-super-Earth conversion process during which planets lose most of their H2-rich (primary) atmospheres and are reduced in ...
Edwin S. Kite, Megan Barnett
openalex +5 more sources
Atmospheric Seasonality as an Exoplanet Biosignature [PDF]
Abstract Current investigations of exoplanet biosignatures have focused on static evidence of life, such as the presence of biogenic gases like O2 or CH4. However, the expected diversity of terrestrial planet atmospheres and the likelihood of both “false positives” and “false negatives” for conventional biosignatures motivate exploration
Victoria S. Meadows+12 more
openaire +6 more sources
We present the first exoplanet phase-curve measurement made with the JWST NIRSpec instrument, highlighting the exceptional stability of this newly commissioned observatory for exoplanet climate studies.
Thomas Mikal-Evans+12 more
doaj +1 more source
The Runaway Greenhouse on Sub-Neptune Waterworlds
The implications of the water vapor runaway greenhouse phenomenon for water-rich sub-Neptunes are developed. In particular, the nature of the postrunaway equilibration process for planets that have an extremely high water inventory is addressed. Crossing
Raymond T. Pierrehumbert
doaj +1 more source
Haze Formation in Warm H2-rich Exoplanet Atmospheres [PDF]
New observing capabilities coming online over the next few years will provide opportunities for characterization of exoplanet atmospheres. However, clouds/hazes could be present in the atmospheres of many exoplanets, muting the amplitude of spectral ...
Chao He+10 more
openalex +2 more sources