Results 111 to 120 of about 193,103 (196)
Helium in Exoplanet Exospheres: Orbital and Stellar Influences
Searches for helium in the exospheres of exoplanets via the metastable near-infrared triplet have yielded 17 detections and 40 nondetections. We performed a comprehensive reanalysis of published studies to investigate the influence of stellar X-ray and ...
Vigneshwaran Krishnamurthy+1 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 Escape From Three Terrestrial Planets in the L 98-59 System
A critically important process affecting the climate evolution and potential habitability of an exoplanet is atmospheric escape, in which high-energy radiation from a star drives the escape of hydrogen atoms and other light elements from a planet’s ...
Emeline F. Fromont+8 more
doaj +1 more source
The Featherweight Giant: Unraveling the Atmosphere of a 17 Myr Planet with JWST
The characterization of young planets (
Pa Chia Thao+31 more
doaj +1 more source
Synergies Between Venus & Exoplanetary Observations: Venus and Its Extrasolar Siblings. [PDF]
Way MJ+11 more
europepmc +1 more source
identifier:oai:t2r2.star.titech.ac.jp ...
+3 more sources
Terrestrial planets in the habitable zone (HZ) of Sun-like stars are priority targets for detection and observation by the next generation of space telescopes.
Antonin Affholder+4 more
doaj +1 more source
Oxygen and ozone are two of the most important gases in Earth’s atmosphere. These arose as a result of photosynthesis and appeared prominently around 2.3–2.4 billion yr ago.
Russell Deitrick+3 more
doaj +1 more source
Planetary atmospheres Through Time: Effects of Mass Loss and Thermal Evolution [PDF]
Atmospheric mass loss is a fundamental phenomenon shaping the structure and evolution of planetary atmospheres. It can engage processes ranging from global interactions with the host star and large-scale hydrodynamic outflows to essentially microphysical kinetic effects.
arxiv
No thick carbon dioxide atmosphere on the rocky exoplanet TRAPPIST-1 c. [PDF]
Zieba S+18 more
europepmc +1 more source