Photochemical hazes are suspected to obscure molecular features, such as water, from detection in the transmission spectra of exoplanets with atmospheric temperatures < 800 K.
extrasolar
The Abundance of Belatedly Habitable Planets And Ambiguities In Definitions Of The Continuously Habitable Zone
A planet’s history dictates its current potential to host habitable conditions and life. The concept of the Continuously Habitable Zone (CHZ) has been used to define the region around a […]
Redox State And Interior Structure Control On The Long-term Habitability Of Stagnant-lid Planets
A major goal in the search for extraterrestrial life is the detection of liquid water on the surface of exoplanets.
A Rocky Exoplanet Classification Method And Its Application To Calculating Surface Pressure And Surface Temperature
With over 5,000 exoplanets currently detected, there is a need for a primary classification method to prioritise candidates for biosignature observations.
Optical Properties Of Organic Hazes In Water-rich Exoplanet Atmospheres: Implications For Observations With JWST
JWST has begun its scientific mission, which includes the atmospheric characterization of transiting exoplanets.
TESS Discovers TOI 700 Planetary System’s Second Earth-Sized World
Using data from NASA’s Transiting Exoplanet Survey Satellite, scientists have identified an Earth-size world, called TOI 700 e, orbiting within the habitable zone of its star – the range of […]
A Gaian Habitable Zone
When searching for inhabited exoplanets, understanding the boundaries of the habitable zone around the parent star is key.
Diverse Carbonates In Exoplanet Oceans Promote The Carbon Cycle
Carbonate precipitation in oceans is essential for the carbonate-silicate cycle (inorganic carbon cycle) to maintain temperate climates.
The CARMENES Search For Exoplanets Around M Dwarfs, Wolf 1069 b: Earth-mass Planet In The Habitable Zone Of A Nearby, Very Low-mass Star
We present the discovery of an Earth-mass planet (Mbsini=1.36±0.21M⊕) on a 15.6d orbit of a relatively nearby (d∼9.6pc) and low-mass (0.167±0.011M⊙) M5.0V star, Wolf 1069.
In Search of the Edge: A Bayesian Exploration of the Detectability of Red Edges in Exoplanet Reflection Spectra
Reflection spectroscopy holds great promise for characterizing the atmospheres and surfaces of potentially habitable terrestrial exoplanets.
