The Hebrew University of Jerusalem Archives

Median temperature (K) differences between high and low pCO2 scenarios and median wind speeds (m s−1) for each scenario for Earth-like (a, c) and TRAPPIST-1e (b, d) ExoCAM simulations at (a, b) upper and (c, d) near-surface levels. Black and green quivers represent the high and low pCO2 scenarios, respectively. Using the Wilcoxon Rank-Sum test, lime and magenta-filled contours for wind speed and temperature represent areas not statistically significant at the 5% level, respectively. -- The Hebrew University of Jerusalem

Atmospheres, Climate, Weather, Biochemistry & Organic Chemistry, Exoplanets, -moons, -comets, Habitable Zones, Press Release, TRAPPIST-1

Greenhouse Gas Supplement Increases Warming And Alters Circulation Patterns On Earth and Earth-like Exoplanets

by Keith CowingJuly 13, 2023July 13, 2023

With the launch of the James Webb Space Telescope (JWST), the study of exoplanetary atmospheres and their potential habitability reached new heights. A team of researchers led by Dr. Assaf […]

Difference (Δ) between Earth analog and TRAPPIST-1e (a, d, g)

Exoplanets, -moons, -comets, Habitable Zones, Press Release, TRAPPIST-1

Innovative System Evaluates Habitability Of Distant Planets

by Keith CowingOctober 20, 2022October 20, 2022

The climate crisis presents a huge challenge to all people on Earth. It has led many scientists to look for exo-planets, planets outside our solar system that humans could potentially […]