Astrobiology70- Page

This artist’s visualisation of WASP-127b, a giant gas planet located about 520 light-years from Earth — ESO Astronomers have discovered extremely powerful winds pummeling the equator of WASP-127b, a giant

Evolution of thermal properties of GJ 486b. The two plots at the top denote the stellar luminosity evolution (bolometric and XUV) and the mantle potential temperature evolution for GJ 486b.

Keith Cowing Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻 Follow on

An astronaut examines apiece of Martian ice — Grok via Astrobiology.com The inclination to explore across vast expanses has been a continual part of human history. In voyages across the

Fluorine on Earth — Astrobiology.com Life on Earth is known to rarely make fluorinated carbon compounds, as compared to other halocarbons. We quantify this rarity, based on our exhaustive natural

L- lactaldehyde — Wikipedia Aldehydes are ubiquitous in star-forming regions and carbonaceous chondrites, serving as essential intermediates in metabolic pathways and molecular mass growth processes to vital biomolecules necessary for

Volvox – a multicellular green algae. Wikipedia It has been argued that the historical nature of evolution makes it a highly path-dependent process. Under this view, the outcome of evolutionary

A small planet orbiting its host star – Grok via Astrobiology.com A key to understand exoplanets is characterisation of their host stars. One of the most powerful tools to characterise

Uranus P-T profiles plotted over H2O phase diagram. The shaded region show adiabatic P-T profiles of distinct-layer structure models, assuming mixed H2O-H/He composition, in the (orange) envelope and (green) mantle