Homepage

Top Story

How High-pressure Ices On Large Ocean Worlds Can Support Habitability: The Compatibility Of Amino Acids Into Ice VI And VII

[Science Advances] Water oceans in large icy moons and exoplanets are isolated from the rocky interior by thick layers of high-pressure ice, which hinder the direct release of nutrients and organics derived from water-rock interaction to the ocean. Possible uptake of these bio-essential compounds into high-pressure ice phases could regulate their availability in the ocean,…

Latest

Upcoming Events

Atmospheres, Climate, Weather

Topographically Forced Stationary Waves Can Explain The Near-Surface Zonal Winds Observed By Huygens On Titan

[astro-ph.EP] Titan’s equatorial superrotation is associated with climatological retrograde (westward) near-surface winds at low latitudes, as consistently simulated by Titan general circulation models. However, the Huygens probe measured prograde (eastward) near-surface winds, contrary to the expected circulation. We investigate whether these observations reflect localized forcing by large-scale topography, using paired three-dimensional dry simulations with and…

Read more

Exploration Gear & Tech

Imaging & Spectroscopy

Biosignatures & Paleobiology

Gift this article