In a cleanroom at the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland, on April 3, 2026, (from left) Sean Gazarik, Tyler Radomsky, Amber Dubill and Emory Toomey complete

A simulated Archean Earth-like TRAPPIST-1 e, to which we apply our novel retrieval algorithm. Left: The modeled temperature profile (black dashed line) and mixing ratio profiles (solid color lines) of

The Dyson Minds 2025 Workshop The Dyson Minds 2025 Workshop, held at the Center for Brains, Minds & Machines at MIT and organized by Penn State, MIT, and The Ultraintelligence

Graphical Abstract Overview of microbial diversity and environmental drivers in Icelandic deep basaltic aquifers. Using 16S rRNA gene metabarcoding across 22 geothermal wells spanning broad temperature, pH, and bedrock-age gradients,

The night-side surface temperatures for different minimum eccentricities for K2-141b, at its present day orbit. The three lines in blue, green and indigo represent three types of mantle mixtures where

Integrated intensity maps of representative CH3COCH3 unblended lines observed towards I16272-4837C1. The color scale is the continuum at a wavelength of 3 mm. The white contours indicate CH3COCH3 at difference

TMC-1 (detail) ESA/Herschel/NASA/JPL-Caltech; acknowledgement: R. Hurt (JPL-Caltech), CC BY-SA IGO 3.0 Source Hydrogen atom tunneling likely plays a substantial role in the gas-phase chemistry of astrochemical environments. To determine the