Nautilus gas-grain model Archives

CO2 ice abundance (upper left panel), visual extinction (upper right panel), H2 density (lower left panel), and dust temperature (lower right panel) as a function of time for a few cells. The blue curves present the results for the "high CO2 column density cases" while the red ones are the "low CO2 column density cases." -- astro-ph.GA

Astrochemistry, Astrogeology, Astronomy & Telescopes, Interstellar, Status Report

Astrochemical Models Of Interstellar Ices: History Matters

by Keith CowingJune 16, 2023June 16, 2023

Ice is ubiquitous in the interstellar medium. We model the formation of the main constituents of interstellar ices, including H2O, CO2 , CO, and CH3 OH.

Nautilus gas-grain model

Astrochemical Models Of Interstellar Ices: History Matters

Potential Survivable Niches For Microbial Life On The Lunar South Pole

JWST Telemetry Combined With Active Coronagraphy: Raw Contrast Predictions For Exoplanet Imaging With The Habitable Worlds Observatory

Antarctica Is Home To Microbes Found Nowhere Else On Earth

Study: Peptides Can Form Well-defined Structures In Harsh, Venus-like Conditions

Modeling Carbon-Based Planets with MAGRATHEA