Molecular Mobility Of Exraterrestrial Ices: Surface Diffusion In Astrochemistry And Planetary Science

editorAstrobiologyYesterday3 Views

Molecular Mobility Of Exraterrestrial Ices: Surface Diffusion In Astrochemistry And Planetary Science

Various examples of surface diffusion and related processes taking place in condensed phases in space. Each panel illustrates a distinct diffusion mechanism: Langmuir–Hinshelwood (top left) shows reactants diffusing before meeting; hot atom diffusion (top right) depicts energetic species moving rapidly across surfaces; non-diffusive reactions (bottom left) occur only requiring serendipitous proximity; and segregation (bottom right) shows separation of different molecular species in mixed ices. Image adapted from Cuppen et al.– Physical Chemistry Chemical Physics

Molecules are ubiquitous in space. They are necessary components in the creation of habitable planetary systems and can provide the basic building blocks of life.

Solid-state processes are pivotal in the formation of molecules in space and surface diffusion in particular is a key driver of chemistry in extraterrestrial environments, such as the massive clouds in which stars and planets are formed and the icy objects within our solar system.

However, for many atoms and molecules quantitative theoretical and experimental information on diffusion, such as activation barriers, are lacking. This hinders us in unravelling chemical processes in space and determining how the chemical ingredients of planets and life are formed.

In this article, an astrochemical perspective on diffusion is provided. Described are the relevant adsorbate-surface systems, the methods to model their chemical processes, and the computational and laboratory techniques to determine diffusion parameters, including the latest developments in the field. While much progress has been made, many astrochemically relevant systems remain unexplored.

The complexity of ice surfaces, their temperature-dependent restructuring, and effects at low temperatures create unique challenges that demand innovative experimental approaches and theoretical frameworks. This intersection of astrochemistry and surface science offers fertile ground for physical chemists to apply their expertise.

We invite the physical chemistry community to explore these systems, where precise diffusion parameters would dramatically advance our understanding of molecular evolution in space-from interstellar clouds to planetary surfaces-with implications on our understanding on the origins of life and planetary habitability.

Molecular mobility of extraterrestrial ices: surface diffusion in astrochemistry and planetary science, Physical Chemistry Chemical Physics via PubMed

Molecular mobility of extraterrestrial ices: surface diffusion in astrochemistry and planetary science, Physical Chemistry Chemical Physics (open access)

Astrobiology, Astrochemistry,

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) 🖖🏻

0 Votes: 0 Upvotes, 0 Downvotes (0 Points)

Leave a reply

Recent Comments

No comments to show.
Join Us
  • Facebook38.5K
  • X Network32.1K

Stay Informed With the Latest & Most Important News

[mc4wp_form id=314]
Categories

Advertisement

Loading Next Post...
Follow
Search Trending
Popular Now
Loading

Signing-in 3 seconds...

Signing-up 3 seconds...