MétaCan
Menu
Back to cohort
Record W4412122813 · doi:10.5194/epsc-dps2025-1091

The At. Astra Research Group: Using Atomic Modelling to Better Explain the Surface-Exosphere Connection on Airless Bodies

2025· preprint· en· W4412122813 on OpenAlexaff
Liam S. Morrissey, Ben Clouter-Gergen, Anastasis Georgiou, Jesse Lewis-Roy, Vikentiy Pashuk, Amanda Ricketts

Bibliographic record

Venuenot available
Typepreprint
Languageen
FieldEngineering
TopicAerosol Filtration and Electrostatic Precipitation
Canadian institutionsMemorial University of Newfoundland
Fundersnot available
KeywordsExosphereASTRAConnection (principal bundle)Group (periodic table)PhysicsAstrobiologyEngineeringMechanical engineering

Abstract

fetched live from OpenAlex

For nearly 40 years, planetary science studies of the exospheres of Mercury, the Moon, and other airless bodies have been hindered because of uncertainties in our understanding of the surface processes influencing exosphere formation. The surfaces of these airless bodies can be subjected to several different emission processes including solar wind induced sputtering, photon stimulated desorption, and micrometeorite impact vaporization. However, the relative contributions of these various processes to the body’s exosphere remains contested for many observed elemental species. To obtain a true understanding of the surface-exosphere connection of airless bodies we must first improve our understanding of the interplay of these different processes and how they are affected by the specific characteristics of the surface. However, many of these key emission processes are occurring on the atomic scale, meaning global exosphere models often require atomically derived parameters as inputs. These inputs are difficult to obtain experimentally, and are therefore typically derived via fitting, often overlooking important complexities that can significantly affect predicted results. Further complicating this picture is the fact that some proportion of the ejected atoms leave the surface at energies lower than the escape energy of the body and thus return to the surface. A portion of these atoms can then be reaccommodated on the surface at an energy and composition unique from the mineral bulk. However, current global exosphere models are unable to consider the effects of adsorbed atoms nor the contribution of emission from the newly formed adsorbed layers.Here, we will discuss how molecular dynamics (MD) modelling on the atomic scale can be a critical tool to provide physically realizable and surface-specific input parameters for global exosphere models. We will discuss a series of our previous studies from our group based out of Memorial University that have used MD modelling to study key planetary science processes on the atomic scale. This will include MD models of sputtering, diffusion, surface adsorption, surface free energy, and micro meteorite impacts. For each study we will discuss key unknowns introducing uncertainties into global models. We will then apply atomic modelling to study these processes on the atomic scale, better understanding the underlying physics.Finally, we will conclude with a discussion on new areas that we can apply these approaches to new research areas including icy bodies and exoplanets.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.347
Threshold uncertainty score0.805

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0010.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.076
GPT teacher head0.321
Teacher spread0.245 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations0
Published2025
Admission routes1
Has abstractyes

Explore more

Same topicAerosol Filtration and Electrostatic PrecipitationFrench-language works237,207