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The Contaminant Footprint of Landed Spacecraft: Toward an Inventory and Modelling FrameworkAll spacecraft generate and carry contaminants, i.e., unwanted and potentially harmful material. When a spacecraft lands and operates in near-vacuum, as onto Earth’s Moon, it introduces contaminants into its environment that may compromise mission science objectives and engineering performance. Contamination of solar system bodies may irrevocably degrade targets of unique value to planetary scientists, for instance, as lunar landed spacecraft introduce propellant effluents into the otherwise pristine ice of the Moon’s permanently shadowed regions.

NASA’s planetary protection discipline seeks to ensure that solar system bodies are not contaminated, for scientific purposes, by terrestrial material (i.e., forward contamination). This interest aligns with planetary science interest in mitigating the transport of terrestrial contaminants onto solar system bodies and in controlling types of contamination that could compromise the scientific value of samples or measurements. NASA, and other entities that practice planetary science, have compelling and multidisciplinary interests in the preservation of special regions and sampling sites of high scientific value – including lunar permanently shadowed regions (PSRs) – from inadvertent contamination by any spacecraft, and in understanding the contamination of such regions by all spacecraft.

Organic molecular contamination here represents a primary threat. Organic molecules will be introduced to solar system bodies by nominal landed spacecraft and crew processes – including by the action of descent and ascent engines; natural materials outgassing; and crew environmental and life support system sources. Molecular contaminants can also travel in the free-molecular sense at global scale across near-vacuum bodies, including into regions where they may be permanently trapped.

This presentation will address a high-level study to identify sources of contaminants – in particular, organic material – generated by landed spacecraft along with the transport vectors by which these contaminants can reach sites of scientific interest on bodies like the Moon. A vision for an integrated modeling framework for the organic contamination footprint of spacecraft missions, individually and collectively, will also be described and presented along with initial conclusions related to organic molecular transport.
Document ID
20260006844
Acquisition Source
Johnson Space Center
Document Type
Presentation
Authors
William A Hoey
(Amentum (United States) Chantilly, France)
Carlos E Soares ORCID
(Amentum (United States) Chantilly, France)
John M Alred
(Jet Propulsion Laboratory Pasadena, United States)
Nick Benardini
(National Aeronautics and Space Administration Washington, United States)
Erin Lalime
(Goddard Space Flight Center Greenbelt, United States)
P Gutierrez Cascales
(NASA Intern Houston, Texas, United States)
R Alves Hailer
(NASA Intern Houston, Texas, United States)
Date Acquired
July 27, 2026
Publication Date
August 5, 2026
Subject Category
Exobiology
Meeting Information
Meeting: COSPAR 2026: 46th Scientific Assembly
Location: Florence
Country: IT
Start Date: August 1, 2026
End Date: August 9, 2026
Sponsors: Lockheed (United States)
Funding Number(s)
CONTRACT_GRANT: 80NM0018D0004
CONTRACT_GRANT: 80JSC022DA035
Distribution Limits
Public
Copyright
Public Use Permitted.
Technical Review
NASA Technical Management
Keywords
Gas Dynamics
Planetary Protection
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