Expanding the Human Factors Toolbox:  An Approach to Balancing Crew and Mission Design Parameters 

Expanding the Human Factors Toolbox:  An Approach to Balancing Crew and Mission Design Parameters 

This article is from the 2025 Technical Update.

The human factors TDT looks for and creates opportunities to influence design to leverage human strengths and to protect people and missions. The human factors team has experts with knowledge of human performance in all aspects of NASA missions as well as from other safety-critical industries. The goal is to ensure that science-based human factors knowledge and lessons learned are applied throughout the mission lifecycle. The strategy is to 1) modify existing and create new discipline tools that meet NASA’s needs and constraints, 2) build strategies to enhance the disciplines’ chances for success, 3) enhance simulation techniques to gain maximum information even when verification and validation  opportunities are limited, 4) develop new analysis methods for human performance in NASA mission contexts, and 5) reframe  understanding of human performance to emphasize the key role of human resilience in mission success. 

This article highlights a set of analytical models of crew workload, training, and expertise that can be used to aid decision makers in determining the size of a Mars crew adequate for crew safety and mission success. These tools are built on a Department of Defense (DoD) capability that has been used extensively to evaluate the success of specific designs. Unlike missions in low Earth orbit or even to the Moon, a crewed Mars mission will operate under extraordinary constraints, primarily a significant communication delay with Earth and prolonged communication blackout periods. This necessitates a radical rethinking of mission design, including the human elements of crew size, workload, expertise, and resilient performance.  

To address this gap, the NESC developed a systematic and quantitative methodology, along with an associated suite of modeling tools, to enable the development of an evidence-based trade space for guiding crew size decisions for human Mars missions. This work provides actionable analysis to programs and projects early in development, enabling simultaneous consideration of mission architecture, operational concepts, and the roles human will play throughout the mission. This analysis supports the development of mission designs that preserve and enable human resilient performance to ensure the success and safety of future Mars exploration. 

Historically, NASA’s human spaceflight programs have relied on real-time support from extensive ground control, composed of a collective intellect that acts as an extended crew to manage objectives and respond to anomalies. As depicted in Figure 1, the volume of ISS ground personnel highlights the vast support structure available for Earth-proximal missions. However, for Mars, communication delays of up to 22 minutes one-way and blackouts lasting up to three weeks during superior conjunctions will eliminate this real-time lifeline. This demands a new focus on the capabilities required of the onboard crew, who will face time-critical decisions and unforeseen failures with only their knowledge and onboard decision-support systems, often without pre-existing procedures. 

Current ground-support expertise for ISS missions
Current ground-support expertise for ISS missions

The NESC’s methodology fills a longstanding gap, as past Mars crew size determinations often lacked detailed quantitative analysis of crew tasking, workload, and expertise. Extending DoD methodologies for manpower determination, the NESC human factors trade space methodology offers a repeatable and data-driven means to assess whether a given crew complement possesses the capability to accomplish mission objectives and respond successfully to unforeseen failures that have potential loss of crew or loss of mission (LOC/LOM) consequences. The core process involves gathering Mars mission concepts and information, determining use cases to model, creating a trade space evaluation framework, conducting human performance modeling, and performing trade space analyses. This iterative approach, conceptually represented by the Mars Crew Size Decision Process (see Figure 2), allows for adaptation as technologies and mission assumptions evolve. 

Central to this methodology are four human performance models, each revealing critical insights into the human factors of Mars mission design. 

1. IV Operations for Planetary Surface EVA Model: This model examined the mental workload of intravehicular (IV) Mars crewmembers supporting a planetary surface extravehicular activity (EVA), simulating activities currently performed by Mission Control Center personnel for ISS EVAs. It predicted that during a Mars surface technical EVA conducted at the pace of an ISS EVA, the workload for an IV crewmember performing combined essential flight controller duties would be unacceptably high, indicating a severe negative impact on task performance. This finding underscores the necessity of reconsidering EVA pacing, task automation, or increasing IV support crew complement to ensure mission-critical EVAs are safely conducted independently of Earth-based support. 

2. Robotic Arm Assisted EVA Operator Model: This model assessed the mental workload of a crewmember operating a robotic arm (see Figure 3) in both manual and automated control modes on a Mars transit vehicle. The model results indicate that two crewmembers may be necessary to mitigate unacceptably high workload during manual robotic arm operations. Furthermore, consistent with the scientific literature, the model predicted that stressors like sleep debt increase mental workload and degrade performance, extending task completion times. This highlights the importance of accounting for crew well-being in crew-size determinations. 

3. Mars Transit Crew Model: This analysis focused on crew utilization and staffing requirements during a 9-month Mars transit mission, reallocating planned and unplanned tasks from ground control to the crew. The modeling, using ISS-equivalent task assumptions, predicted that more than six crewmembers (given average rates for unplanned events) would be needed to achieve the same number of work hours as a four-person ISS mission. This substantial increase emphasizes the critical impact of Earth-independence on daily crew workload and the imperative for adequate crew complement to manage ongoing responsibilities. 

4. Personnel, Expertise, and Training Model: Given the communication delay/blackout with Mars, paired with no rapid return-to-Earth options, NASA will need to rely on the expertise of the crew to respond to unforeseen failures. A custom model was developed to quantify the crew expertise required to meet mission objectives and respond to unforeseen events with LOC/LOM potential and short time-to-effect. Based on analysis of ISS historical data, the probability of at least one occurrence of such a failure during Mars transit is greater than 99%. A sensitivity analysis of the relationship between a successful crew response and LOC/LOM outcome was conducted for cases in which the crew gave a successful response 90%, 95%, 98%, and 99.985% of the time. The estimated likelihood of a LOC/LOM consequence for all but the most conservative of these cases is greater than 1%, which is considered in the “very high” (red) range, per the Human System Risk Board risk matrix. The likelihood of LOC/LOM consequences only drops below 0.1% (yellow) for a successful response rate of 99.985%. When unforeseen failures occur on a mission to Mars, it will be critical that the crew have the necessary level of expertise to accurately diagnose problems and restore critical functionality. The Personnel, Expertise, and Training model is designed to provide the agency with the capability to consider the trade space

The NESC’s proposed methodology to aid crew-size determinations.
Trade-space parameters are input into any of four models, whose output
characterizes the risk level associated with a given crew size.
Astronaut Anne McClain using the
Space Station Remote Manipulator System on ISS.

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Meagan Chappell

Webinar 3/25: NASA CSDA Vendor Focus – Satellogic

Webinar 3/25: NASA CSDA Vendor Focus – Satellogic

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Webinar 3/25: NASA CSDA Vendor Focus – Satellogic

Satellite image of coastal Louisiana showing sediment plumes entering the Gulf of Mexico near river outlets, with surrounding wetlands and agricultural land patterns along the coastline.
Satellogic satellite imagery of coastal Louisiana shows sediment plumes entering the Gulf of Mexico, illustrating how Earth observation data can monitor coastal and environmental dynamics.
Image courtesy of Satellogic

Join us on Wednesday, March 25 at 2:00 p.m. EDT (-04:00 UTC) to learn more about NASA Commercial Satellite Data Acquisition (CSDA) program vendor Satellogic and how to discover, access, and work with their high-resolution commercial datasets.

NASA’s Earth Science Division (ESD) established the Commercial Satellite Data Acquisition (CSDA) program to explore the potential of commercial satellite data in advancing the agency’s Earth science research and application objectives. The program aims to identify, assess, and acquire data from commercial providers, which may offer a cost-effective means of supplementing Earth observations collected by NASA, other U.S. Government agencies, and international collaborators.

Satellogic delivers high-resolution Earth observation imagery at scale through its vertically integrated satellite constellation. During this NASA CSDA program webinar, speakers will introduce Satellogic and its constellation of commercial Earth Observation satellites. Representatives will highlight current and future capabilities, including service-level monitoring at scale, and plans for global daily remapping. They will also discuss how these data products complement NASA Earth science data holdings for research and applications. In addition, presenters will address the services and tools available to data users, including how they can get expert assistance when using Satellogic datasets.  

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Mar 10, 2026

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COPV Damage Tolerance Life Demonstration Guidelines 

COPV Damage Tolerance Life Demonstration Guidelines 

This article is from the 2025 Technical Update.

The NESC has invested significant time and resources to better understand composite overwrapped pressure vessels (COPV) performance and more importantly, how these complex, high-pressure storage systems can fail. These vessels, which store high pressure propulsion and life-support system fluids on launch vehicles and spacecraft, are ubiquitous at NASA, and failures have the potential to be catastrophic. 

This year the NESC finalized work on a set of guidelines intended for use by NASA civil servants and support contractors in their development or assessment of damage-tolerance demonstration data for COPVs. These guidelines are based on the NESC’s experience in assessing agency-wide COPV applications and compiling the best practices for complying with the damage-tolerance requirements of AIAA S-081, the standard for COPVs used in human and robotic spaceflight, and NASA-STD-5019, Fracture Control Requirements for Spaceflight Hardware.

Previously referred to as “safe-life,” damage tolerance life assumes detectable cracks exist before service and demonstrates that such cracks, in worst-case locations and orientations, will not grow to failure over the service life. A 4x life factor is applied, requiring that cracks do not reach failure (leakage or unstable growth) within four times the expected service cycles.  

These guidelines are meant to support NASA personnel in applying S-081 requirements and also to clarify areas that historically have had varied interpretation. And by leveraging NESC assessments where approaches to damage tolerance were found to be unconservative, the guidelines offer best practices for minimizing risk based on supporting data—and do so without introducing new standards. The guidelines touch on numerous aspects of damage tolerance life including:  

  • COPV mechanics and model correlation, 
  • Identifying worst case locations for damage tolerance,  
  • Nondestructive evaluation (NDE), 
  • Addressing crack aspect ratios, 
  • Defining load spectra, 
  • Addressing autofrettage crack growth, 
  • Performing damage-tolerance life demonstration by analysis using a crack-growth analysis software like NASGRO, 
  • Performing damage-tolerance life by coupon or vessel testing, and 
  • Addressing sustained-load crack growth and environmentally assisted cracking. 

In determining the worst-case locations for damage tolerance evaluation, the guidelines offer a method for evaluating the contributing factors—stress/strain, material properties, thick-ness, and initial crack size. The identified regions show different liner material forms and welds, and within each form, the initial crack size based on the NDE method used, the minimum thickness, and the peak stress/strain level are determined for that form. The guidelines then provide best practices for addressing damage tolerance with each material form and worst-case location in the COPV.  

EXAMPLES OF MATERIAL FORMS IN COPV LINER

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Meagan Chappell

Two Observatories, One Cosmic Eye: Hubble and Euclid View Cat’s Eye Nebula

Two Observatories, One Cosmic Eye: Hubble and Euclid View Cat’s Eye Nebula

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Two Observatories, One Cosmic Eye: Hubble and Euclid View Cat’s Eye Nebula

A planetary nebula in space. The star in the very center is surrounded by white bubbles and loops of gas, all shining with a powerful blue light. Farther away a broken ring of red and blue gas clouds surrounds the nebula. A multitude of golden and white stars, wisps of gas and distant galaxies of various sizes surround the nebula on the black background.
Hubble and Euclid teamed up in this image of the Cat’s Eye Nebula, NGC 6543.
Credits:
ESA/Hubble & NASA, ESA Euclid/Euclid Consortium/NASA/Q1-2025, J.-C. Cuillandre & E. Bertin (CEA Paris-Saclay), Z. Tsvetanov
Two images of a planetary nebula (the Cat's Eye Nebula) in space. The image to the left, labeled “Euclid & Hubble”, shows the whole nebula and its surroundings. A star in the very center is surrounded by white bubbles and loops of gas, all shining with a powerful blue light. Farther away a broken ring of red and blue gas clouds surrounds the nebula. The background shows many stars and distant galaxies. A white box indicates the center of the nebula and this region is the image to the right, labelled “Hubble”. It shows the multi-layered bubbles, pointed jets and circular shells of gas that make up the nebula, as well as the central star, in greater detail.
ESA/Hubble & NASA, ESA Euclid/Euclid Consortium/NASA/Q1-2025, J.-C. Cuillandre & E. Bertin (CEA Paris-Saclay), Z. Tsvetanov

This new NASA/ESA Hubble Space Telescope image features one of the most visually intricate remnants of a dying star: the Cat’s Eye Nebula, also known as NGC 6543. This extraordinary planetary nebula lies in the constellation Draco and has captivated astronomers for decades with its elaborate and multilayered structure. Observations with ESA’s Gaia mission place the nebula at 4,400 light-years away.

Planetary nebulae, so-called because of their round shape, which made them appear to look like planets when viewed through early telescopes, are in fact expanding gas thrown off by stars in their final stages of evolution. It was the Cat’s Eye Nebula itself where this fact was first discovered in 1864 — examining the spectrum of its light reveals the emission from individual molecules that’s characteristic of a gas, distinguishing planetary nebulae from stars and galaxies. 

Hubble also revolutionized our understanding of planetary nebulae; its detailed images showed that the simple, circular appearance of a planetary nebula seen from the ground belies a very complex morphology. This was particularly true of the Cat’s Eye Nebula, where Hubble images in 1995 revealed never-before-seen structures that broadened our understanding of how planetary nebulae come to be.

An image of the center of a planetary nebula (the Cat's Eye Nebula). A blue star sits at the center within a series of overlapping, translucent bubbles of gas. The bubbles have a complex, filamentary structure. The two largest bubbles overlap halfway, creating an eye-like shape with the star at the center. Jets of high-speed gas point out of the top and bottom of the nebula. Faint, concentric circles of gas also surround the star, out beyond the bubbles.
In this new image, Hubble captures the very core of billowing gas with the High Resolution Channel sub-instrument on its Advanced Camera for Surveys (ACS). This instrument is optimized for taking very sharp images of fine details in a small area, such as the complex features at the heart of the Cat’s Eye Nebula. The data reveal a tapestry of concentric shells, jets of high-speed gas and dense knots sculpted by shock interactions, features that appear almost surreal in their intricacy. These structures are believed to record episodic mass loss from the dying star at the nebula’s center, creating a kind of cosmic “fossil record” of its final evolutionary stages. Part of these data were also used in a previous image of the Cat’s Eye Nebula, released in 2004. Previously unused data from ACS is combined with state-of-the-art image processing to create this new image, the sharpest yet taken of this nebula.
ESA/Hubble & NASA, Z. Tsvetanov

This time, Hubble is joined by ESA’s Euclid space telescope to create a new image of NGC 6543. The combined eyes of Hubble and Euclid reveal the remarkable complexity of stellar death in this object. Though primarily designed to map the distant universe, Euclid captures the Cat’s Eye Nebula as part of its deep imaging surveys. In Euclid’s wide, near-infrared, and visible light view, the arcs and filaments of the nebula’s bright central region are situated within a halo of colorful fragments of gas zooming away from the star. This ring was ejected from the star at an earlier stage, before the main nebula at the center formed. The whole nebula stands out against a backdrop teeming with distant galaxies, demonstrating how local astrophysical beauty and the farthest reaches of the cosmos can be seen together with Euclid.

A planetary nebula in space. The star in the very center is surrounded by white bubbles and loops of gas, all shining with a powerful blue light. Farther away a broken ring of red and blue gas clouds surrounds the nebula. A multitude of golden and white stars, wisps of gas and distant galaxies of various sizes surround the nebula on the black background.
In Euclid’s wide, near-infrared, and visible light view, the arcs and filaments of the nebula’s bright central region are situated within a halo of colorful fragments of gas zooming away from the star. This ring was ejected from the star at an earlier stage, before the main nebula at the center formed. Hubble captures the very core of the billowing gas with high-resolution visible-light images, adding extra detail in the center of this image. The whole nebula stands out against a backdrop teeming with distant galaxies, demonstrating how local astrophysical beauty and the farthest reaches of the cosmos can be seen together in modern astronomical surveys. Together, these missions provide a rich and complementary view of NGC 6543 — revealing the delicate interplay between stellar end-of-life processes and the vast cosmic tapestry beyond.
ESA/Hubble & NASA, ESA Euclid/Euclid Consortium/NASA/Q1-2025, J.-C. Cuillandre & E. Bertin (CEA Paris-Saclay), Z. Tsvetanov

Within this broad view of the nebula and its surroundings, Hubble captures the very core of the billowing gas with a new high-resolution visible-light image, adding extra detail in the center of this image. The data reveal a tapestry of concentric shells, jets of high-speed gas and dense knots sculpted by shock interactions, features that appear almost surreal in their intricacy. These structures are believed to record episodic mass loss from the dying star at the nebula’s center, creating a kind of cosmic “fossil record” of its final evolutionary stages.

Combining the focused view of Hubble with Euclid’s deep field observations not only highlights the nebula’s exquisite structure but also places it within the broader context of the universe that both space telescopes explore. Together, these missions provide a rich and complementary view of NGC 6543 — revealing the delicate interplay between stellar end-of-life processes and the vast cosmic tapestry beyond.

Media Contact:

Claire Andreoli
NASA’s Goddard Space Flight CenterGreenbelt, MD
claire.andreoli@nasa.gov

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Last Updated
Mar 03, 2026
Editor
Andrea Gianopoulos

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Smoke Rises Over Big Cypress National Preserve

Smoke Rises Over Big Cypress National Preserve

A satellite image of southern Florida shows white-gray smoke east of the coastal city of Naples. Winds carry the plume northward toward Lake Okeechobee.
February 25, 2026

On February 22, 2026, a wildland fire was discovered in Big Cypress National Preserve, about 25 miles (40 kilometers) east of Naples, Florida. The blaze, dubbed the National fire, moved through dry vegetation and sent a plume of smoke billowing over parts of the preserve and nearby communities. 

The MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Aqua satellite captured this image on the afternoon of February 25. By then, the fire had burned around 24,000 acres (9,700 hectares), according to the National Park Service.

After carrying smoke southward in previous days, winds shifted to start pushing it north by the time Aqua captured this image. According to news reports, the smoke reduced visibility and led to the brief closure of I-75—the interstate nicknamed “Alligator Alley” that runs east-west through the northern part of the preserve. It also contributed to smog over Lake Okeechobee

The fire continued to spread over the next several days, reaching just over 35,000 acres (14,000 hectares) by February 28, according to InciWeb. As of March 2, it remained roughly the same size and was 38 percent contained. 

The fire’s cause remains under investigation. Officials noted, however, that its spread was driven by ample fuel, including vegetation that was dry from persistent, extreme drought and damaged by recent frost. The National Interagency Fire Center’s wildland fire outlook calls for above-normal fire potential across Florida through May.

NASA Earth Observatory image by Lauren Dauphin, using MODIS data from NASA EOSDIS LANCE and GIBS/Worldview. Story by Kathryn Hansen.

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