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University Team Proposed Retractable, Pressurized Tunnels for Missions to Mars
NASA and China’s national space agency plan to send crewed missions to Mars in the coming decades. Per NASA’s Moon to Mars mission architecture, this will involve using infrastructure established through the Artemis Program to send crews to the Red Planet sometime in the 2030s or 2040s. Similar to Artemis, these missions will culminate in the creation of habitats that will facilitate long-duration exploration and research. Naturally, this presents many challenges, including lengthy deep-space transits and the hazards of extended periods in microgravity.
However, crewed missions will also face significant challenges upon arrival, such as the dangers of working in Mars’ thin, unbreathable atmosphere, extreme temperature variations, and elevated radiation levels. Fortunately, these challenges are inspiring innovative concepts from space agencies, their affiliated research institutes, and commercial partners. In a recent report, the Bioastronautics and Life Support Systems (BLiSS) team at the University of Michigan proposed an active, pressurized tunnel system to connect habitats on the Martian surface.
Their concept is described in the paper “LATCH: Lightweight Actuated Tunnels for Crewed Habitation,” which was submitted to the annual Moon to Mars eXploration Systems and Habitation (M2M X-Hab 2026) Academic Innovation Challenge. The report is one of several projects NASA selected under the X-Hab program, an incentive challenge administered by the National Space Grant Foundation (NSGF) that invites university students nationwide to provide concepts prototypes, and lessons learned that will help shape future space missions.
*Full Tunnel Extended with Components Labeled. Credit: BLiSS team/NTRS*
Dr. Nilton Renn, the John R. Barker Collegiate Professor in Planetary Sciences and Space Engineering at the University of Michigan, is the BLiSS team’s Principal Investigator. Dr. Tracie Prater, an esteemed aerospace and mechanical engineer at NASA’s Marshall Space Flight Center and a materials and processes engineer at United Launch Alliance, served as the Project Sponsor.
Challenges
Regardless of the location – the Moon or Mars – maintaining a continuous human presence requires a lot of movement. This means the movement of crews and cargo from the surface to orbit, and between surface assets – i.e., habitats, vehicles, landing pads, etc. Given the nature of the lunar and Martian environments, this will require crews to don spacesuits and conduct Extravehicular Activities (EVAs) every time. This is a time-consuming process that requires hours of preparation (pre-breathing oxygen), suiting up, airlock depressurization, and post-EVA cleanup.
This process takes a full day to complete, and also places crewmembers at risk of decompression and exposure to elevated radiation. Similarly, crews must remain in their spacesuits when entering or leaving the Mars Ascent Vehicle (MAV), which is cumbersome given the size of the suits themselves. The need for pressure suits during ascent and descent also adds mass to the vehicle’s overall load, increasing costs and the propellant required. As the team describes in their report:
In fact, preliminary analysis of the Mars Ascent Vehicle (MAV) used by crew to get to and from the Martian surface shows that each EVA suit requires 560 kilograms more propellant than an Intra-Vehicular Activity (IVA) suit would require. Additionally, EVA suits take up volume in the launch vehicle, roughly the size of a person. This would require a larger cabin size, which in turn would require more propellant mass.
To eliminate this burden, the HATCH team proposed a “lightweight pressurized tunnel system [which can] provide active positioning and berthing between crewed surface assets on Mars.” This concept would consist of tunnels that could be deployed as needed for transits, then retracted when not in use. Such tunnels would reduce transit times to and from habitats and landing pads from a full day to just a few minutes.
“The project calls for the development of concepts for a ‘lightweight pressurized tunnel system’ which can ‘provide active positioning and berthing between crewed surface assets on Mars,'” the team writes.
*Full Tunnel Model with Different Views. Credit: BLiSS team/NTRS*
Design
Each tunnel consists of an inflatable shell, structural rings, a passive extension mechanism (driven by motors and actuators), extendable handrails and tracks, and tread units mounted to each section. These tunnels are then integrated with each airlock on the habitat, which the crew can extend using the User Interface (UI). The UI will also allow crew members and ground controllers to view the tunnel’s status, which will be routinely monitored by sensors for leakage, contamination, or system faults.
The process begins with the crew member selecting a destination (the MAV or another surface element), then instructing the UI to extend the tunnel towards its hatch. The passive extension mechanism also allows crew members to make fine adjustments to its path, while sensor data and ground-controller monitoring provide feedback for alignment and trajectory correction. Once the tunnel is fully extended and both ends are secured, the tunnel will slowly pressurize with oxygen and nitrogen gas.
Once pressurized and the environment is confirmed safe by the sensors and ground control, the tunnel is used to allow up to two crew members to walk through it carrying cargo. During their transit, crew members not using the tunnel will be informed by the UI of any sudden safety issues. In the event of an emergency, alert systems will be activated automatically (lights, handrails, and other needed support systems) to help ensure the crew members safely reach the other side of the tunnel.
When not in use, the tunnels will be depressurized and retracted. This will prevent the tunnels from accumulating radiation inside and Martian dust on the outside. Maintaining them in the retracted position between usage also ensures that they are less vulnerable to debris damage.
Testing and Risk Assessment
As part of their proposal, the BLiSS team provided full Computer-Assisted Design (CAD) models and a prototype demonstrator of the tunnel and actuation system (along with the control software) for testing. In addition, a comprehensive risk matrix was developed to identify and assess potential hazards that could impact the success of future missions. This allowed the BLiSS team to identify various technical, schedule, cost, and safety-related risks that could compromise the functionality and safety of their system.
One notable risk involved the possibility of the structure yielding while astronauts are inside, leading to potential injury or death. To mitigate this, they proposed adding additional floor beams and/or a roll-out floor to support increased loads or accidents (e.g., cargo being dropped). The team also took measures to mitigate the risk of inaccurate berthing that could render the system unusable, including a multi-sensor fusion approach using LiDAR and computer vision. This would allow for cross-validation between sensors, enabling course correction and fine-motion detection.
*Prototype of a two-tendon actuator showing the system components and independent articulation of each segment. Credit: Baldwin Wallace University team/NTRS*
“By implementing robust mitigation measures and continuously monitoring and reassessing risks throughout the project life cycle, we aim to minimize disruptions and maximize the effectiveness of our tunnel system in supporting crew transportation between surface assets during space missions,” they state.
A similar concept submitted by the Baldwin Wallace University Engineering Department was the Tunnel Ready Elements for Active Deployment (T.R.E.A.D). Their concept is also in keeping with the goals of the 2026 M2M X-Hab Challenge: to create a system of extending tunnels that will connect surface elements on Mars, emphasizing reusability and preventing the accumulation of buildings and tunnels on the surface that no longer serve mission objectives.
For their proposal, the Baldwin Wallace team conceived a double-tendon-based actuation system with pressurized bladders. Each set of tendons consists of four individual cables controlled via a winch system, with the first set controlling the initial half of the tunnel’s curvature and the second controlling the final stretch. The tendon system also serves as a primary means of retraction and provides the necessary flexibility to bend and adjust to uneven terrain.
These and other concepts are merely some of the latest proposals for how astronauts will live and work in the extraterrestrial environment of Mars. As the 2030s approach, NASA and other space agencies will continue to ramp up their preparations for sending crewed missions to the Red Planet. The methods used and the lessons learned from these missions will likely inform the blueprint for off-world living should humanity embark on a path that leads us to become “interplanetary” someday.
Further Reading: NASA Technical Reports Server (NTRS)
News
Two Million X-Ray Sources, and One Cluster That Doesn’t Fit
Clusters are the largest gravitationally bound things in the universe, thousands of galaxies held together in a vast reservoir of hot gas, gas so hot it glows in X-rays rather than visible light. But they do not stop at a tidy, neat edge. They taper away into the surrounding darkness, and they are still being fed, drawing in fresh material along enormous threads of gas that run between them like the strands of a web. Those outskirts are the interesting part, because they are where the universe is still assembling itself. They are also very faint, which is why so little is known about them.
The eROSITA telescope, launched in 2019 aboard the joint Russian and German Spektrum-RG mission, has now published its second major data release. Built from three complete surveys of the sky, DR2 contains close to two million X-ray sources across the western half of the sky, about twice as many as the first release. Roughly 1.9 million are point like, mostly stars and feeding supermassive black holes. Some 64,000 are extended: galaxy clusters, nearby galaxies and the shredded remains of supernovae.

Galaxy cluster A3266 in X-rays, linked by a filament of hot gas to a neighbouring galaxy group. The Bonn team measured the faint outer glow for the first time and found gas hotter and denser than the models predict (Credit : Jakob Dietl/Uni Bonn/eROSITA-DE)
Within that haul, Thomas Reiprich and Jakob Dietl at Bonn’s Argelander Institute went after a single object. A3266 is a massive cluster connected by a filament of gas to a neighbouring group of galaxies, and their team became the first to measure the faint X-ray glow in its outer reaches.
Our current theories of how cosmic structure formed match what eROSITA sees, that’s reassuring. The interesting news is in the detail, where they don’t quite match. The gas in the outskirts and in the filament runs hotter and denser than predicted, and contains comparatively little in the way of heavy elements.

The Perseus cluster, one of the brightest X-ray objects in the sky. The diffuse glow is gas hot enough to shine in X-rays, and it holds more mass than all the cluster’s stars together (Credit : X-ray: NASA/CXC/SAO/V. Olivares et al.; Optical/IR: DSS; H-alpha: CFHT/SITELLE; Image Processing: NASA/CXC/SAO/N. Wolk)
Heavy elements, anything past hydrogen and helium, are manufactured inside stars and flung out when those stars die. Gas that is short of them has therefore never spent much time near a galaxy, which marks it as relatively pristine material arriving from the wider cosmic web rather than something expelled from the cluster itself. Yet it’s warmer and denser than models predict for gas of that kind. The two facts pull against each other, and reconciling them means adjusting our picture of how matter actually falls into a cluster: how quickly it heats, how thoroughly it mixes with what is already there and how much enriched gas the galaxies push back out to meet it.
Before eROSITA, the only X-ray survey of the whole sky came from ROSAT in 1990, so astronomers waited the best part of three decades for a successor. And eROSITA itself has been in safe mode since February 2022, with no return to science operations. There is a lesson in that about the value of surveying everything, whether or not you know yet what you are looking for.
Source : Homing In on the X-Ray Sky
News
L.A. reaches deal on cost recovery for 2028 Olympics, amid warnings

A divided Los Angeles City Council finalized a deal with organizers of the 2028 Summer Olympic Games aimed at controlling the city’s costs during the global event, amid complaints that the protections don’t go far enough.
On a 10-4 vote, the council approved the Enhanced City Resources Master Agreement, which lays out the process for the city to seek reimbursement for the services it provides during the Games.
City Administrative Officer Matt Szabo said the agreement sets up additional financial safeguards, by allowing the city to tap a $270-million contingency fund set up by LA28, the privately run Olympic organizing committee, if outstanding costs remain.
Still, some on the council warned that taxpayers could wind up on the hook for $1 billion in police and other public safety costs if LA28 incurs serious losses.
“This fails to provide any safeguards for Los Angeles taxpayers and most assuredly risks the city’s fiscal stability,” Councilmember Monica Rodriguez said after voting against the agreement. Councilmembers Eunisses Hernandez, Ysabel Jurado and Nithya Raman, who is running against Mayor Karen Bass, also were opposed.
Critics of the Games have long voiced concern about the risks that surround the event.
If LA28 incurs massive financial losses, the city would cover the first $270 million. The state would absorb the next $270 million. After that, the city’s general fund, which pays for basic services, would cover any remaining shortfall.
The city’s negotiating team said L.A.’s political leaders committed the city roughly a decade ago to serve as a financial backstop for the Games, as part of the contract that made L.A. the host city.
“We are providing you today as many protections as we can, given the reality that if it is not financially successful, it does fall onto us,” Szabo said. “So there is nothing we could propose today or tomorrow or next year that would eliminate that risk.”
The council, in a flurry of votes, sidelined proposals from Councilmembers Imelda Padilla, Hernandez and Raman that were billed as a way to reduce the risk facing the city.
LA28 spokesperson Jacie Prieto Lopez, in a statement, said the newly approved agreement delivers on the committee’s commitment to “execute a safe, secure and fiscally responsible Games that benefit Los Angeles for decades to come.”
Under the terms approved by the council, LA28 would pay the city ahead of the Games for services that are ineligible for reimbursement from the federal government, such as street sweeping and deployment of traffic officers.
The terms around police protection are more complicated.
The city would first seek reimbursement from the federal government for law enforcement services, particularly in high-security zones, Szabo said. If the government fails to cover the cost of security in those areas, the city would seek all or a portion of LA28’s contingency funds to make up difference, he said.
Last year, President Trump signed the One Big Beautiful Bill Act, setting aside $1 billion for state and local governments for security, planning and other costs associated with the Games.
Some council members have voiced concerns that the federal government might not follow through on its commitment, or that only a fraction of those funds would make their way to L.A., one of several Southern California communities slated to host Olympic competitions.
In April, Rodriguez sent LA28 a letter warning the city’s public safety costs could easily blow past $1 billion if there is an emergency or major weather event.
City Controller Kenneth Mejia, in an interview, said he intends to use his office to look into LA28’s finances in the run-up to the Games. He also argued that the deal to secure the Olympics was a bad one from the beginning.
“We’re already locked into a huge financial liability. This was one of our big chances to throw in protections for the city and also provide that transparency,” said Mejia, who opposed the agreement.
If LA28 makes money on the Games, the organizing committee would be barred from distributing that surplus to any organization until it has covered its financial obligations to the city, according to the terms approved Wednesday by the council.
Szabo, appearing before the council, acknowledged that the city faces a financial risk. If LA28 does experience a financial loss, it first would tap its own $330-million contingency fund, he said.
After that, LA28 and the city would have access to a second, $270-million contingency fund set up to protect taxpayers, he said.
“Is that a likely scenario? We don’t believe so,” Szabo said. “Their reports thus far have suggested that they are meeting their targets on their sponsorships and on other revenues, and we want them to continue to hit their targets.”
Those arguments haven’t satisfied an array of activists, who urged the council to rewrite the agreement.
“LA28 has no incentive to keep the city from being forced into bankruptcy,” said Chris Tyler, spokesperson for Strategic Actions for a Just Economy, a nonprofit that advocates for low-income communities in L.A.
Under a deal reached in 2021, LA28 must reimburse the city for services that go beyond what would be provided on a normal day in key parts of the city, such as Exposition Park, the Sepulveda Basin and parts of downtown L.A.
The organizing committee is obligated to create a $270-million contingency fund that can be distributed as a surplus if the Games make money or cover any losses in the event of a shortfall.
The proposal approved Wednesday calls for the five-year-old agreement to be amended to ensure that those contingency funds can be used to cover the city’s costs in the event that other funds aren’t available.
The city and LA28 were supposed to have a draft agreement on the cost recovery process completed by October. A draft document did not surface until June.
City negotiators now head into another round of talks with LA28 on the precise level of services needed at the Convention Center, Venice Beach, Dodger Stadium and other locations. Those venue agreements must be completed in July 2027.
Under the terms approved Wednesday, the two sides must reach an accord on the cost of those additional services by October 2027.
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