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Another Success for Hayabusa 2 as it Completes a Flyby of Asteroid Torifune
Hayabusa 2’s primary mission is well in the past, now. JAXA’s asteroid sampling spacecraft rendezvoused with asteroid Ryugu back in June 2018. It studied the asteroid for 1.5 years and gathered a sample which was returned to Earth in December 2020.
After that successful endeavour, Hayabusa 2 was sent on its way to visit other targets, though another sample-return is not possible. It’s on its way to visit a tiny asteroid called 1998 KY26, a near-Earth object (NEO) only about 11 meters in diameter. But on its way, it also flew past another asteroid named Torifune (98943 Torifune).
Ground-based observations showed that Torifune is a near-Earth asteroid (NEA) measuring about 450 meters in diameter. It’s an S-type asteroid, meaning its a stony-type or siliceous-type. These are high-density objects that make up about 17% of the asteroid population, making them the second most common type after carbonaceous C-type asteroids.
*These are two different top-down ways of envisioning Hayabusa 2 and asteroid Torifune. The left panel shows a view in a frame that rotates with Earth’s orbit. The right panel shows a stationary frame. Image Credit: By Original by Hirabayashi et al. 2026, modified by Nrco0e – Modified from Figure 2 of https://arxiv.org/html/2604.08832v1, CC BY 4.0, https://commons.wikimedia.org/w/index.php?curid=189386318*
Hayabusa 2 began looking at Torifune in June with its Optical Navigation Camera – Telescopic (ONC-T). The ONC-T directly imaged Torifune on June 20th for navigation purposes.
Then on July 5th, Hayabusa 2 came to within about 800 meters of the asteroid. It used ONC-T to capture images of Torifune that revealed details about its surface. While ground-based observations showed the asteroid was elongated, hinting at its contact binary nature, only these images confirm it. In contact binaries, two separate asteroids orbited a common center of mass until they spiralled in towards each other and joined into one. Contact binary asteroids aren’t expected to be rare.
Beginning at about one hour before closest approach, Hayabusa 2 also observed Torifune with its other instruments, the NIRS3 (Near-Infrared Spectrometer), TIR (Thermal InfraRed Imager), and LIDAR (Light Detection and Ranging).
*Hayabusa 2 also imaged asteroid Torifune with its Thermal InfraRed Imager (TIR). This TIR image is from about 10 km away. Image Credit: JAXA, Maebashi Institute of Technology, Chiba Institute of Technology, The University of Aizu, Hokkaido University of Education, AIST*
Hayabusa 2 was travelling very fast during this flyby. Its relative speed was 5 km/s (3.1 mi/s), making navigation and image capturing challenging. It has less than half of its xenon propellant remaining, enough to power its ion thrusters to meet Torifune and 1998 KY26, but not enough for any extra maneuvers.
Hayabusa 2’s next milestone will be in December 2027 when it swings past Earth. Then in June 2028, it will swing by Earth again. That will set it up for its rendezvous with 1998 KY26 in July 2031.
The exact nature of 1998 KY26 isn’t clear. Observations in optical and radar suggest that it’s a water-rich asteroid, and since it’s known to be a fast-rotator, it’s almost certainly one single chunk of rock rather than a rubble pile asteroid. It could also potentially be an X-type asteroid, which is a catch-all term that encapsulates objects that look similar through a telescope but are composed of different materials.
All of Hayabusa 2’s data from its flyby of Torifune has not yet reached Earth, so these are preliminary results. JAXA will release more in the near future.
News
Ex-SoCal sheriff’s deputy shoved detainee, whose spine fractured. He’s going to prison
A San Diego County Sheriff’s Department then-deputy shoved a pretrial detainee from behind while his legs were shackled and his hands chained at the waist, causing the man to “fly across his holding cell, headfirst into the far wall and collapse to the ground,” according to prosecutors.
The man’s spinal column was fractured. The deputy then attempted a cover-up.
Jeremiah Manuyag Flores, 45, of La Jolla was sentenced on Tuesday to four years and nine months in prison for the incident that occurred in August 2024.
The victim lay in a pool of his own blood for more than two hours before being found by another deputy. In a report that Flores was directed to fill out about his interactions with the detainee, referred to in court documents as J.P, the defendant made “multiple false statements, including, ‘no force was used,’” prosecutors said.
A still shot from a surveillance camera showed Flores walking away from the detainee’s cell following the incident with a smile on his face. During Flores’ sentencing, U.S. District Judge Linda Lopez said, “I don’t know how many years it’s going to be before I get that photo out of my mind. Your conduct was egregious.”
In a federal investigation, Flores was charged with the deprivation of rights under color of law and falsification of records. He was found guilty in December 2025 on both counts by a jury after just two hours of deliberations, according to the U.S. attorney’s office for the Southern District of California.
In a statement, the San Diego County Sheriff’s Department condemned the actions of its former deputy, saying “his actions do not reflect the values of our organization” and that “our agency does not tolerate the use of excessive force or lying by deputies.” The department said that, as a result of an internal investigation, Flores was effectively terminated from his role at the department on June 9 of this year.
Because of the convictions, Flores will no longer be eligible to work for law enforcement at any level, including local, state and federal agencies.
Flores, who had been out of jail on bond, was ordered to begin his prison sentence on Aug. 18.
News
Louise Lasser, Star of TV’s ‘Mary Hartman,’ Is Dead at 87
She began her screen career in Woody Allen movies (he was also her husband), but she was best known for her portrayal of the Ohio housewife in the pigtails and puffed sleeves.
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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)
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