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Secrets of Living on Mars Deep Underground in the UK

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One-point-one kilometers below the surface, tunnels in North Yorkshire offer a unique opportunity to study how humans might be able to live and operate on the Moon or on Mars. Researchers have now launched the “Bio-SPHERE project” in a unique research facility located, in one of the deepest mine sites in the UK. The project aims to learn how scientific and medical operations would take place in the challenging environments of the Moon and Mars.

In a 4,000-meters-deep underground facility, usually focused on particle physics, Earth sciences and astrobiology research, a team from the University of Birmingham is working in partnership with the Boulby Underground Laboratory. It is the first of a series of new laboratory facilities planned to study how humans might work – and stay healthy – during long space missions, a key requirement for ensuring mission continuity on other planets.
This new capability will help to gather information that can advise on the life support systems, devices and biomaterials which could be used in medical emergencies and tissue repair following damage in deep-space missions.
The Bio-SPHERE project is based in a 3,000-meter tunnel network adjacent to the Boulby Laboratory, which goes through 250-million-year-old rock salt deposits, consisting of Permian evaporite layers left over from the Zechstein Sea. This geological environment, together with the deep subsurface location, have enabled researchers to recreate the operational conditions humans would experience working in similar caverns on the Moon and Mars. This includes remoteness, limited access to new materials and challenges in moving heavy equipment around.

At the same time, thanks to the ultra-low radiation environment provided by that depth, the location will enable scientists to investigate how effective underground habitats might be in protecting space crews from deep-space radiation, which is a significant risk in space exploration, as well as other hazards, such as falling debris from meteorites, which risks damaging the life-support infrastructure.

The first facility to be opened as part of Bio-SPHERE (Biomedical Sub-surface Pod for Habitability and Extreme-environments Research in Expeditions), is based in a 3-meter-wide simulation module and is designed specifically to test biomedical procedures needed to prepare materials for treating tissue damage. These include complex fluids, polymers and hydrogels for regenerative medicine that could be used, for example, in wound dressings, or fillers for damage mitigation.

A paper describing the concept and design of such a habitat was recently published in Nature (NPJ) Microgravity (https://www.nature.com/articles/s41526-023-00266-3).

Bio-SPHERE, which includes a range of capabilities for sterile work and material processing, combines these simulation facilities and useful geological environment with access to the adjacent physics and chemistry laboratory facilities.
In a 4,000-meters-deep underground facility, usually focused on particle physics, Earth sciences and astrobiology research, a team from the University of Birmingham is working in partnership with the Boulby Underground Laboratory. It is the first of a series of new laboratory facilities planned to study how humans might work – and stay healthy – during long space missions, a key requirement for ensuring mission continuity on other planets.
This new capability will help to gather information that can advise on the life support systems, devices and biomaterials which could be used in medical emergencies and tissue repair following damage in deep-space missions.
The Bio-SPHERE project is based in a 3,000-meter tunnel network adjacent to the Boulby Laboratory, which goes through 250-million-year-old rock salt deposits, consisting of Permian evaporite layers left over from the Zechstein Sea. This geological environment, together with the deep subsurface location, have enabled researchers to recreate the operational conditions humans would experience working in similar caverns on the Moon and Mars. This includes remoteness, limited access to new materials and challenges in moving heavy equipment around.

At the same time, thanks to the ultra-low radiation environment provided by that depth, the location will enable scientists to investigate how effective underground habitats might be in protecting space crews from deep-space radiation, which is a significant risk in space exploration, as well as other hazards, such as falling debris from meteorites, which risks damaging the life-support infrastructure.

The first facility to be opened as part of Bio-SPHERE (Biomedical Sub-surface Pod for Habitability and Extreme-environments Research in Expeditions), is based in a 3-meter-wide simulation module and is designed specifically to test biomedical procedures needed to prepare materials for treating tissue damage. These include complex fluids, polymers and hydrogels for regenerative medicine that could be used, for example, in wound dressings, or fillers for damage mitigation.

A paper describing the concept and design of such a habitat was recently published in Nature (NPJ) Microgravity (https://www.nature.com/articles/s41526-023-00266-3).

Bio-SPHERE, which includes a range of capabilities for sterile work and material processing, combines these simulation facilities and useful geological environment with access to the adjacent physics and chemistry laboratory facilities.

AR #129

Hidden Living Space on Moon & Mars

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Loeb’s Spherules from Beyond Solar System, Appear Artificial

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BOSTON, MA — August 29, 2023 — The Interstellar Expedition of June 2023 — led by the expedition’s Chief Scientist, Harvard University Astrophysicist Avi Loeb and coordinated by Expedition Leader Rob McCallum of EYOS Expeditions — retrieved hundreds of metallic spheres thought to be unmatched to any existing alloys in our solar system from the seafloor in the Pacific Ocean near Papua New Guinea. Early analysis shows that some spherules from the meteor path contain extremely high abundances of Beryllium, Lanthanum and Uranium, labeled as a never-seen-before “BeLaU” composition. These spherules also exhibit iron isotope ratios unlike those found on Earth, the Moon and Mars, altogether implying an interstellar origin. The loss of volatile elements is consistent with IM1’s airburst in the Earth’s atmosphere.

The expedition retrieved spherules with a yield per background mass that increased the count of spherules near IM1’s path significantly. Using a heatmap developed from the spherule detection statistics by postdoc Laura Domine, the team was able to identify the regions with a high concentration of the retrieved spherules. The Harvard laboratory team, led by Stein Jacobsen, found “BeLaU”-type spherules of extrasolar composition only in these high-yield regions. “This abundance pattern is unprecedented in the scientific literature and could have originated from differentiation in a magma ocean on an exo-planet with an iron core,” said Stein Jacobsen.

Electron microscope images of some of the collected spherules display lopsided massive composites, indicating mergers of small spherules within the fireball volume. “The “BeLaU” composition is tantalizingly different by factors of hundreds from solar system materials, with beryllium production through spallation of heavier nuclei by cosmic-rays flagging interstellar travel,” said Avi Loeb.

Avi Loeb is the leading author on the expedition team’s paper (linked here), submitted for publication in a peer-reviewed scientific journal. The spherules will continue to be analyzed by four laboratories around the world, at Harvard University, UC Berkeley, the Bruker Corporation, and the University of Technology in Papua New Guinea (Unitech, PNG), using the most advanced instruments of their kind. “Our Vice Chancellor already signed a Memorandum of Understanding on our ongoing partnership with Harvard University,” said Jim Lem, head of the Department of Mining Engineering at Unitech, PNG. “I very much look forward to being part of the team in analyzing the spherules that are believed to have come from outside our solar system and are so rich in scientific information.”
Charles Hoskinson, who funded the expedition, likewise expressed his support for the findings: “This is a historic discovery, marking the first time that humans hold materials from a large interstellar object, and I am extremely pleased with these results from this rigorous scientific analysis.”

According to Expedition Coordinator Rob McCallum: “These results have been well received by the entire expedition team; those onboard and those working onshore. The findings demonstrate the success of the first exploratory expedition and pave the way for a second expedition to seek more data. We love to enable our clients’ projects anywhere on Earth, but this one is out of this world”.

Read more on Professor Loeb’s Medium.com article here https://avi-loeb.medium.com/the-im1-spherules-from-the-pacific-ocean-have-extrasolar-composition-f025cb03dec6.

AR #122

MEGA Engineering In The Stars

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NASA Voyager 1’s Data Anomaly Said Fixed

A critical system aboard the probe was sending garbled data about its status. Engineers have fixed the issue but are still seeking the root cause.

Engineers have repaired an issue affecting data from NASA’s Voyager 1 spacecraft. Earlier this year, the probe’s attitude articulation and control system (AACS), which keeps Voyager 1’s antenna pointed at Earth, began sending garbled information about its health and activities to mission controllers, despite operating normally. The rest of the probe also appeared healthy as it continued to gather and return science data.


The team has since located the source of the garbled information: The AACS had started sending the telemetry data through an onboard computer known to have stopped working years ago, and the computer corrupted the information.


Suzanne Dodd, Voyager’s project manager, said that when they suspected this was the issue, they opted to try a low-risk solution: commanding the AACS to resume sending the data to the right computer.


Engineers don’t yet know why the AACS started routing telemetry data to the incorrect computer, but it likely received a faulty command generated by another onboard computer. If that’s the case, it would indicate there is an issue somewhere else on the spacecraft. The team will continue to search for that underlying issue, but they don’t think it is a threat to the long-term health of Voyager 1.


“We’re happy to have the telemetry back,” said Dodd. “We’ll do a full memory readout of the AACS and look at everything it’s been doing. That will help us try to diagnose the problem that caused the telemetry issue in the first place. So we’re cautiously optimistic, but we still have more investigating to do.”


Voyager 1 and Voyager 2 have been exploring our solar system for 45 years. Both probes are now in interstellar space, the region outside the heliopause, or the bubble of energetic particles and magnetic fields from the Sun.
For more information about the Voyager spacecraft, visit: https://www.nasa.gov/voyager


https://www.jpl.nasa.gov/news/engineers-solve-data-glitch-on-nasas-voyager-1

AR Issue #57

Project Stardust

by William Henry