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Sudden drop just before 1990..
The global decline in bauxite mining in and around 1990 was primarily due to a stagnating demand for primary aluminum, which resulted in a worldwide oversupply of the metal and structural changes in the global market.
Specific factors contributing to the drop include:
Global Overcapacity: Additions to aluminum production capacity were larger than the increase in demand, leading to an oversupply that reduced prices and the need for new bauxite.
Increased Competition: Traditional producers, particularly in the Caribbean and the U.S., faced increased competition from other bauxite-endowed countries like Australia and Brazil, which had cost advantages.
Economic Transition in Eastern Europe: The dissolution of the Eastern Bloc and the war in former Yugoslavia seriously affected production in those regions, and the subsequent export of cheap aluminum from former USSR republics into Western markets contributed to the global glut.
Domestic U.S. Factors: In the United States, a significant reduction in domestic production in 1990 was attributed to the permanent closure of the last major bauxite mining operation in Arkansas. The U.S. became highly dependent on foreign bauxite sources, with most domestic output used for non-metallurgical products.
Operational Inefficiencies: Some countries, like Guyana, faced loss of market share due to un-competitiveness and inefficient management under state ownership
So the stagnation was due to importing being cheaper most likely.
A Mars airlock to a 7.5 psi dome entrance involves a crucial pressure transition, requiring robust, sealed systems like those simulated in *Space Engineers* or *Stationeers, using inner/outer doors, vents, sensors, and timers to cycle air from the low-pressure Martian exterior (around 0.1 psi) to the pressurized habitat (7.5 psi) while filtering dust, ensuring safety and breathable air, often with automated sequences for seamless, efficient passage.
Key Components & Functions:
Dual Doors: An inner door (habitat side) and an outer door (exterior side) to create a sealed chamber.
Airlock Chamber: The space between the doors, containing sensors and vents.
Vents & Pumps: Active vents manage air flow; pumps rapidly depressurize or fill the chamber with the habitat's air (or Martian CO2 for initial pressurization).
Sensors & Timers: Detect occupants, monitor pressure, and automate the sequence (e.g., outer door opens when depressurized, inner opens when pressurized).
Dust Filtration (Air Showers): Critical for Mars to prevent corrosive dust from entering habitats.
Operational Sequence (Pressurization Example):
Entry: Person enters from the Martian surface (low pressure) into the airlock, closing the outer door.
Depressurization (if needed): Air vents to the outside or is pumped out.
Pressurization: Air from the 7.5 psi dome is let into the chamber via a controlled valve.
Inner Door Opens: Once pressure matches the habitat, the inner door unlocks and opens, allowing passage.
Key Considerations for 7.5 psi:
Pressure Differential: The system must handle the significant pressure difference between the near-vacuum of Mars and the 7.5 psi of the dome.
Martian Dust: Requires advanced filtering (HEPA) and possibly air showers to keep interiors clean and equipment safe.
Automation: Sensors and programmable logic (like in game simulations) ensure smooth, safe transitions without human error.
This system ensures life support, environmental control, and protection from the harsh Martian conditions while allowing continuous access to the habitat
So the habitat air is purged from inside the air lock and drawn down to mars entry levels which is then once door closed to the outside is then back filled to the dome pressure.
Mars' atmosphere is overwhelmingly carbon dioxide (\(CO_{2}\)), about 95-96%, with trace amounts of carbon monoxide (\(CO\)) around 0.06% to 0.09% by volume, but the total atmospheric pressure is extremely low, less than 1% of Earth's, making \(CO\) content small in absolute terms. The pressure fluctuates seasonally, averaging around 6-7 millibars (mbar), but this is still very thin, meaning even 95% \(CO_{2}\) doesn't create intense greenhouse effects like on Venus. Key Figures: Carbon Dioxide (\(CO_{2}\)): ~95.3%Nitrogen (\(N_{2}\)): ~2.7%Argon (Ar): ~1.6%Oxygen (\(O_{2}\)): ~0.16%Carbon Monoxide (\(CO\)): ~0.06% - 0.09%Water Vapor (\(H_{2}O\)): ~0.03% (variable)
so each small chamber builds up what could be poisonous to the crew inside the dome.
Gasses inside are hot so they float to the top of the dome accumulating. Cold gasses sink and can come from the floor building up over time.
other is from bacteria and plant growth plus from the humans that are inside.
Also this was the heat source from burning methane for the food soil growth cells to keep temperature to create co2 but incomplete burn makes Co...
Human respiration primarily involves taking in oxygen and exhaling carbon dioxide and water vapor, but the air we breathe out is a mixture containing nitrogen, unused oxygen, and trace amounts of other waste gases like volatile organic compounds (VOCs), nitric oxide (NO), and ammonia (NH3). While carbon dioxide is the main waste product of cellular respiration, exhaled air still contains a significant amount of nitrogen (about 78%) and some oxygen (around 16%).
Key Gases Given Off Carbon Dioxide (\(CO_{2}\)): The primary waste gas, produced when cells use oxygen to break down sugar for energy.Water Vapor (\(H_{2}O\)): A byproduct of cellular metabolism, released as humidified vapor.
Nitrogen (\(N_{2}\)): The most abundant gas in the air, most of which is exhaled unchanged, as humans don't use it.Oxygen (\(O_{2}\)): A portion of the oxygen we inhale isn't used and is exhaled, which is why rescue breaths in CPR can still provide oxygen.
Trace Gases: Small amounts of other substances, including:Volatile Organic Compounds (VOCs).Nitric Oxide (NO).Ammonia (NH3).Carbon Monoxide (CO).Alcohol (when consumed).
The Process Inhalation: Air (21% Oxygen, 78% Nitrogen, ~0.04% Carbon Dioxide) enters the lungs.
Gas Exchange: In the alveoli (tiny air sacs in the lungs), oxygen moves into the blood, and carbon dioxide moves from the blood into the alveoli.
Exhalation: The diaphragm and chest muscles push air out, carrying the waste \(CO_{2}\) and water vapor, along with unused nitrogen and oxygen, out of the body
The cost comparison between mining bauxite and importing it is complex and depends heavily on location, quality of the bauxite, and market conditions. Generally, mining bauxite can be cheaper than importing it, but only if significant domestic reserves and infrastructure are available.
Cost Breakdown: Mining vs. Importing
Mining Bauxite: Initial mining costs for high-volume producers can be low, sometimes under $30 per ton. However, this requires substantial initial investment in infrastructure, equipment, and compliance with environmental regulations.
Importing Bauxite: Import prices can fluctuate significantly based on global supply and demand, geopolitical factors, and freight costs. Recent (2024/2025) average import prices (free alongside ship, or f.a.s./FOB) in the U.S and China have ranged from approximately $30 to over $100 per ton, with prices recently peaking at $115–$130 per mt in early 2025 due to supply disruptions
Global Imported Bauxite Prices Remain Stable at $74/mt
So if you want lower costs you do not invest in capital equipment and fights against mining regulations.
The U.S. primarily relies on imported bauxite (aluminum ore) for its aluminum production, though small amounts are mined domestically for non-metal uses like abrasives and proppants in oil/gas drilling. Arkansas has historically been the main U.S. source, but mining for metal ceased years ago, with the nation now depending on imports from countries like Jamaica, Guinea, and Brazil for its refineries, mainly in Louisiana.
Key Points:
Primary Ore: Bauxite, a rock rich in aluminum hydroxides (gibbsite, boehmite, diaspore).
Domestic Mining: Limited; primarily for non-metallurgical uses like refractories or hydraulic fracturing proppants, not primary aluminum.
Main Source: Imports, with significant quantities coming from Jamaica, Guyana, China, and Australia.
Refining: U.S. alumina refineries are in Louisiana, converting imported bauxite into alumina for smelting.
Energy Intensive: Aluminum production is energy-intensive, making electricity costs a major factor in U.S. smelter operations.U.S. Bauxite Resources:
Arkansas: Historically the largest domestic producer, but mining for metal stopped in the 1980s.
Other States: Small deposits exist in Alabama, Georgia, and other areas, but aren't major suppliers for metal production.
In essence, while the U.S. consumes and produces aluminum, it relies heavily on foreign sources for the raw bauxite ore.Yes, the U.S. has bauxite, primarily in Arkansas, Alabama, and Georgia, but production is small and mostly for non-metallurgical uses like chemicals, abrasives, and proppants for fracking; the nation imports the vast majority of its metallurgical-grade bauxite for aluminum production from other countries like Jamaica, Guinea, and Brazil.
Key Details:
Domestic Production: Small amounts are mined in the Southeastern U.S., with Arkansas being the leading domestic producer, though not for primary aluminum metal in recent decades.
Uses: U.S. bauxite is used for chemicals, abrasives, cements, and hydraulic fracturing proppants, not as much for aluminum metal as in the past.
Imports: The U.S. relies heavily on imports for aluminum, with significant quantities of metallurgical bauxite coming from global suppliers.
History: Major U.S. bauxite mining for aluminum happened in the past, especially in Arkansas, but stopped in the 1980s for metal production.
Mean mining needs to increase within the US
If air locks are well as soil seepage happens then Co will be present. Plus acidents of paper and other things can burn with in the domes atmosphere.
Mars' atmosphere is overwhelmingly carbon dioxide (\(CO_{2}\)), about 95-96%, with trace amounts of carbon monoxide (\(CO\)) around 0.06% to 0.09% by volume, but the total atmospheric pressure is extremely low, less than 1% of Earth's, making \(CO\) content small in absolute terms. The pressure fluctuates seasonally, averaging around 6-7 millibars (mbar), but this is still very thin, meaning even 95% \(CO_{2}\) doesn't create intense greenhouse effects like on Venus. Key Figures: Carbon Dioxide (\(CO_{2}\)): ~95.3%Nitrogen (\(N_{2}\)): ~2.7%Argon (Ar): ~1.6%Oxygen (\(O_{2}\)): ~0.16%Carbon Monoxide (\(CO\)): ~0.06% - 0.09%Water Vapor (\(H_{2}O\)): ~0.03% (variable)
Suppose we did simply create an open pit "mine" of the kind shown by SpaceNut in Post #30. The "Superdome" that Calliban want to build is merely a means to an end- pressurized living space, presumably appropriately "greened" using seeds brought from Earth. Apart from holding in the pressure, I presume the most important secondary reason for piling on so much regolith over the structure is to block-out space-based radiation, primarily the highly penetrating and damaging (slowly but surely) Galactic Cosmic Rays (GCR). All available literature from NASA indicates that using approximately 2m of regolith shielding is sufficient to absorb enough of the dose to remain below lifetime limits. GCR is not like SPE / CME radiation, in that it consists of ionized nuclei, ranging in weight from Hydrogen to Iron, although it's over 90% Hydrogen in practice, traveling through space near the speed of light. There's no practical passive shielding material for an interplanetary spacecraft due to shielding mass, but once the settlers arrive on Mars we're obligated to provide appropriate protective measures incorporated into the engineering of habitable spaces.
Here's a question I'd like the AI to answer for us:
By constructing Calliban's Superdome at the bottom of the open pit mine shown in Post #30, how much Solar Particle Event (SPE) / Coronal Mass Ejection (CME) / Galatic Cosmic Ray (GCR) radiation will the open pit mine block by erecting the dome at the bottom of the pit?If the protection provided is still insufficient for humans, is it enough for the plants to survive all or most SPE / CME / GCR?
Maybe the humans will still need to temporarily seek more substantial shelter during a SPE / CME, presumably by evacuating to tunnels carved into the rock underneath the dome or into the walls of the pit. I'm thinking of the open pit mine as being somewhat akin to "castle walls", used to protect the people inside from powerful space-based radiation rather than invaders, but a castle nonetheless. The Superdome at the bottom is the castle's "keep"- for keeping the people inside warm / fed / clothed.
Erecting a giant dome is supposed to be a significant quality of life improvement for the settlers, so if it still gets sufficient sunlight to grow plants using fiber optics and/or mirrors arrayed around the pit, then perhaps the effort to dig the pit and erect the Superdome at the bottom of the pit still represents an acceptable energy trade for the long term security and psychological support of a miniature Earth-like environment.
Its is a far less requirement than 10M of regolith to just move only 2 Meter to do protection for the spiral road around the dome for compression and protection.
A comprehensive iron ore processing and steel production facility on Mars would require an integrated suite of mining, comminution, beneficiation, and refining equipment. A 200-meter diameter is a massive scale, likely referring to the entire facility's footprint rather than a single piece of equipment, and would enable significant production capacity.
Required Equipment: The equipment would function in a sequence from raw material extraction to finished product, much like on Earth, but adapted for the Martian environment and the use of in-situ resources.
1. Mining and Raw Material Handling Excavation and Loading: Robotic rovers and excavators with magnetic systems could collect iron-rich regolith or access concentrated ore deposits.
Transportation: Robust, self-driving transport systems (e.g., heavy-duty rovers or a rail system) to move ore from the mine to the processing plant.
Crushing and Grinding: Equipment such as jaw crushers, hammer mills, and ball mills would be needed to break down the iron ore into fine particles for processing.
2. Beneficiation and Concentration Sizing and Screening: Vibrating screens and classifiers to sort particles by size.
Separation: Magnetic separators are key for iron ore beneficiation, potentially complemented by flotation equipment, to increase the iron concentration in the ore.
Dewatering/Filtration: Equipment like filter presses or vacuum filters would be necessary if wet processing is used, to remove water from the concentrated ore.
3. Iron & Steel Production Martian steelmaking would likely favor direct reduction or electric arc furnaces over traditional blast furnaces due to the lack of abundant coking coal and the availability of atmospheric \(\text{CO}_{2}\) and water ice for reactants/power generation.
Ore Agglomeration: Pelletizing or sintering machines to form the fine concentrate into larger, usable pellets.
Reduction Reactors/Furnaces:Direct Reduction Kiln: Equipment to reduce iron oxides using hydrogen and/or carbon monoxide derived from Martian resources.
Electric Arc Furnace (EAF): An EAF would melt the sponge iron (produced from direct reduction) and allow for the controlled addition of carbon (extracted from the Martian atmosphere's \(\text{CO}_{2}\)) and other alloying elements to produce specific steel grades.
Continuous Caster/Molds: Machinery to form the molten steel into basic shapes (e.g., billets, slabs) for further processing.
Ladle Furnace: Used for final refining of the steel.
4. Manufacturing and Finishing Rolling/Finishing Mills: Large mills to shape the raw steel into plates, sheets, beams, or pipes.Additive Manufacturing (3D Printing): Metal powder bed fusion or directed energy deposition machines could use the produced steel powder for on-site fabrication of parts and infrastructure. Infrastructure and Support Equipment Power Systems: The entire process requires enormous amounts of power, suggesting large-scale nuclear fission reactors or extensive concentrating solar power (CSP) fields and storage systems.
Gas Processing Plant: A complex system involving electrolysis cells (like NASA's MOXIE technology) and chemical reactors (e.g., Sabatier reaction) to produce the necessary oxygen, hydrogen, and carbon monoxide from the Martian atmosphere and water ice.Habitat and
Maintenance Facilities: Pressurized environments, repair shops, and storage facilities for personnel and spare parts.Fume Extraction Equipment: Systems to manage and clean process gases, essential for operational efficiency and safety in a closed environment
Russia’s bold plan to recycle ISS modules for new space station, will it work?
Russia’s Roscosmos is taking an unconventional route to its new space station, by recycling old modules from the International Space Station (ISS). With the ISS slated for retirement, Roscosmos has announced plans to repurpose several modules from the Russian segment of the station, marking a significant shift in the country’s space station strategy.
The new Russian Orbital Station (ROS) will incorporate modules like Zarya, Zvezda, Poisk, Rassvet, Nauka, and Pricha. These aging structures, which have been orbiting Earth for nearly 30 years, will be separated from the ISS once the program concludes, forming the heart of the new station. It’s a move that raises questions about the long-term durability of these modules and the scientific viability of the station as a whole.
A Shifting Vision for Russia’s Space Future
For years, Roscosmos has been toying with the idea of an independent space station. Initially, the Russian Orbital Service Station (ROSS), a successor to the Orbital Piloted Assembly and Experiment Complex (OPSEK) project, was supposed to be entirely new, free of the ISS’s aging modules. But by 2021, the plan shifted to an even bolder vision: creating a new space station using some of the hardware that has already been in orbit for decades.
According to the report published inUniverse Today, the re-use of ISS modules marks a significant departure from Roscosmos’ previous plans, and according to a recent statement from Oleg Orlov, director of the Institute of Biomedical Problems at the Russian Academy of Sciences (RAS), the decision reflects the growing financial constraints and geopolitical shifts the country has faced in recent years.
With many of the ISS modules showing their age, particularly the Russian ones, it may seem like a cost-effective move, but some experts are skeptical of just how feasible it is to recycle these old, often problematic pieces of hardware.
Aging Modules and Serious Concerns
While the idea of recycling ISS modules may seem like a quick fix, there are significant concerns about the condition of the modules Roscosmos plans to repurpose. As Maria Sokolova of New Izvestia pointed out, some of the Russian modules are well over 25 years old and have suffered considerable wear and tear. The Zarya module, for instance, is 27 years old, and Zvezda, which is another key module for the new station, is not far behind.These modules were designed for a much shorter operational lifespan, and the harsh conditions of space, including extreme temperature fluctuations and radiation, have taken their toll. Still, with Roscosmos under financial strain and facing limited options, recycling the modules could be seen as the only realistic path forward.
They do own there modules which are shared in a partnership that is coming to its end.
The US should also look to do the same for the Halo...
The thoughts of making use of Co as a fuel got me thing about the safe levels for inside the habitat space of the large 200 m diameter dome.
This ties into atmosphere detection for fire as well plus more.
In a Mars dome with a reduced atmospheric pressure of 0.5 bars (50 kPa or approximately 7.25 psi), the safe level of carbon monoxide (CO) for continuous human exposure is likely to be similar to, or potentially even lower than, the limits recommended for Earth environments, as the toxicity of CO is related to its partial pressure and its ability to bind with hemoglobin, which is a key part of oxygen transport.
While reduced total pressure can alter gas dynamics, the goal for a safe habitat is to maintain the internal environment within established safe limits developed from extensive medical and occupational studies.
Recommended Safe Levels
Standards from major health and occupational organizations for Earth-based, 1-atmosphere environments include:
OSHA Permissible Exposure Limit (PEL): 50 parts per million (ppm) averaged over an 8-hour workday.
NIOSH Recommended Exposure Limit (REL): 35 ppm averaged over a 10-hour workday, with a ceiling of 200 ppm for any 15-minute period.
EPA/WHO/ASHRAE (General Indoor Air Quality): The maximum indoor safe level is considered to be 9 ppm for an 8-hour average. This limit is more stringent and is intended for the general population and continuous exposure, making it more applicable to a long-term habitat.
NASA Standards: For long-duration spaceflight, NASA applies strict standards, with levels typically kept much lower than occupational limits to account for continuous exposure in a closed system. The average CO concentration in the ISS cabin is typically <2 mg/m³, which is well below terrestrial limits.
Considerations for a Reduced-Pressure Mars Dome
The human body's uptake of CO depends on its partial pressure in the inhaled air, which leads to the formation of carboxyhemoglobin (COHb) in the blood, reducing oxygen-carrying capacity. The lower total pressure of 0.5 bars does not change the fundamental toxicity of CO; the concentration in ppm (parts per million) remains the critical measurement for health standards.
Therefore, for the safety and long-term health of inhabitants in a Mars dome, the most appropriate and safe level would be the stringent public health recommendation of no more than 9 ppm over an 8-hour period, or as close to zero as possible.
Exposure to levels of:
50 ppm over 8 hours is the occupational limit for healthy workers, but not ideal for continuous living.
200 ppm or greater will cause physical symptoms such as headaches and dizziness after a few hours and is considered dangerous for prolonged exposure.
Continuous monitoring and effective filtration/atmosphere revitalization systems are crucial to keep CO concentrations extremely low in a closed Martian habita
Carbon Monoxide Levels and Exposure Limits Chart
This page also covers others that we will need to ensure with the Dome does not reach deadly or near critical levels.
We have started to give itemized things required to ensure safety.
So lets plan for "clark's calamity", when bad luck is all you have
Methane backup not nuclear vs solar
Planning of cargo as noted must be planned for as Constructing a human mission, a tonne at a time
Fire on the ISS, lunar base or Mars habitat or domes
There are many products and reuses that are all part of the planning for man to use the large Dome.
Just a note of the topics for Earth on this Mars Sol day.
Merry Christmas and Happy Holidays to all of the posters and lurkers!
Holidays
Real holiday flashing lights...
Merry Christmas to all of you not just the NewMars forum members.
It is funny how many topics we have for special days of the earth year.
what could be issues within a Dome on Mars.
just a back up from insitu resources
leveraging cargo to mars surface
bump for dome construction issue to include.
Sprinkler heads with a finer mist capability seems to me a do able.
Plus if these are controllable they can be used to produce rain for the internal Dome plants that are there for earth like feel.
NASA's new leader makes his priorities clear on day one
NASA’s new leader, billionaire entrepreneur Jared Isaacman, is making his priorities for the space agency clear in his first days on the job.
Isaacman was sworn in Thursday as the 15th administrator of NASA. The same day, President Donald Trump signed an executive order directing NASA to return astronauts to the moon by 2028, begin the development of a permanent outpost on the lunar surface by 2030, and lay the foundations for future exploration of Mars.
The order will likely provide a roadmap for Isaacman and NASA.
“Within the next three years, we are going to land American astronauts again on the moon, but this time with the infrastructure to stay,” Isaacman told NBC News in an interview after his swearing in on Thursday.
He has stepped into the role at a key time for NASA: The Trump administration has made it an urgent objective to return astronauts to the moon before China’s astronauts reach the lunar surface.
“We are faced with another space race,” Isaacman said.
The next phase of NASA’s return-to-the-moon program, known as Artemis, could launch as early as February. The mission, Artemis II, will send four astronauts on a roughly 10-day flight around the moon to test the agency’s Space Launch System rocket and Orion spacecraft.
The Artemis III flight that will follow is expected to land astronauts near the moon’s south pole.
Under Isaacman, NASA is expected to continue its push toward more commercialization. Companies like SpaceX and Blue Origin are set to play a critical role in the space agency's efforts to return to the moon, and Isaacman said other private space firms will support the agency’s lunar ambitions, as well.
Trump's executive order on space policy calls for developing a “vibrant commercial space economy through the power of American free enterprise,” and outlines a plan to wind down the International Space Station by 2030 and launch commercial space stations in its place.
The order also focuses on nuclear power in space. Building on a directive from Transportation Secretary Sean Duffy, who served as acting administrator of NASA before Isaacman was confirmed, it sets a goal to develop a nuclear reactor that is ready to launch to the moon by 2030.
Isaacman said nuclear power in space will be key to exploration beyond the moon, including future missions to Mars.
One of the challenges he faces as administrator, however, will be executing the White House’s vision with a limited budget.
Current funding across the U.S. government extends through Jan. 30. After that, NASA faces the possibility of significant budget cuts, particularly to its science operations.
Despite that looming obstacle, Isaacman expressed optimism about the agency’s ability to juggle the administration’s priorities.
“Whether it’s $25 billion or $20 billion, that’s an awful lot of money coming into the agency every single year,” he said. “We’ve got the best and brightest that are capable of taking on numerous challenging endeavors — the near impossible — simultaneously.”
“In the president’s space policy, it’s the opportunity to go back to the moon, establish the infrastructure there, and then make investments in the future technology like nuclear to set up for Mars missions,” Isaacman said. “I think with the resources that are provided, the commitment from the president here in the White House with that space policy, we’re going to be able to get the job done.”
Executive Orders
December 18, 2025
ENSURING AMERICAN SPACE SUPERIORITY
I think this is where this should go.
Acoustic signals have been important markers during NASA's Mars missions. Measurements of sound can provide information both about Mars itself—such as turbulence in its atmosphere, changes in its temperature, and its surface conditions—and about the movement of the Mars rovers.
Using these sound measurements to the best extent possible requires an accurate understanding of how sound propagates on Mars. Charlie Zheng, a professor of mechanical and aerospace engineering at Utah State University, and his doctoral student Hayden Baird, presented their work simulating sound propagation on Mars at the Sixth Joint Meeting of the Acoustical Society of America and Acoustical Society of Japan, running Dec. 1–5 in Honolulu, Hawaii.
"We expect that the study will provide deeper insight into weather and terrain effects on acoustic propagation in environments that are not easily measured," said Zheng. "The Martian environment is obviously one of them."
Baird and Zheng's work uses NASA's measurements of the atmospheric conditions and terrain on Mars, most of which have been previously modeled at meter-scale resolutions. They also had access to decades of data about the red planet's atmospheric composition and properties, as well as seismic studies that measure the ground porosity—all factors that play into how sound propagates.
"The setup of the simulation model used in this study relies heavily on previous results from multiple scientific disciplines," said Baird.
Focusing on the Jezero crater, the 2021 landing and exploration site of NASA's Perseverance rover and its attached Ingenuity helicopter, the researchers simulated how sound moves through and scatters off the region's complex terrains, whether it comes from a moving or stationary source. This will help them understand how other atmospheres compare to our own.
The researchers hope their model will help identify signals and patterns that indicate specific Martian atmospheric events. In the longer term, it may even help with sensor designs for future missions to other planets or moons to study atmospheric conditions.
"This study is a beginning to dive into many potential areas of planetary research," said Zheng.
Provided by Acoustical Society of America
This story was originally published on Phys.org.
Part of why we should and could re-use the cargo ships for raw materials to build with first and then later with natural sources.
The Starship spacecraft is built from large cylindrical rings of this steel, with each ring weighing around 1600 kg (3,600 lbs) and 21 rings used per ship. SpaceX's Starship has a consistent diameter of 9 meters (30 feet) for both the Starship upper stage and a height of 121.3 m (398 ft). These cylinders have a height of 1.83 m (6 ft), and a thickness of 3.97 mm (0.156 in). Super Heavy booster is 71 m (233 ft) tall, 9 m (30 ft) wide.
Total rocket Height
Block 1: 121.3 m (398 ft)
Block 2: 123.1 m (404 ft)
Block 3: 124.4 m (408 ft)
Block 4: 142 m (466 ft)
So some math and we have how much can be repurposed.
Its not the first time I have heard of Duckweed but much like algae that can be eaten people have gotten those early days of life out of the normal menu of choices.
The what appears to Th is that they are difficult on earth and make no profits for the other fuels of choice.