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repurposing starship has a note of issues
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Table 1: Individual Functional Spaces and Volumes
FUNCTION VOLUME - 4 CREW (m3) VOLUME - 6 CREW (m3)
Exercise
Aerobic Exercise 3.38 6.76
Aerobic Exercise 4.91 9.82
Resistive Exercise 3.92 7.84
Bone Loading 4.91 9.82
Sensorimotor Conditioning 4.91 9.82
Group Socialization & Recreation
Athletic Games 18.2 27.3
Personal Recreation 1.2 1.2
Tabletop games & artistic/creative recreation 10.09 15.14
Video/movie viewing 4.8 7.2
Window viewing 4.62 4.62
Human Waste Collection
Hand cleaning 2.69 5.38
Liquid waste collection 2.36 4.72
Solid waste collection 2.36 4.72
Hygiene
Changing Volume 2.18 4.36
Facial cleaning 2.69 5.38
Finger/toenail clipping 2.34 4.68
Full body cleaning 4.34 8.68
Hair styling/grooming 2.34 4.68
Hand cleaning 2.69 5.38
Oral hygiene 2.34 4.68
Physical work surface access 4.35 8.7
Viewing appearance 1.8 3.6
Shaving 2.34 4.68
Skin care 2.34 4.68
Logistics
Physical work surface access 4.35 4.35
Small item containment 1.2 1.2
Temporary stowage 6 6
Maintenance & Repair
Computer display and control interface 1.7 3.4
Equipment Diagnostics 4.35 4.35
Physical work surface access 4.35 4.35
Soft goods fabrication 2.69 2.69
EVA Support
Suit Component Testing 4.82 4.82
Computer Display and Control Interface 1.7 1.7
Video Communication 1.7 1.7
Audio Communication 1.7 1.7
Meal Consumption Full Crew Dining 10.09 15.14
Meal Preparation
Food Item Sorting 3.3 3.3
Food Preparation 4.35 4.35
Utensil and food equipment hygiene 3.3 3.3
Medical Operations
Advanced Medical Care 5.8 5.8
Ambulatory care 1.7 1.7
Basic Medical Care 5.8 5.8
Computer data entry / manipulation 1.2 1.2
Dental care 5.8 5.8
Private telemedicine 1.2 1.2
Two person meetings 3.4 3.4
Mission Planning
Command and control interface 3.42 3.42
Physical work surface access 10.09 15.14
Team Meetings 4.8 7.2
Mission Training 18.2 27.3
Private Habitation
Changing clothes 8.72 13.08
Meditation 4.8 7.2
Non-sleep rest/relaxation in private quarters 4.8 7.2
Physical work surface access 17.4 26.1
Single person private work, entertainment, and comm. 4.8 7.2
Sleep accommodation 10.76 16.14
Stretching 13.96 20.94
Two person meetings 13.6 20.4
Viewing appearance in private quarters 7.2 10.8
Spacecraft Monitoring and Commanding
Command and Control 3.42 3.42
Teleoperation and Crew Communication 1.7 1.7
Waste Management
Trash Containment 2.55 2.55
Trash Packing for Disposal | 3.76 | 3.76
Nasa document text Table 17: Comparison of Minimum Habitable Volumes and Case Study Habitable Volumes
Functional Space | Minimum Volume (m3) | MTH Volume (m3)
Exercise-1 (Cycle Ergometer) | 3.38 | 3.50
Exercise-2 (Treadmill) | 6.12 | 6.20
Exercise-3 (Resistive Device) | 3.92 | 4.29
Group Social-1 (Open Area) / Mission Planning-3 (Training) | 18.20 | 21.21
Group Social-2 (Table) / Meal Consumption (Table) / Mission Planning-2 (Table) 10.09 10.48
Human Waste-1 (Waste Collection) 2.36 2.36
Human Waste-2 (Cleansing) / Hygiene-1 (Cleansing) 4.35 4.35
Logistics-2 (Temporary Stowage) 6.00 6.18
Maintenance-1 (Computer) / EVA-2 (EVA Computer/Data) 3.40 3.55
Maintenance-2 (Work Surface) / Logistics-1 (Work Surface) / EVA-1 (Suit Testing) 4.82 5.11
Meal Preparation-1 (Food Prep) 4.35 4.35
Meal Preparation-2 (Work Surface) 3.30 3.30
Medical-1 (Computer) 1.20 1.65
Medical-3 (Medical Care) 5.80 6.40
Mission Planning-2 (Computer/Command) / Spacecraft Monitoring 3.42 3.55
Private Habitation-1 (Work Surface) / Medical-2 (Ambulatory Care) 17.40 17.40
Private Habitation-2 (Sleep & Relaxation) / Hygiene-2 (Non-Cleansing) 13.96 14.00
Waste Management 3.76 4.43
Logistics-3 (Storage Access) - 2.14
Utilization-1 (Scientific Research) - 5.22
Passageway to Hygiene - 3.84
Passageway to Second Deck - 10.25
Passageway to Third Deck / Egress/Ingress for Airlock - 3.43
Total NHV 115.83 147.19
NHV per Crewmember | 28.96 | 36.80
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Requiring 10 starships of stainless steel to make the exoskeleton with a lot os tools to reform and repurpose it is a task that seems to make for failure.
37,050m of 30mm OD / 2mm wall thickness 304L tubing per Starship primary structure. 10 Starships provide 370,500m of tubing to work with.
It seems that just 1 m over our structure can not be supported by this tubing.
Based on structural requirements to support 2 meters of Martian regolith, 304L stainless steel would require significant thickness or structural reinforcement (such as corrugation or supporting arches) rather than a simple flat sheet.
Here is the breakdown based on structural analysis for Martian conditions: 1. Load Calculation (The Challenge) Regolith Depth: 2 meters (sufficient for radiation shielding).
Regolith Density: Approximately \(1000\text{--}1500\text{\ kg/m}^{3}\) (loose to packed).
Martian Gravity: \(0.38\text{\ g}\).Load per \(m^{2}\): 2 meters of regolith creates a vertical load of roughly \(7.6\text{--}11.4\text{\ kN/m}^{2}\) (approx. \(1500\text{\ kg}\times 2\text{\ m}\times 0.38\text{\ g}\approx 11.4\text{\ kPa}\)).
Internal Pressure: The habitat must also maintain internal air pressure (approx. \(10\text{--}100\text{\ kPa}\)), which often acts in favor of the structure by lifting the load, but requires the steel to act as a pressure vessel.
2. Thickness and Span for 304L Stainless Steel For a flat roof, 304L stainless steel would be prohibitive in thickness. Therefore, structural forms are required.
Thin Sheet (0.5 mm - 1 mm): Cannot span any meaningful distance; it would buckle under 2 meters of regolith.
Corrugated 304L Sheets (1.5 mm - 3 mm): If using a 2-3 inch deep corrugated profile, a thickness of \(1.5\text{\ mm}\) (\(16\text{\ gauge}\)) to \(3\text{\ mm}\) (\(1/8\text{\ inch}\)) might support the load over short spans of \(1\text{--}2\text{\ meters}\) between supports.
Structural Plate (\(6\text{\ mm}\) - \(12\text{\ mm}\)+): To span larger distances (e.g., \(3\text{--}5\text{\ meters}\)) without intermediate supports, \(304\text{L}\) plates of at least \(6\text{\ mm}\) to \(12\text{\ mm}\) (\(1/4\text{\ inch}\) to \(1/2\text{\ inch}\)) would likely be required to prevent sagging and failure under 2 meters of regolith.
Summary Recommendation To support 2 meters of regolith over a modest span of 3-4 meters, a \(6\text{\ mm}\) (\(1/4\text{\ inch}\)) thick 304L steel plate, properly stiffened or arched, is a reasonable starting engineering estimate. If using corrugated sheets, thicknesses as low as \(2\text{--}3\text{\ mm}\) could be used if closely supported
The other thing is the double toru constructed with 2 layers is insufficient for the 0.5 bar internal pressure. The stuff Nasa and Bigelow created is using 13 to 15 layers which means we are in need of 6 to 8 layers to get the same performance.
The internal of the inflatable needs for support structures that are not so far planned.
Estimated time to build a starship less engine is about 8 months plus so to think it will take any less to pull them apart and store until we need the pieces is also not in our favor.
Also landing them in a cluster means being 500 m to 1,000 meters from each other to limit debris damage push is the site has to much ice the units may not land stably possibly falling.
since we need 4 cargo ships to land and make fuel this could be a problem.
Starship Cargo Fuel Tank Dimensions (Metric)
Starship uses two main tanks inside its 9m‑diameter hull:
LOX tank (upper)
CH₄ tank (lower)
Both tanks share the same 9m outer diameter, with domed bulkheads separating them.
1. Outer Tank Diameter
9.0m external diameter (hull diameter)
Internal tank diameter is slightly less (~8.8m) due to wall thickness.
2. LOX Main Tank (Liquid Oxygen)
Approximate Dimensions
Diameter: ~8.8m internal
Height: ~20–22m (varies by configuration)
Volume: ~1,200–1,300m³ (estimated from total propellant volume split)
Notes
LOX tank occupies the upper half of Starship.
Uses a common dome to separate it from the CH₄ tank.
3. CH₄ Main Tank (Liquid Methane)
Approximate Dimensions
Diameter: ~8.8m internal
Height: ~12–14m
Volume: ~700–800m³
Notes
Located in the lower section of Starship.
Slightly smaller than the LOX tank because methane is less dense.
4. Header Tanks (Landing Tanks)
SpaceX has published header tank dimensions.
LOX Header Tank
Diameter: 3.14m
Internal Volume: 18.67m³
CH₄ Header Tank
Diameter: 3.14m
Internal Volume: 16.21m³
These are small spherical/ellipsoidal tanks used for landing burns.
5. Total Propellant Capacity (for context)
~1,200t LOX + ~240t CH₄ (varies by variant)
Total propellant volume ~1,900–2,000m³ (derived from density and mass)
Summary Table
Tank Diameter (m) Height (m) Volume (m³) Notes
Main LOX Tank ~8.8 ~20–22 ~1,200–1,300 Upper tank
Main CH₄ Tank ~8.8 ~12–14 ~700–800 Lower tank
LOX Header Tank 3.14 — 18.67 Published spec
CH₄ Header Tank 3.14 — 16.21 Published spec
crater image has been fixed
Also removed Quonset hut tent from the posting removing structural confusion
Posts created by the topic first post or any other notable members get churned under by our forums software as a part of database management in the MYSQL. The way to look for topics is now via our Daily Recap - Recapitulation of Posts in NewMars by Day, looking for bookmarks, or hash tags that you started, plus we have Posted | New | Active, memory of member profile check for any post that they have made. Keyword for our site can only do so much but then again we have google advance which looks at just the our website only.
All members are equal when it comes to making a post, the reason is for MOD's or Admins are to ensure we have no bad operators within them. Posing question in topic is what should be done so as to get all members that have knowledge to respond and to keep information within discussions and not privately scattered all over the place.
I am sorry that you took it personally as that was not the intent.
NASA delays Artemis mission to moon due to cold weather
Bracing for a weekend cold snap in Florida, NASA delayed a dress rehearsal fueling test for its Artemis II moon rocket, moving it from Saturday to Monday, and pushed the long-awaited launch back at least two days to no earlier than 11:20 p.m. EST on Feb. 8.
At the same time, NASA is gearing up to launch a fresh crew to the International Space Station to replace the four Crew 11 fliers who cut their mission short and returned to Earth on Jan. 15 due to a medical issue with an unidentified crew member.
Crew 12, launching atop a SpaceX Falcon 9 rocket, will be ready to blast off as early as Feb. 11. But if the Artemis II mission gets off on Feb. 8 as NASA hopes, Crew 12 commander Jessica Meir, pilot Jack Hathaway, European Space Agency astronaut Sophie Adenot and cosmonaut Andrey Fedaev will stand down until after the Artemis II crew returns to Earth. In that scenario, Crew 12 would launch around Feb. 19.
If Artemis II takes off on Feb. 10 or 11, the only other opportunities left in the February launch period, then Crew 12 could take off 11 days later. If Artemis II runs into major problems and slips to the next launch period in March, Crew 12 could launch as early as Feb. 13, depending on when the moon mission is called off.
But there are no scenarios where Artemis II and Crew 12 would be in space at the same time unless there's an emergency aboard the space station that requires a quick launch for Meir and her crewmates. Otherwise, the moon mission has priority.
The long-awaited Artemis II mission will use NASA's huge Space Launch System rocket to boost three NASA astronauts and a Canadian crewmate on a trip around the moon and back, the first such flight since the final Apollo mission 54 years ago. The upcoming mission will set the stage for another crew to attempt a landing near the moon's south pole in 2028.
Artemis II commander Reid Wiseman, Victor Glover, Christina Koch and Canadian astronaut Jeremy Hansen had planned to blast off next Friday, assuming a leak-free fueling test Saturday.
But with the test delay and the time needed for NASA to analyze the results, the agency opted to give up launch opportunities on Feb. 6 and 7. That leaves just three opportunities in the February launch period: Feb. 8, 10 and 11. If the rocket is not off the ground by Feb. 11, the flight will slip to early March.
The "wet dress" rehearsal countdown now will start at 8 p.m. EST Saturday. Fueling will begin around 11 a.m. Monday, leading to the opening of a simulated launch window at 9 p.m. that night.
Engineers plan to load the Space Launch System rocket with more than 750,000 gallons of supercold hydrogen and liquid oxygen to work through loading procedures and to make sure the rocket's tanks, valves, propellant plumbing and umbilicals attached to the side of the booster are leak-free and good to go.
Launch Director Charlie Blackwell-Thompson and her team plan to work through a variety of recycle options to rehearse procedures for dealing with unexpected problems.
The Artemis II SLS will be making the program's second flight. Before its unpiloted maiden flight in 2022, multiple fueling tests were required to address a variety of propellant leaks and other issues. The Artemis II rocket features upgrades and improvements to eliminate those issues.
"Artemis I was the test flight, and we learned a lot during that campaign, getting to launch," said Blackwell-Thompson. "And the things that we learned relative to how to go load this vehicle, how to load LOX (liquid oxygen), how to load hydrogen, have all been rolled into the way in which we intend to load the Artemis II vehicle.
Lunar Starship was never meant to come home to Earth, SpaceX admits
SpaceX’s lunar Starship was never designed to blaze back through Earth’s atmosphere in a shower of plasma. Instead, the company has quietly positioned its Human Landing System as a one‑way ferry that lives and dies in cislunar space, while NASA’s Orion capsule handles the brutal trip home. That architectural choice, long embedded in Artemis planning documents, is only now breaking through to a wider public that assumed every Starship would eventually come back to Earth.
Framed correctly, this is less a retreat from reusability than a bet on specialization. By stripping out the heavy heat shield and recovery hardware, SpaceX can turn its lunar variant into a tall, fuel‑hungry elevator between orbit and the Moon, while the rest of the Artemis stack focuses on launch and reentry. The tradeoffs behind that decision reveal how NASA and SpaceX are trying to thread the needle between ambition, schedule pressure, and basic physics.
Artemis needs a lunar shuttle, not a return capsule
NASA’s Artemis architecture was built around the idea that no single vehicle would do everything, and that includes the trip home. The agency’s own outline for Artemis III makes clear that astronauts will launch on the Space Launch System, ride in Orion to lunar orbit, then transfer into a separate lander for the descent and ascent. The Artemis program description spells out that SLS and Orion are the pieces designed for deep‑space transit and Earth reentry, while the lander is a dedicated vehicle for the last leg between orbit and the Moon’s surface.That division of labor is why NASA refers to SpaceX’s vehicle as the Starship Human Landing System, or HLS, rather than simply Starship. Agency material on the Initial Human Landing concepts shows a tall, stripped‑down lander on the Moon, with Orion waiting in lunar orbit as the ride home. In other words, the mission design assumes from the start that the lunar Starship is a shuttle between the Moon and orbit, not a capsule that ever sees Earth’s atmosphere.
Inside the one‑way Starship design
SpaceX’s own technical descriptions underline that the lunar lander is a specialized branch of the broader Starship family. A detailed overview of Starship‑HLS notes that the Human Landing System is derived from Starship but modified for operation as a lunar lander, and explicitly states that this configuration is not designed to return to Earth. That is not a late‑breaking compromise, it is a core assumption baked into the hardware, from the missing heat shield to the absence of aerodynamic control surfaces needed for atmospheric entry.The logic behind that choice has even filtered into public discussion among enthusiasts and engineers. In one widely shared explanation, Forrest and Townsend tell fellow fans that engineers “dont’ plan on ont he lunar starship to return to earth, no heatshield, save on the cerami,” while David Cluett promises to explain the trade in layman’s terms. The point is simple: every kilogram not spent on ceramic tiles and reentry systems can be spent on propellant, cargo, or life support for the lunar mission itself.
Why Orion still matters in a Starship era
The decision to keep the lunar Starship in space also explains why Orion remains central to NASA’s plans, despite Starship’s headline‑grabbing capabilities. A technical discussion of whether the lander could replace Orion, framed as Can Starship Lunar return to Earth orbit so Orion is not needed anymore, points back to the reality that Orion on SLS is planned to handle the high‑energy return and splashdown. The Orion capsule is built around a robust heat shield and abort systems that the lunar Starship variant simply does not carry.Programmatically, that means Artemis is locked into a choreography where SLS, Orion, and the lander are all indispensable. The SLS missions listed for Artemis I, Artemis II, and beyond show a steady cadence of Orion flights, while separate documentation describes how the Starship Human Landing will be instrumental in ferrying crews from lunar orbit to the surface and back. That is why, even in a Starship era, Orion’s role as the Earth‑return vehicle is not a redundancy but a structural pillar of the mission design.
A “simplified” mission profile, still complex in practice
As schedule pressure mounts, SpaceX has been working with NASA on what it calls a simplified mission architecture for the lunar lander, but that streamlining does not include bringing the vehicle home. Company representatives have described to NASA a Starship for NASA approach that reduces the number of on‑orbit refueling events and mission steps while still delivering astronauts to the lunar surface. A separate account of that simplified approach notes that the company is defending the viability of its lander even as it trims complexity to hit key milestones.Critics inside the space community have questioned whether those changes are enough. At a high‑profile event, former NASA leaders Charlie Bolden and Jim Bridenstine expressed skepticism that the current Starship schedule could deliver on time, even with a leaner mission design. Yet SpaceX has publicly stood behind its timeline, with one detailed feature on its lunar plans, titled around Fly Me to the Moon, stressing that, unlike Apollo, Unlike Apollo, Artemis III will rely on a multi‑vehicle choreography that includes several crucial milestones in 2025.
Refueling, timelines, and the politics of delay
Behind the scenes, the biggest technical swing remains in‑space refueling, which is essential if a non‑returning lander is going to haul enough propellant to and from the Moon. SpaceX’s official updates describe how the next major flight milestones tied specifically to HLS will be a long‑duration flight test and an in‑space propellant transfer in Earth orbit. Without those capabilities, the one‑way lunar Starship would struggle to carry the fuel it needs for multiple sorties between lunar orbit and the surface.That technical risk feeds directly into political anxiety. In one public exchange, Rob Jacobs But the points out that the many Falcon 9 flights are irrelevant to NASA’s immediate problem, because what the agency needs is HLS, which is a special version of Starship. That concern has grown loud enough that NASA has signaled it may consider new proposals from other top space companies to get America back to the Moon if delays mount, a reminder that the lunar Starship’s one‑way design does not insulate it from competition.
A Chicago-sized bulge has appeared near Yellowstone’s volcano — and scientists say it’s growing
Yellowstone National Park is a must-visit site for its geothermal features. From hot springs to geysers, the place is embellished with serene views at every corner. Beneath the park's landscape lies a volcano that hasn't erupted in more than 600,000 years. But recently, experts observed a one-inch-high bulge from underneath, prompting speculations of an eruption. The slight rise in ground along Yellowstone's north rim is as wide as the city of Chicago.
Mike Poland, scientist-in-charge of the Yellowstone Volcano Observatory, spoke to Cowboy State Daily about what he and his fellow scientists observed at the site. “It’s an area over 19 miles across, give or take a few miles,” he said, adding, “Saying the uplift is the size of Chicago makes it sound incredibly grandiose, but I think it’s pretty stunning even if it’s not particularly unusual."
Does the wide bulge indicate that an eruption is on the horizon? Experts have slashed the speculations without any fluff. “That doesn't mean that the volcano is about to erupt. It’s Yellowstone being Yellowstone," Poland said. The reply makes perfect sense, given that the ground uplift has happened a few times before. Under the outlet's Facebook post, people reacted similarly to the news, not making too much of a big deal out of the development. "Is it time for the annual Yellowstone is gonna erupt stories again?" one person wrote. "A whole inch, huh? Wowsers," another wrote, sarcastically. "Not a bad thing. Upheavals in Yellowstone happen all the time," a third added. The slight movement of the surface above the dormant volcano of Yellowstone, a deformation known as the Norris Uplift Anomaly, occurred once between 1996 and 2000 near Norris Geyser Basin. The instance repeated in 2004 and then again in 2020.
Thanks to modern technology, scientists can get real-time data on the movements of the ground along Yellowstone's north rim and other areas of the park. The data has enabled experts to curate a map showing the uplift or "bulge" in the middle of Yellowstone. “It's a measure of how advanced our monitoring networks have gotten, and their sensitivity in detecting these small changes. That’s the story of the year for me,” Poland noted. The expert compared the bulge to a balloon blowing up in the subterranean and is quite insignificant in size to be observed with the naked eye. However, advanced technology has allowed scientists to observe these slight upheavals quite accurately. Poland revealed that the experts have been observing movements through radar maps and satellites.
“We've got 17 GPS stations in Yellowstone, and many more in the surrounding area, and they could pinpoint exactly when this uplift started," he revealed. But if Yellowstone's volcano shows no sign of eruption, then what does the bulge indicate? Experts believe that the activities within the magma chamber of the volcano are the most probable explanation behind the sudden yet subtle ground uplift. “The most likely explanation is that it's the accumulation and withdrawal of magma at a depth of nine miles,” Poland explained. The movement is nothing to be worried about and will certainly not result in an eruption. Scientists believe that the bulge would be much larger if the magmatic system were preparing to erupt anytime soon.
Are we on for discussion of what we know?
Things to talk about is Korolev location landing cycles and what they are to do.
Initial is Insitu propellant plant which is cargo ships in quantities maybe due to what is shipped for mass is 2 all the way to 6 ships the cycle before men can go.
First crew out is exploratory probably 20 crew split between 2 crewed starships and setting up shop for future construction utilizing all spare cargo mass to cut the quantity for the future asset required with compliment of 4 cargo..
second mission is more science with a larger crew of possibly 50 or more across a pair of crewed starship with compliment of 4 cargo.
Another view of the Korolev

Another view of the Korolev

The Korolev Crater on Mars, located in the northern lowlands at 73°N latitude and 165°E longitude, features a remarkably smooth, flat, and dome-shaped surface in its central region. This topographically uniform area is a 1.8-kilometer-thick, 60-kilometer-wide mound of permanent water ice.
Topographic Features and Data:
Smooth Center: The central, ice-filled floor of the 82-km-wide crater acts as a natural "cold trap," creating a flat, bright, and smooth surface.
Elevation: The crater floor lies approximately 2 kilometers below its rim.
Topographic Profile: Color-coded topographic views (such as those from the High Resolution Stereo Camera on Mars Express) show the central ice mound as a relatively high-altitude, flat deposit, whereas the surrounding area is characterized by the rugged, steep crater walls.
Composition: The flat surface is not snow, but a massive deposit of water ice, with a volume of approximately 2,200 cubic kilometers, that remains stable year-round.
The smooth, ice-filled depression is surrounded by the dune fields of Olympia Undae, further distinguishing the flatness of the crater floor from the surrounding terrain
AI seems to not understand being not landing inside the crater on the ice.
Trying to land outside of the crater but on flat smooth surface:
Landing outside the immediate topographical map area of the Korolev Crater on Mars (located at 73°N, 165°E in the northern lowlands) allows for access to smooth, flat terrain within the broader Planum Boreum or the nearby Olympia Undae region. These areas are characterized by extensive, low-lying northern plains.
Recommended Smooth/Flat Areas Outside Korolev Crater
Planum Boreum (Northern Polar Plain): The Korolev Crater is located on this vast, relatively flat expanse. The plains surrounding the 2-kilometer-high crater rim offer extensive flat, solid ground suited for landing.
Olympia Undae: Located just north/northeast of Korolev, this dune field wraps around part of the north polar cap. While it is a dune field, the boundary regions between the plains and the dunes offer relatively smooth, accessible terrain.
Northern Lowlands (General): The region surrounding Korolev is part of the northern lowlands, which are characterized as being much smoother and lower in elevation than the southern hemisphere. These areas are often favored for landing due to having fewer obstacles and lower topographical variation.
Key Topographical Features in the Area
Rim Elevation: The rim of Korolev Crater stands approximately 2 kilometers above the surrounding Plains.
Surface Composition: The terrain immediately surrounding the crater is typical of the northern high-latitude plains, often covered in seasonal frost and dust.
Accessibility: The region is considered a "cold trap" and is a primary target for finding water-ice and studying polar climate history.
The surrounding northern plain, specifically the area within the Mare Boreum quadrangle (specifically away from the crater rim), provides a flat, stable surface

Mars settlement projects typically progress through phases from initial robotic exploration and small outposts (Pre-settlement) to permanent, growing settlements with developing infrastructure (In-settlement), culminating in self-sufficient, potentially terraformed societies (Post-settlement), focusing first on establishing basic life support, resource utilization (ISRU), energy, and habitats before expanding to a city-like presence with economic independence. Key stages involve robotic reconnaissance, crewed landings, building propellant plants, establishing habitats, developing local agriculture, mining, and transitioning to self-sufficiency, requiring advances in transportation, closed-loop life support, and energy systems.
Key Phases & Stages
1. Pre-Settlement (Robotic & Early Outpost):
• Robotic Reconnaissance: Detailed surveys, sample collection (e.g., Perseverance), testing technologies for fuel/oxygen production from the atmosphere.
• Cargo Pre-Deployment: Sending autonomous cargo, including fuel production equipment, before human arrival.
• First Crewed Missions: Establishing a rudimentary base, completing the propellant plant for return fuel, and testing life support.
2. In-Settlement (Permanent & Growing Colony):
• Infrastructure Development: Building habitats, mining water, growing crops, creating power systems (solar/nuclear).
• Resource Utilization (ISRU): Extracting and processing Martian resources (water, metals, minerals) for construction and fuel.
• Population Growth: Increasing crew sizes, developing a local economy, and establishing governance.
3. Post-Settlement (Self-Sufficiency & Beyond):
• Industrial Independence: Scaling up mining, manufacturing (3D printing, metals, plastics) to reduce Earth reliance.
• Societal Development: Growing into towns/cities, developing unique Martian culture, governance, and potentially independent political structures.
• Terraforming (Long-Term): Modifying the environment to create breathable air and habitable zones, a highly speculative long-term goal.
Key Technologies & Goals
• Transportation: Reliable, efficient Earth-Mars transport (e.g., SpaceX Starship).
• Life Support: Perfecting closed-loop systems for air, water, and food.
• Energy: Sustainable power generation (solar, nuclear).
• ISRU: Water extraction, atmospheric processing for fuel/oxygen, material processing.
• Habitats: Durable, radiation-shielded shelters (surface and underground)Mars settlement projects, like SpaceX's vision, progress through phases: pre-settlement (outposts), in-settlement (permanent bases), and post-settlement (self-sufficient society), aiming for crewed landings in the late 2020s/early 2030s and self-sufficiency by mid-century, requiring massive initial cargo (Starships carrying 100+ tons) for habitats, life support, and resource utilization (ISRU) like water and fuel production from Martian air and ice, with the ultimate goal of a large, self-sustaining population.
Phases of Development (Conceptual)
1. Pre-Settlement (Exploration & Outpost)
• Focus: Robotic missions, establishing basic infrastructure, resource identification (water ice, minerals).
• Key Tech: Advanced rovers, ISRU (In-Situ Resource Utilization) for oxygen/methane (fuel/air).
• Timeline: Current robotic exploration, early cargo missions (late 2020s).
2. In-Settlement (Permanent Base)
• Focus: First human landings, establishing initial habitats, expanding resource production (ISRU, agriculture), reducing Earth dependency.
• Key Tech: Habitable modules, power systems, water processing, basic manufacturing.
• Timeline: First crewed landings (early 2030s), developing permanent presence.
3. Post-Settlement (Self-Sufficient Society)
• Focus: Large-scale population, full industrialization, economic self-sufficiency, cultural development.
• Key Tech: Advanced manufacturing, large-scale life support, robust local economy, potential for terraforming elements.
• Timeline: Decades-long process, aiming for self-sufficiency by 2050+.
Timeline & Mass Estimates (SpaceX Example)
• Early Missions (2020s-2030s): Cargo & Crew via Starship (100+ tons capacity).
• Cargo: Essential for habitats, initial supplies, ISRU equipment.
• Crew: Small groups (4-10+), increasing over time.
• Self-Sufficiency: Goal by 2050, requiring a million people using numerous Starships over many launch windows (every ~26 months).
Mass Requirements & Challenges
• High Mass: Water, air (oxygen/nitrogen), fuel, food, equipment, habitats.
• ISRU Critical: Extracting water ice and using atmospheric CO2 for oxygen and methane fuel (CH4) is essential to reduce launch mass from Earth.
• Example: Water is heavy; a Starship (100 tons payload) could carry enough water for 20 people for years, but continuous resupply is needed.
In essence, Mars settlement requires a phased approach, leveraging current tech like Starship for massive cargo delivery, transitioning from outposts to permanent bases, and finally, fostering self-sufficiency through local resource utilization to support a growing populationEstablishing a Mars propellant plant to refuel a Starship for a return trip likely requires several cargo missions, with estimates suggesting 2 to 6+ ships to deliver necessary infrastructure (solar panels, mining equipment) and initial fuel stocks. While some scenarios suggest 3-4 ships can enable a return via in-situ resource utilization (ISRU), initial, safer approaches might use 6+ tankers to establish necessary infrastructure.
Seems that we are not going to our landing site of Korolev Crater
SpaceX is planning to land multiple uncrewed Cargo Starships on Mars as early as 2030, with a focus on locations in the northern lowlands, such as Arcadia Planitia, which are rich in subsurface water ice. While the Korolev Crater is a notable, 82-kilometer-wide, ice-filled feature, it is located at 73° North latitude, which is generally outside the prime, lower-latitude, or mid-latitude zones (closer to the equator for solar power) favored for initial,, easier landings.
Key Aspects of Multiple Cargo Starship Landings on Mars:
Landing Locations: SpaceX has downselected candidate sites, primarily focusing on Arcadia Planitia, Deuteronilus Mensae, and Phlegra Montes. These areas offer flat, low-elevation, and less rocky terrain, reducing the need for extensive obstacle avoidance.Challenges and Strategy: Landing requires high precision due to the thin atmosphere, necessitating a "belly-flop" maneuver followed by a vertical landing using legs. The ships are designed to land at least 6–9 engines to generate sufficient braking force.
Landing Procedures: Multiple Starships are expected to land in close proximity (within a few kilometers of each other) to build up an initial outpost.
Infrastructure Setup: The initial cargo missions will land equipment, including tools to extract water from ice for propellant production (using the Sabatier process) and for creating breathable oxygen.
Why Not Directly in the Center of Korolev Crater?
Latitude and Solar Power: Korolev Crater is at a high northern latitude (73°N), whereas early missions require closer to the equator (under 40° latitude) for consistent solar power and better thermal management.Terrain: The center of the crater is a 1.8-kilometer-deep, 60-kilometer-wide mound of solid water ice. While this is ideal for resources, it is a massive glacier, not a "level surface" in the sense of a stable, rocky landing pad, making it unsuitable for heavy, vertical-landing rockets.
Therefore, multiple Starships would likely land on the level plains of Arcadia Planitia or adjacent to large, accessible ice deposits rather than inside the Korolev Crater itself, even though that crater is a significant source of iceInfrastructure Requirements: A fully operational plant capable of producing 1,000+ tons of propellant (methane and oxygen) for a return journey requires substantial power, estimated at 5 GWh, needing ~250 metric tons of equipment, equivalent to 2+ fully loaded cargo Starships.
Fuel Mining & Production: The process involves extracting water ice and capturing \(CO_{2}\) from the atmosphere.
Alternative/Interim Methods: Rather than immediate, full ISRU, early missions might rely on landing 3-4 Starships, where 3 are drained to fuel 1 for the return trip, or using 4-6 ships to establish a rudimentary plant.
Scale: SpaceX aims to send at least 2 uncrewed cargo ships before the first crewed mission to set up power, mining, and life support. Ultimately, the number of ships depends on the efficiency of the ISRU plant, the power capacity installed, and the willingness to risk the first crew's return capability
Water source from Korolev Crater
Based on current SpaceX Mars mission architecture, establishing a propellant plant on Mars to refuel a Starship for a return journey, utilizing water ice, requires a multi-stage, cargo-heavy operation. Initial Setup Phase: To establish the necessary propellant plant (Sabatier reactors, mining equipment, solar arrays) at a location like Korolev Crater, early, uncrewed missions would need to land several cargo Starships (potentially 2–5) containing roughly 100+ tons of equipment each.Propellant Production Requirement: To refuel a single Starship for a return journey, the plant must produce approximately 1,200 metric tons of propellant (methane and oxygen).Operational
Requirement: While early estimates suggested 1–2 cargo ships worth of equipment could start production, a more robust and faster turnaround (within one synod, or 26 months) likely requires at least 3-4 cargo ships to be active to ensure enough power and water processing capability to produce the ~1,200+ tons of fuel. In summary, to start a plant, 2-5 dedicated cargo Starships are required to land the equipment, with at least 3-4 of them acting as operational plant components/fuel depots to reliably produce enough fuel for one return trip.
Key considerations: Water Source: Korolev Crater is an ideal, high-latitude location (\(73^{\circ }\text{N}\)) with large, accessible, near-surface water ice deposits, reducing the need for deep drilling.
Power: The limiting factor will be the mass of solar panels or nuclear reactors required to power the electrolysis process to turn that water into hydrogen, requiring significant cargo mass for power generation.
Launch Windows: These cargo ships must arrive at least one, if not two, synodic periods (26–52 months) before the crew arrives, to ensure the tanks are full
Landing multiple SpaceX Starships on the level surface of the Korolev Crater on Mars to avoid damaging its 1.8 km thick, 60 km wide water ice mound is feasible but requires careful landing site selection and operational procedures. The Korolev Crater is an ideal destination for future missions because its deep basin acts as a natural "cold trap," creating a permanent, stable, and protected reservoir of ice, with air above it being significantly colder and heavier than the surrounding atmosphere.
Strategies for Non-Destructive Landing
To avoid melting or destroying the ice, landings must be carefully managed to minimize heat and debris:
Distance from Ice Mound: Landings should occur on the outer edges of the crater floor or on the flat plains outside the crater rim, rather than directly on the central ice mound, to prevent heat-induced sublimation or contamination.
Controlled Descent & Landing: Starship uses controlled, vertical landings powered by its Raptor engines, allowing it to precisely target non-ice zones.
Landing Pad Development: Initial cargo missions would likely need to prepare a, stable, and possibly paved, or reinforced landing surface on the Martian regolith to prevent the engines from creating a large, dangerous, and erosive crater beneath them.
Engine Exhaust Management: While the Raptor engines operate for a short time, they still produce high heat and pressure, so landing on prepared, rocky, or flat, non-ice areas is crucial to prevent the ice from "melting" or being covered in soot.
Environmental Considerations
The "Cold Trap" Stability: The ice in the Korolev Crater is protected because the cold air above it acts as a shield from surrounding warm air, meaning a small amount of disturbance will not immediately cause the entire ice mound to melt.
Impact of Multiple Landings: Multiple landings would require extensive site surveys and careful planning to ensure the cumulative, long-term impact on the local environment is kept to a minimum.
Potential Contamination: The use of methane/oxygen fuel is relatively clean, producing less soot than other rockets, but still produces CO₂ and water vapor, which could potentially contaminate the pristine, untouched ice.
By landing on the periphery of the crater's interior or on the surrounding plains, multiple cargo Starships can safely deliver supplies to the edge of this vast water resource without destroying the unique geological feature
The Korolev Crater on Mars, located in the northern lowlands at 73°N latitude and 165°E longitude, features a remarkably smooth, flat, and dome-shaped surface in its central region. This topographically uniform area is a 1.8-kilometer-thick, 60-kilometer-wide mound of permanent water ice.
Topographic Features and Data:
Smooth Center: The central, ice-filled floor of the 82-km-wide crater acts as a natural "cold trap," creating a flat, bright, and smooth surface.
Elevation: The crater floor lies approximately 2 kilometers below its rim.
Topographic Profile: Color-coded topographic views (such as those from the High Resolution Stereo Camera on Mars Express) show the central ice mound as a relatively high-altitude, flat deposit, whereas the surrounding area is characterized by the rugged, steep crater walls.
Composition: The flat surface is not snow, but a massive deposit of water ice, with a volume of approximately 2,200 cubic kilometers, that remains stable year-round.
The smooth, ice-filled depression is surrounded by the dune fields of Olympia Undae, further distinguishing the flatness of the crater floor from the surrounding terrain
AI seems to not understand being not landing inside the crater on the ice.
Trying to land outside of the crater but on flat smooth surface:
Landing outside the immediate topographical map area of the Korolev Crater on Mars (located at 73°N, 165°E in the northern lowlands) allows for access to smooth, flat terrain within the broader Planum Boreum or the nearby Olympia Undae region. These areas are characterized by extensive, low-lying northern plains.
Recommended Smooth/Flat Areas Outside Korolev Crater
Planum Boreum (Northern Polar Plain): The Korolev Crater is located on this vast, relatively flat expanse. The plains surrounding the 2-kilometer-high crater rim offer extensive flat, solid ground suited for landing.
Olympia Undae: Located just north/northeast of Korolev, this dune field wraps around part of the north polar cap. While it is a dune field, the boundary regions between the plains and the dunes offer relatively smooth, accessible terrain.
Northern Lowlands (General): The region surrounding Korolev is part of the northern lowlands, which are characterized as being much smoother and lower in elevation than the southern hemisphere. These areas are often favored for landing due to having fewer obstacles and lower topographical variation.
Key Topographical Features in the Area
Rim Elevation: The rim of Korolev Crater stands approximately 2 kilometers above the surrounding Plains.
Surface Composition: The terrain immediately surrounding the crater is typical of the northern high-latitude plains, often covered in seasonal frost and dust.
Accessibility: The region is considered a "cold trap" and is a primary target for finding water-ice and studying polar climate history.
The surrounding northern plain, specifically the area within the Mare Boreum quadrangle (specifically away from the crater rim), provides a flat, stable surface

Mission build up is an issue to see how we can change the numbers to be able to get to the real life colony that we want on Mars.
Establishing a Mars propellant plant to refuel a Starship for a return trip likely requires several cargo missions, with estimates suggesting 2 to 6+ ships to deliver necessary infrastructure (solar panels, mining equipment) and initial fuel stocks. While some scenarios suggest 3-4 ships can enable a return via in-situ resource utilization (ISRU), initial, safer approaches might use 6+ tankers to establish necessary infrastructure.
Infrastructure Requirements: A fully operational plant capable of producing 1,000+ tons of propellant (methane and oxygen) for a return journey requires substantial power, estimated at 5 GWh, needing ~250 metric tons of equipment, equivalent to 2+ fully loaded cargo Starships.
Fuel Mining & Production: The process involves extracting water ice and capturing \(CO_{2}\) from the atmosphere.
Alternative/Interim Methods: Rather than immediate, full ISRU, early missions might rely on landing 3-4 Starships, where 3 are drained to fuel 1 for the return trip, or using 4-6 ships to establish a rudimentary plant.
Scale: SpaceX aims to send at least 2 uncrewed cargo ships before the first crewed mission to set up power, mining, and life support. Ultimately, the number of ships depends on the efficiency of the ISRU plant, the power capacity installed, and the willingness to risk the first crew's return capability
Water source from Korolev Crater
Based on current SpaceX Mars mission architecture, establishing a propellant plant on Mars to refuel a Starship for a return journey, utilizing water ice, requires a multi-stage, cargo-heavy operation. Initial Setup Phase: To establish the necessary propellant plant (Sabatier reactors, mining equipment, solar arrays) at a location like Korolev Crater, early, uncrewed missions would need to land several cargo Starships (potentially 2–5) containing roughly 100+ tons of equipment each.Propellant Production Requirement: To refuel a single Starship for a return journey, the plant must produce approximately 1,200 metric tons of propellant (methane and oxygen).Operational
Requirement: While early estimates suggested 1–2 cargo ships worth of equipment could start production, a more robust and faster turnaround (within one synod, or 26 months) likely requires at least 3-4 cargo ships to be active to ensure enough power and water processing capability to produce the ~1,200+ tons of fuel. In summary, to start a plant, 2-5 dedicated cargo Starships are required to land the equipment, with at least 3-4 of them acting as operational plant components/fuel depots to reliably produce enough fuel for one return trip.
Key considerations: Water Source: Korolev Crater is an ideal, high-latitude location (\(73^{\circ }\text{N}\)) with large, accessible, near-surface water ice deposits, reducing the need for deep drilling.
Power: The limiting factor will be the mass of solar panels or nuclear reactors required to power the electrolysis process to turn that water into hydrogen, requiring significant cargo mass for power generation.
Launch Windows: These cargo ships must arrive at least one, if not two, synodic periods (26–52 months) before the crew arrives, to ensure the tanks are ful
Missions that proceed must be able to produce propellant:
Establishing a Mars propellant plant to refuel a Starship for a return trip likely requires several cargo missions, with estimates suggesting 2 to 6+ ships to deliver necessary infrastructure (solar panels, mining equipment) and initial fuel stocks. While some scenarios suggest 3-4 ships can enable a return via in-situ resource utilization (ISRU), initial, safer approaches might use 6+ tankers to establish necessary infrastructure.
Infrastructure Requirements: A fully operational plant capable of producing 1,000+ tons of propellant (methane and oxygen) for a return journey requires substantial power, estimated at 5 GWh, needing ~250 metric tons of equipment, equivalent to 2+ fully loaded cargo Starships.
Fuel Mining & Production: The process involves extracting water ice and capturing \(CO_{2}\) from the atmosphere.
Alternative/Interim Methods: Rather than immediate, full ISRU, early missions might rely on landing 3-4 Starships, where 3 are drained to fuel 1 for the return trip, or using 4-6 ships to establish a rudimentary plant.
Scale: SpaceX aims to send at least 2 uncrewed cargo ships before the first crewed mission to set up power, mining, and life support. Ultimately, the number of ships depends on the efficiency of the ISRU plant, the power capacity installed, and the willingness to risk the first crew's return capability
Water source from Korolev Crater
Based on current SpaceX Mars mission architecture, establishing a propellant plant on Mars to refuel a Starship for a return journey, utilizing water ice, requires a multi-stage, cargo-heavy operation. Initial Setup Phase: To establish the necessary propellant plant (Sabatier reactors, mining equipment, solar arrays) at a location like Korolev Crater, early, uncrewed missions would need to land several cargo Starships (potentially 2–5) containing roughly 100+ tons of equipment each.Propellant Production Requirement: To refuel a single Starship for a return journey, the plant must produce approximately 1,200 metric tons of propellant (methane and oxygen).Operational
Requirement: While early estimates suggested 1–2 cargo ships worth of equipment could start production, a more robust and faster turnaround (within one synod, or 26 months) likely requires at least 3-4 cargo ships to be active to ensure enough power and water processing capability to produce the ~1,200+ tons of fuel. In summary, to start a plant, 2-5 dedicated cargo Starships are required to land the equipment, with at least 3-4 of them acting as operational plant components/fuel depots to reliably produce enough fuel for one return trip.
Key considerations: Water Source: Korolev Crater is an ideal, high-latitude location (\(73^{\circ }\text{N}\)) with large, accessible, near-surface water ice deposits, reducing the need for deep drilling.
Power: The limiting factor will be the mass of solar panels or nuclear reactors required to power the electrolysis process to turn that water into hydrogen, requiring significant cargo mass for power generation.
Launch Windows: These cargo ships must arrive at least one, if not two, synodic periods (26–52 months) before the crew arrives, to ensure the tanks are full
Will SpaceX Send Humans to Mars in 2028?
A number of press releases on the Internet claim that SpaceX will send a human mission to Mars as early as 2028, but only very limited information is available [2020Making Life Multiplanetary. Available from: https://www.spacex.com/media/making_lif … pdf.SpaceX. Updates. Available from: https://www.spacex.com/updates/.]. Such a claim is difficult to appraise without further detail, and as far as we can tell the challenges appear to be overwhelming. Maiwald, et al. [2121Maiwald V, Bauerfeind M, Fälker S, Westphal B, Bach C. About feasibility of SpaceX's human exploration Mars mission scenario with Starship. Sci Rep. 2024 May 23;14(1):11804. doi: 10.1038/s41598-024-54012-0. Erratum in: Sci Rep. 2024 Sep 5;14(1):20718. doi: 10.1038/s41598-024-71955-6. PMID: 38782962; PMCID: PMC11116405.] reviewed the SpaceX plan for a large-scale human mission to Mars, making educated guesses about missing data, and they found significant problems with the mass balance for the mission.
The SpaceX plan is extremely ambitious (and is likely to be very costly as well) with at least 72 heavy lift launches to land a crew of twelve and several hundred tons of infrastructure on a long-stay mission.
Several unique architectural innovations were introduced, such as using a single vehicle for departure from LEO, landing on Mars, and returning directly from Mars without rendezvous. The propellants used throughout (transfer to Mars, ascent from Mars, and transfer to Earth (CH4 + O2) remain the same, thus simplifying the mission. The three major challenges are (1) landing a 200 MT vehicle on Mars (2) producing 1,200 MT of CH4 and O2 on Mars via ISRU, and (3) implementing many repeated heavy lift launches. Nevertheless, the SpaceX mission concept provides an interesting departure from previous mission scenarios that might provide a good basis for long-term planning of a human mission to Mars decades in the future.
References
Portree DSF. Humans to Mars: Fifty Years of Mission Planning, 1950—2000. Monographs in Aerospace History. NASA Technical Reports Server (NTRS), Number 21. 2001.Platoff A. Eyes on the Red Planet: Human Mars Mission Planning, 1952-1970. NASA/CR-2001-208928. 2001.
Rapp D. Human Missions to Mars. 3rd ed. Heidelberg: Springer-Praxis Book Co. 2023.
Hoffman SJ, Kaplan DI. Human Exploration of Mars: The Reference Mission of NASA Mars Exploration (DRM-3). NASA Special Publication 6107; 1997.
Drake BG. Human Exploration of Mars – Design Reference Architecture 5.0 (DRA-5). NASA Report SP-2009-566. Human Exploration of Mars Design Reference Architecture 5.0 Addendum. NASA Report SP-2009-566. 2009.
Zubrin R. The Mars direct plan. Sci Am. 2000 Mar;282(3):52-5. doi: 10.1038/scientificamerican0300-52. PMID: 10736835.
McNutt RL Jr., Delamereb WA. Human Exploration of Mars: Cost Realities of a First Mission. 68th International Astronautical Congress (IAC); 2017 Sep 25-29; Adelaide, Australia. IAC-17-A5.IP.10.
Cangi E, Gibson J, Luebbers M. Mission Costs: Past, Present, Future. Humans to Moon and Mars Seminar; 2019 Nov 5. Available from: https://lasp.colorado.edu/mop/files/201 … -costs.pdf.
Smith G, Spudis PD. Op-ed - Mars for Only $1.5 Trillion. Available from: https://spacenews.com/op-ed-mars-for-only-1-5-trillion/.
Jones HJ. Humans to Mars Will Cost About ‘Half a Trillion Dollars’ and Life Support Roughly Two Billion Dollars. 46th International Conference on Environmental Systems; 2016 Jul 10-14; Vienna, Austria. ICES-2016-111.
Bleacher J, Rucker M. Human Mars Exploration. Presentation to: Mars Exploration Program Analysis Group (MEPAG); 2021.
Rucker M. NASA’s Strategic Analysis Cycle 2021 (SAC21) Human Mars Architecture. NASA ESDMD Mars Architecture Team; 2022 Mar 7. 2022 IEEE Aerospace Conference; Big Sky, MT.
Rucker M, et al. NASA’s Strategic Analysis Cycle 2021 (SAC21) Human Mars Architecture. NASA Report; Available from: https://ntrs.nasa.gov/citations/20210026448.
Levine JS. NASA Wants to Send Humans to Mars in the 2030s − a Crewed Mission Could Unlock Some of the Red Planet’s Geologic Mysteries. Available from: https://www.space.com/nasa-wants-humans … ents-68435.
Bell S. NASA Hopes to Send Astronauts to Mars in the 2030s; Here's How They Will Get There. Available from: https://abcnews.go.com/US/nasa-hopes-se … =111859633.
NASA’s Journey to Mars. Essence Festival. Available from: https://www.nasa.gov/specials/reach-new-heights/.
Bridenstine J. Bridenstine Says NASA Planning for Human Mars Missions in 2030s. Available from: https://spacenews.com/bridenstine-says- … -in-2030s/.
Explore Mars. Website Advocating Human Exploration of Mars. Available from: https://www.exploremars.org/summit/?gad … gLO8vD_BwE.
Rapp D. Mars Ascent Propellants and Life Support Resources - Take it or Make it? IgMin Res. 2024 Jul 29;2(7):673-682. DOI: 10.61927/igmin232.
Making Life Multiplanetary. Available from: https://www.spacex.com/media/making_lif … pdf.SpaceX. Updates. Available from: https://www.spacex.com/updates/.
Maiwald V, Bauerfeind M, Fälker S, Westphal B, Bach C. About feasibility of SpaceX's human exploration Mars mission scenario with Starship. Sci Rep. 2024 May 23;14(1):11804. doi: 10.1038/s41598-024-54012-0. Erratum in: Sci Rep. 2024 Sep 5;14(1):20718. doi: 10.1038/s41598-024-71955-6. PMID: 38782962; PMCID: PMC11116405.
Reference Surface Activities for Crewed Mars Mission Systems and Utilization. NASA Report HEOMD-415; 2022. Available from: https://ntrs.nasa.gov/api/citations/202 … update.pdf.
Rapp D. Lunar-Derived Propellants for Fueling Mars-Bound Spacecraft in Cis-Lunar Space. IgMin Res. 2024 Sep 3;2(9):744-751. IgMin ID: igmin242. DOI: 10.61927/igmin242. Available from: igmin.link/p242.
Ewert MK, Chen TT, Powell CD. Life Support Baseline Values and Assumptions Document. NASA Report NASA/TP-2015–218570/REV2; 2015. Available from: https://ntrs.nasa.gov/api/citations/202 … -final.pdf.
Adler M, et al. NASA Draft Entry, Descent, and Landing Roadmap Technology Area 09. 2010 Nov. Available from: http://www.nasa.gov/pdf/501326main_TA09 … 2010-A.pdf.
Braun RD, Manning RM. Mars Exploration Entry, Descent, and Landing Challenges. J Spacecraft Rockets. 2007;44. Available from: https://arc.aiaa.org/doi/10.2514/1.25116.
Manning R. Aerocapture, Entry, Descent and Landing (AEDL) Capability Evolution toward Human-Scale Landing on Mars, Capability Roadmap #7: Human Planetary Landing Systems. NASA Report; 2005 Mar 29. Available from: https://ntrs.nasa.gov/api/citations/200 … 205032.pdf.
Cain F. The Incredible Challenge of Landing Heavy Payloads on Mars. Phys.org; 2019 Mar. Available from: https://phys.org/news/2019-03-incredibl … -mars.html.
Lorenz CG, Putnam ZR. Entry Trajectory Options for High Ballistic Coefficient Vehicles at Mars. J Spacecraft Rockets. 2019;56(3):811-822. Available from: https://arc.aiaa.org/doi/abs/10.2514/1. … alCode=jsr.
Rapp D. Use of Extraterrestrial Resources for Human Space Missions to Moon or Mars. 2nd ed. Springer-Praxis Books; 2018.
The Guardian. Musk Says Humans Can Be on Mars in Four Years. Many Laugh, but Some See Purpose. 2024 Sep 15. Available from: https://www.theguardian.com/technology/ … ars-spacex
A 4-year round-trip mission to Mars represents a long-duration, high-safety-margin, or potentially, a lower-energy, extended-stay scenario often discussed in human spaceflight studies. While, theoretically, minimum-energy missions (Hohmann transfers) take roughly 2-3 years, a 4-year limit is proposed to mitigate cosmic radiation exposure. A typical 3-year mission involves a 6-9 month transit each way with a long, ~18-month, stay.
Radiation Safety Limits: Research indicates that limiting the total round-trip, including the surface stay, to roughly 4 years is crucial to keep astronaut radiation exposure within acceptable limits.
Mission Structure: A 4-year timeframe allows for a more relaxed, extended scientific exploration on the Martian surface compared to "short-stay" missions that only last 2 years but are higher-risk, faster transits.
Alternative Mission Durations: While 4 years is a safe, long-duration option, most near-term mission architectures with current chemical technology focus on 2 to 3-year round trips to manage logistical constraints.
The extended duration of a 4-year mission provides more time for surface operations and potentially reduces the fuel required for rapid orbital maneuvers, at the cost of increased health risks from radiation, which requires robust shielding solutions
The radiation showstopper for Mars exploration
Beating 1 Sievert: Optimal Radiation Shielding of Astronauts on a Mission to Mars
Moon 2 Mars Space Radiation Protection “Buying Down” Risks to Crew
A 4-year round-trip mission to Mars represents a long-duration, high-safety-margin, or potentially, a lower-energy, extended-stay scenario often discussed in human spaceflight studies. While, theoretically, minimum-energy missions (Hohmann transfers) take roughly 2-3 years, a 4-year limit is proposed to mitigate cosmic radiation exposure. A typical 3-year mission involves a 6-9 month transit each way with a long, ~18-month, stay.
Radiation Safety Limits: Research indicates that limiting the total round-trip, including the surface stay, to roughly 4 years is crucial to keep astronaut radiation exposure within acceptable limits.
Mission Structure: A 4-year timeframe allows for a more relaxed, extended scientific exploration on the Martian surface compared to "short-stay" missions that only last 2 years but are higher-risk, faster transits.
Alternative Mission Durations: While 4 years is a safe, long-duration option, most near-term mission architectures with current chemical technology focus on 2 to 3-year round trips to manage logistical constraints.
The extended duration of a 4-year mission provides more time for surface operations and potentially reduces the fuel required for rapid orbital maneuvers, at the cost of increased health risks from radiation, which requires robust shielding solutions
The radiation showstopper for Mars exploration
Beating 1 Sievert: Optimal Radiation Shielding of Astronauts on a Mission to Mars
Moon 2 Mars Space Radiation Protection “Buying Down” Risks to Crew
First missions will have less protection and with duration mars for those first will see long term effects to their lives over time after return.
A 4-year round-trip mission to Mars represents a long-duration, high-safety-margin, or potentially, a lower-energy, extended-stay scenario often discussed in human spaceflight studies. While, theoretically, minimum-energy missions (Hohmann transfers) take roughly 2-3 years, a 4-year limit is proposed to mitigate cosmic radiation exposure. A typical 3-year mission involves a 6-9 month transit each way with a long, ~18-month, stay.
Radiation Safety Limits: Research indicates that limiting the total round-trip, including the surface stay, to roughly 4 years is crucial to keep astronaut radiation exposure within acceptable limits.
Mission Structure: A 4-year timeframe allows for a more relaxed, extended scientific exploration on the Martian surface compared to "short-stay" missions that only last 2 years but are higher-risk, faster transits.
Alternative Mission Durations: While 4 years is a safe, long-duration option, most near-term mission architectures with current chemical technology focus on 2 to 3-year round trips to manage logistical constraints.
The extended duration of a 4-year mission provides more time for surface operations and potentially reduces the fuel required for rapid orbital maneuvers, at the cost of increased health risks from radiation, which requires robust shielding solutions
Humans can safely stay on the Mars surface for a maximum of approximately four years before cumulative radiation exposure from cosmic rays and solar particles becomes too dangerous. While short-term, unprotected exposure would cause death from freezing or suffocation in seconds, long-term, unshielded surface survival is limited by high-energy radiation to about four years.
Key factors and findings regarding radiation on Mars:
Total Mission Time: Studies suggest a round-trip mission (including transit and stay) should be kept under four years to avoid exceeding safe, long-term exposure limits.
Radiation Source: The primary dangers are Galactic Cosmic Rays (GCRs) and solar particle events, which are not blocked by the thin Martian atmosphere.
Surface Risks: Without adequate shielding (e.g., habitat shielding), a person would face high cancer risks and potential acute radiation sickness over long durations.
Mitigation: Optimal mission timing during the "solar maximum" can provide some protection, as the sun's activity helps deflect harmful cosmic rays.
Without a protective spacesuit, an individual would instantly succumb to Mars' near-vacuum atmosphere and freezing temperatures. The four-year limit specifically refers to the cumulative dose of radiation, not immediate, acute, unprotected, unshielded environmental conditions
Radiation mitigation for a first human mission to Mars is a critical "showstopper" challenge, with crew exposures during a 3-year round trip expected to exceed standard safety limits (600 mSv), likely requiring an exception to current regulations and an reliance on "buying down" risks through advanced shielding. The strategy for a first mission will likely be a, combination of passive shielding (materials), operational mitigation (timing/scheduling), and natural terrain protection on the surface.
Key Radiation Mitigation Strategies
Optimal Mission Scheduling (Solar Max): Launching during the solar maximum (when the Sun is most active) is counter-intuitively the best strategy, as the increased solar wind deflects the more dangerous Galactic Cosmic Rays (GCRs). While this increases the risk of Solar Particle Events (SPEs), they are easier to shield against than GCRs.
Hydrogen-Rich Materials: Passive shielding is more effective using low-atomic-mass materials (hydrogen, plastics, rubber, synthetic fibers) rather than metals like aluminum, which can generate dangerous secondary radiation when struck by GCRs. Polyethylene is a top candidate for lining spacecraft.
Martian Regolith Shielding: On the surface, placing 2–3 meters of Martian soil (regolith) over habitats can significantly reduce radiation exposure.
Natural Terrain Shelter: Using natural geological features, such as lava tubes, cliffs, or canyons, offers significant, immediate reduction in radiation, with data showing a 4% reduction in dose simply by parking near a small butte.
"Storm Cellar" Design: Creating a heavily shielded, specialized, and compact area within the spacecraft or habitat to protect the crew during high-energy solar storms.
First Mission Challenges and Risks
Secondary Radiation: High-energy particles can cause a cascade of radiation when they hit shielding, which can be worse than the initial exposure.
Prohibitive Mass: Bringing massive amounts of shielding from Earth is cost-prohibitive, making the use of in-situ resources (like Martian soil) essential.
Health Consequences: Beyond radiation sickness, the primary risks are increased long-term cancer, cardiovascular disease, central nervous system damage, and cognitive decline.
While active shielding (using magnetic fields to deflect particles) is considered the ultimate goal, it is not considered practical for the first, near-term, missions due to power and structural requirements
The radiation showstopper for Mars exploration
Beating 1 Sievert: Optimal Radiation Shielding of Astronauts on a Mission to Mars
Moon 2 Mars Space Radiation Protection “Buying Down” Risks to Crew
Trying to do without prefilling of numbers being generated making use of excel and auto fill to do my best
starting post is carried from the previous days 2026-01-29 last number for the day 237757 - last post 237790
2-1-26 postings
Martian Calender - I have created a martian calender...
Martian Calender - I have created a martian calender...
Daily Recap - Recapitulation of Posts in NewMars by Day
Ring Habitat on Mars Doughnut Torus
Ring Habitat on Mars Doughnut Torus
Ring Habitat on Mars Doughnut Torus
Radiation amount type risk mitigation
Radiation amount type risk mitigation
Radiation amount type risk mitigation
Starship to mars count down 273 days to launch
Bogs and Bog, Floating Island Technology, and Roller Solar.
kbd512 Postings
kbd512 Postings
Housekeeping
Housekeeping
Housekeeping
WIKI Project Designing for Mars
WIKI Project Designing for Mars
Peter Zeihan again: and also other thinkers:
Peter Zeihan again: and also other thinkers:
Google Meet Collaboration - Meetings Plus Followup Discussion
Volcanic Holocaust - Monster Eruption Overdue.
Starship Lunar Lander and landing legs
Why Artemis is “better” than Apollo.
Why Artemis is “better” than Apollo.
Carbon is the New Metal
Carbon is the New Metal
Multi-Ship Expeditions, Starboat & Starship, Other.
Multi-Ship Expeditions, Starboat & Starship, Other.
Risk mitigation priorities for crewed missions to mars
Risk mitigation priorities for crewed missions to mars
Based on current SpaceX projections and studies of the Starship vehicle, the crew size for a mission to Mars is designed to be highly scalable, ranging from small, specialized teams for early missions to over 100 passengers for colonization.
Starship Mars Mission Crew Size Chart (Projected)
Mission Phase Estimated Crew Size Primary Focus
Initial Crewed Missions (2028-2030s) 6 – 15+ Pathfinders, base construction, infrastructure setup
Mature/Mid-Term Missions ~12 – 50 Increased operational efficiency and cargo capacity
Colonization Era (Long Term) 100 – 200+ Rapid, high-volume, cost-effective transportation
Key Factors Impacting Crew Size
Design & Comfort: With 1,000 m³ of usable space, the Starship can accommodate 10–15 people with private cabins and common areas.
Safety & Logistics: Early missions will likely use lower crew numbers (6–8) to prioritize safety, consumables management, and payload for return fuel.
Mission Profile: Initial missions will focus on landing, setting up in-situ resource utilization (ISRU) for fuel, and testing habitation systems.
First Mission Target: Estimates suggest 12 people on the first landing, likely accompanied by 2 or 3 total ships for redundancy.
Note: The first crewed missions are officially targeted for 2028 or late
SpaceX is executing a multi-stage strategic buildup for Mars colonization, centered on the Starship launch system. The ultimate goal is to transport 1 million people and millions of tons of cargo to establish a self-sustaining city by 2050.
Strategic Phase Timeline
2026 (Uncrewed Phase): SpaceX plans to launch approximately five uncrewed Starships during the Earth-Mars transfer window. These missions will carry Tesla Optimus robots to survey resources, test landing reliability, and begin setting up basic ground infrastructure.
2028–2029 (Initial Human Landing): If the 2026 landings succeed, the first crewed mission is targeted as early as 2029. This initial crew of roughly 10–20 people will focus on establishing Mars Base Alpha, building a propellant plant, and installing solar power systems.2030s (Rapid Scaling): The mission cadence will increase significantly with each 26-month window:
2031: Target of 100 Starships.
2033: Target of 500 Starships.
2030s–2040s: Peak cadence of 1,000 to 2,000 Starships launched per window.Housing & Infrastructure for 1,000+
To house the initial population and eventually reach the target of 1,000+ residents, the strategy relies on:
Starships as Habitats: Early colonists will live directly inside the Starship vehicles that transported them. Each ship has roughly 1,100 m³ of pressurized volume, capable of supporting dozens of people.
In-Situ Resource Utilization (ISRU): To sustain 1,000 people, local resources are essential. SpaceX plans to harvest CO₂ from the atmosphere and water ice from the soil to produce methane fuel and breathable oxygen using the Sabatier process.
Industrial Buildup: Early cargo missions will deliver machines for producing fertilizer, building materials for transparent domes, and large-scale solar arrays to power the settlement.Starfactory Production: To support this fleet, SpaceX's "Starfactory" in Texas aims to eventually build one Starship per day.
Summary of Strategic Goals
Objective Target Date Fleet Size
First Uncrewed Landings 2026 5 Ships
First Human Landing 2029 (Aspirational) 20 Ships
Sustainable Outpost Mid-2030s ~100 Ships
Self-Sustaining City 2050 1,000+ ShipsWould you like to explore the specific technical challenges of Mars Base Alpha's life support systems or the current status of the Raptor 3 engines powering this fleet?