Hawaiian Man Files Lawsuit Against the Large Hadron Collider (LHC)

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The Large Hadron Collider (LHC) is set to go online in May of this year. This magnificent machine will accelerate particles and collide them at such high energies that scientists expect to make some of the biggest discoveries ever about the very small (exotic sub-atomic particles) and the very large (the structure of the Universe itself).

But not everyone is happy. Particle accelerators have always been the source of controversy; at the end of the day, we can only predict the outcome of the LHC experiments. But what if scientists have overlooked something? What if the theories are wrong? A guy living on the other side of the planet to the LHC believes the world may come to an end and he’s begun filing a lawsuit against the completion of the accelerator. The concern? A massive black hole might be created, or vast amounts of antimatter will destroy the Earth. And where’s the scientific basis for all this panic? Hmmm… didn’t think so…

Through fear that the LHC is going to unleash death and destruction on the world, Walter Wagner from Hawaii has filed a lawsuit against an impressive array of defendants. The U.S. Department of Energy, the Fermilab particle-accelerator near Chicago, CERN and the National Science Foundation (NSF) are all named.

Wagner and his associate Luis Sancho have a pretty dubious (and quite frankly, weak) argument against the LHC, as they describe in the lawsuit:

The compression of the two atoms colliding together at nearly light speed will cause an irreversible implosion, forming a miniature version of a giant black hole. […] Any matter coming into contact with it would fall into it and never be able to escape. Eventually, all of earth would fall into such growing micro-black-hole, converting earth into a medium-sized black hole, around which would continue to orbit the moon, satellites, the ISS, etc.” Walter F. Wagner and Luis Sancho lawsuit, filed in U.S. District Court in Honolulu.

There is no evidence to suggest that colliding particles will create a black hole that will swallow the planet. I do however like their description that the International Space Station will continue to orbit the Earth-mass black hole – at least we’ll have somewhere to hide as the rampaging black hole eats the ground from under us!

The credentials of the plaintiffs are also pretty sketchy. Wagner has worked in nuclear medicine and has a minor degree in physics from Berkley, but he has nothing more advanced than that. His colleague Sancho has an even more sketchy physics background.

Wagner wants the opening of the LHC to be delayed until further safety studies are carried out. Its cases like these that scientists have had to combat for many years. Unfounded predictions of the “end of the world” and fear of the unknown have been published only to be debunked through correct scientific thinking. If the world listened to alarmists such as Wagner and co, we would advance no further.

I for one hope that the LHC does produce micro-black holes. I hope that this time next year we’ll be looking in awe at images of particle tracks from the sensors at the LHC showing the point of creation and the point of evaporation of micro-black holes. Peering very closely we see particle emission as if from nowhere, the evaporating particles from the tiny event horizon. The image will be entitled Hawking Radiation Experiment.

Even if the accelerator energies are not high enough to create mini-black holes, thereby giving Stephen Hawking some experimental evidence for his radiation, we are pretty sure we’ll find some other exotic and exciting particles to help us understand our universe a little bit better. We might gain a better grasp of other dimensions, detect some exotic particles, and lets not forget the possibility of discovering the Higgs Boson.

If we give into the fear of the unknown, scientific advancement will be stopped in its tracks and we may be restricted to scratching at the surface of space-time and string theory, rather than physically proving its existence with tools like the LHC.

Source: FOXnews.com

Under Construction: SpaceShipTwo, on Course for 2009 Testflight (Pictures)

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It is really taking shape. The future of Virgin Galactic’s fleet of space tourism rockets is currently forming in a non-descript factory in the Mojave Desert, California. As if to prove that the Scaled Composite-design is not a pipe dream, pictures of the first commercial spaceflight vehicle have been released. It looks fairly crude and welded together, but this forms the bare bones of the worlds first viable hi-tech space tourism vehicle. All it needs now are some windows, seats, wings and an engine and we’re good to go!

Scaled Composites owner, Burt Rutan inside the next SpaceShipTwo (credit: Scaled Composites)
It is as if Scaled Composites wanted to trump their competitor’s cards with proof that the SpaceShipTwo design is more than just a concept. It seems that everyone is claiming a portion of the space tourism industry, including economy class. Nancy covered XCOR’s press release (26th March) that the company was designing a smaller, cheaper, economy-class space plane, designed to take two people into low-Earth orbit (note: lower Earth orbit than Virgin Galactic’s design). Even the rocket builder Astrium has gotten in on the act, claiming that there will be a market for their mass-produced conventional space plane (18th March), releasing some uber-cool images and simulations of the craft in action.

The SpaceShipTwo production line (credit: Scaled Composites)

So the economy-class market has been claimed by XCOR and Astrium has grabbed the “AirBus-in-space” mass-production market. But in the aim to prove that “the original and the best” concept is actually growing beyond the design phase and in full production, Scaled Composites are proving that their spaceship is one step closer than all their competitors: they’re building their spaceship right now.

To rub it in, one photo shows Burt Rutan sitting proudly inside the shell of the SpaceShipTwo cockpit proving they are accelerating production toward a 2009 test-run. These new images are from the production line in a factory in the Californian Mojave Desert.

The finished product. Artist impression of SpaceShipTwo (credit: Virgin Galactic)

SpaceShipTwo will carry six people into the lower limit of space and will experience a few minutes of weightlessness. The craft will be helped on its way by the WhiteKnightTwo aircraft, giving the rocket a piggyback ride to 50,000 ft. At this height, SpaceShipTwo will be released and its rockets will blast to life taking the first tourists into space. You can find out more about SpaceShipTwo in a previous Universe Today story.

Source: Popular Mechanics

13.73 Billion Years – The Most Precise Measurement of the Age of the Universe Yet

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NASA’s Wilkinson Microwave Anisotropy Probe (WMAP) has taken the best measurement of the age of the Universe to date. According to highly precise observations of microwave radiation observed all over the cosmos, WMAP scientists now have the best estimate yet on the age of the Universe: 13.73 billion years, plus or minus 120 million years (that’s an error margin of only 0.87%… not bad really…).

The WMAP mission was sent to the Sun-Earth second Lagrangian point (L2), located approximately 1.5 million km from the surface of the Earth on the night-side (i.e. WMAP is constantly in the shadow of the Earth) in 2001. The reason for this location is the nature of the gravitational stability in the region and the lack of electromagnetic interference from the Sun. Constantly looking out into space, WMAP scans the cosmos with its ultra sensitive microwave receiver, mapping any small variations in the background “temperature” (anisotropy) of the universe. It can detect microwave radiation in the wavelength range of 3.3-13.6 mm (with a corresponding frequency of 90-22 GHz). Warm and cool regions of space are therefore mapped, including the radiation polarity.

This microwave background radiation originates from a very early universe, just 400,000 years after the Big Bang, when the ambient temperature of the universe was about 3,000 K. At this temperature, neutral hydrogen atoms were possible, scattering photons. It is these photons WMAP observes today, only much cooler at 2.7 Kelvin (that’s only 2.7 degrees higher than absolute zero, -273.15°C). WMAP constantly observes this cosmic radiation, measuring tiny alterations in temperature and polarity. These measurements refine our understanding about the structure of our universe around the time of the Big Bang and also help us understand the nature of the period of “inflation”, in the very beginning of the expansion of the Universe.

It is a matter of exposure for the WMAP mission, the longer it observes the better refined the measurements. After seven years of results-taking, the WMAP mission has tightened the estimate on the age of the Universe down to an error margin of only 120 million years, that’s 0.87% of the 13.73 billion years since the Big Bang.

Everything is tightening up and giving us better and better precision all the time […] It’s actually significantly better than previous results. There is all kinds of richness in the data.” – Charles L. Bennett, Professor of Physics and Astronomy at Johns Hopkins University.

This will be exciting news to cosmologists as theories on the very beginning of the Universe are developed even further.

Source: New York Times

Cassini Sniffs Organic Chemicals Leaking into Space from Saturn Moon, Enceladus

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During a flyby of the small moon on March 12th, the Cassini probe detected significant amounts of organic chemicals as it flew through powerful geyser-like jets of ice blasting into space. This active moon appears to be generating organic chemicals much like the substances found in comets. As Cassini bravely travelled through the plume at a speed of 32,000 mph, it was able to take some indirect measurements of the density of the gas from the surprising amount of torque applied to spacecraft. Fortunately the craft was undamaged as the particles bounced off its bodywork…

Cassini took the daring journey through the plumes of ice crystals and gas at 200 km above the moon’s surface. It came within 50 km of the surface at closest approach, giving mission scientists an unprecedented view of the mysterious satellites northern hemisphere. Images acquired by Cassini showed a vast, ancient region of pits and craters mixed with cracks, with geysers fizzing chemicals into space. Enceladus is located in the densest region of Saturn’s E-ring, possibly indicating there is some relationship between the geyser emissions and ring density.

To discover significant quantities of organic compounds being emitted from the Saturn system is of particular interest to scientists trying to understand how Saturn evolved as the solar system formed.

A completely unexpected surprise is that the chemistry of Enceladus, what’s coming out from inside, resembles that of a comet, to have primordial material coming out from inside a Saturn moon raises many questions on the formation of the Saturn system.” – Hunter Waite, principal investigator for the Cassini Ion and Neutral Mass Spectrometer, Southwest Research Institute, San Antonio

Saturns rings and moons (credit: NASA)

From measurements by the Ion and Neutral Mass Spectrometer on Cassini, scientists are able to deduce that the moon is highly active, driven by an internal energy source. There is also evidence for tectonic activity on the 500 km diameter body. The gases detected can be likened to the fizz of gas released from carbonated water, with a twist of organic chemicals mixed in. The spectrometer effectively “tasted and sniffed” the gas and was able to get a good idea about what the energetic geysers are spewing into space.

The gases detected, over 20 times more dense than estimated, contained water vapour, carbon dioxide, carbon monoxide, organic compounds and volatile molecules. Quite an explosive mix. The clouds of gas were so dense that the spacecraft felt the force of the emission, creating a torque. From this, some measurements on gas density were possible.

It is thought Cassini was unharmed during the flyby and it will return in August for an even more daring, lower flyby of this strange, gassy moon.

Source: NASA

The Sun Bursts to Life: Sunspots, Flares and CMEs

The new sunspots appearing as the Sun rotates (credit: Greg Piepol)

As if to remind us it is still there, the Sun has put on an explosive show of sunspots, flares and coronal mass ejections (CMEs). This is quite surprising as only last month it was declared that the Sun had just started a new solar cycle, and a period of minimum activity. Up until now, the solar disk has been void of any observable features… but like an invasion party, three sunspots have rotated into view, showing complex arcs of magnetic fieldlines (coronal loops), blasting plasma into space by the biggest flare observed this year. Observers have also recorded the radio burst from the CME, so if you want to know what a CME sounds like, read on…

The magnetic flux of the Sun through the solar cycle (credit: Ian O'Neill)

The Sun undergoes an 11 year cycle, beginning at “solar minimum”, culminating at “solar maximum”, and then calming down toward minimum again. At solar minimum, the Sun’s magnetic field lines, reaching from pole to pole, are at their least stressed state. As the cycle progresses, the differential rotation of the Sun (i.e. the Sun rotates quicker at its equator) drags the magnetic field lines around the solar body like an elastic band. As time goes on, the magnetic field lines become so stressed and coiled that massive loops of magnetic flux breaks through the solar photosphere (the solar “surface”). As the Sun’s atmospheric layers are hotter than the Sun’s interior (a situation known at the “coronal heating problem“), as the magnetic loops of flux appear through the photosphere, the cooler interior is exposed. When this happens, sunspots appear; the cooler interior looks darker than the surrounding photosphere, therefore creating a spot, or a “sunspot”.

If there are a lot of sunspots, the magnetic field is most stressed, and the Sun is at its most active. The magnetic flux may get so stressed that it may “reconnect” with opposite polarities, releasing huge amounts of energy as flares. Coronal mass ejections may be unleashed from these flare events, sending hot solar plasma into space. If directed at the Earth, these CMEs can cause damage to satellites, astronauts, even whole power grids on the ground. Predicting space weather (i.e. observing solar dynamics) is therefore paramount to scientists.

The CME caught by the Solar and Heliospheric Observatory, LASCO instrument (credit: SOHO)

Interestingly, these sunspots are not from a new cycle, they are actually “left overs” from the previous cycle. Solar astronomers know this by analysing Michelson Doppler Imager (MDI) images from the Solar and Heliospheric Observatory (SOHO) currently observing the Sun. The MDI instrument has revealed that the sunspots are of the same polarity as the spots from the previous solar cycle, and not from “Solar Cycle 24“.

Yesterday, the Sun unleashed an M2-class solar flare which in-turn created a large CME, propagating away from the solar disk. The CME was not directed toward Earth. A radio astronomer in New Mexico, Thomas Ashcraft, recorded the sound coming from his 21 MHz radio telescope during the event. He heard a strange “heaving sound” as the shock wave on the leading edge of the CME generated radio waves.

Listen to the sound of the radio wave emission from a CME as it travels from the Sun.

It was a Type II solar radio burst.” – Thomas Ashcraft, remarking on his observation of the CME.

Space weather predictions suggest there is a 50% chance of more M-class flares in the next 24 hours, so the world’s solar telescopes will be watching and waiting…

For more stunning images of the Sun by Greg Piepol (like the sunspots pictured at the top) see: http://www.sungazer.net/032508h.html

Source: spaceweather.com

NASA U-Turn Over Mars Rover Funding

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No sooner had news hit the web that NASA had cut funding to the Mars Exploratory Rovers (MER), NASA took a huge U-turn and voided the letter that was sent to MER mission scientists. Apparently both Spirit and Opportunity can continue to roll around the Mars landscape as if nothing had ever happened; in fact the two robots will probably be unaware of the drama that unfolded here on Earth in the last 24 hours. Talk about a storm in a teacup…

But what caused the change of heart? What was behind all this funding craziness? Unfortunately, this ordeal highlights the pressures government-funded space agencies are under, and it is unlikely this will be the end of it…


You could almost hear the news sites and blogs rumble to life last night as the news surged through the web about NASA needing to cut $4 million from the MER program. Reports flooded in that the rover scientists were shocked and saddened by this surprise turn of events, the whole world seemed to react. Every other story on Digg.com showed a new article about the budget cut, and looking through the comments, most reactions were of shear disgust about the short-sightedness of the government funded space agency. After all, Spirit and Opportunity represent the most successful robotic planetary mission ever; to simply switch one of them off seemed like a crime. Rushing to the keyboard I posted my five cents worth on the Universe Today, thinking to myself “this is insane”, but wondering why it was happening.

Spirit and Opportunity landed on the Red Planet in 2004 and were only expected to live for a few months. The previous successful rover, Sojourner (of NASA’s Pathfinder mission in 1997), was expected to last for a couple of weeks, it survived for three months. So expectations were high for the MER program. Not only did the 2004 mission surpass the few months the rovers were designed for, they have both independently survived the last four years and the science they are carrying out has surpassed even the most extreme predictions. Every day we read about new discoveries coming from our intrepid explorers on Mars, they have been embraced by the international community, and they are as popular as ever.

So it is understandable that when it is announced that Spirit will need to be “turned off” for a few weeks and Opportunity will be on a “go slow”, the news sites should go crazy. I spotted several commenters and blogs requesting a petition to be sent to Congress.

The disappointment extends beyond the two rovers, what about the 300+ highly trained scientists in the Californian Jet Propulsion Lab (JPL)? Where would they go? Would they be transferred or laid off? The worry was obvious when MER principal investigator, Steve Squyres, gave a statement: “It’s very demoralizing for the team […] we would have to make some very tough decisions about which one we would hibernate and which one we would keep active. That’s a situation I do not want to face … but that’s a future worry.”

The reasons for this false alarm have been attributed to the “unexpected” long overrun of the MER mission and the ever increasing bill for the future Mars Science Laboratory Mission; a cut of $4 million was therefore inevitable.

But why the turnaround? Did NASA change its mind after being shocked by the outpouring of shock from the public? It is hard to say. So far, the only piece of extra information I have found is from the Associated Press where a letter was sent to JPL instructing mission scientists of the budget cut, but the letter was not approved by NASA Administrator Michael Griffin. When the cut was announced at JPL, NASA withdrew the letter and instructed the MER team to continue as if the letter was never sent.

I’m sure there are some questions as to why an unapproved financial letter was ever sent to JPL in the first place (I personally think NASA needs to get its paperwork in order).

So the Mars rovers can breathe a sigh of relief. However, the fact remains that NASA is under increasing pressure to save money, and an overrunning rover mission on Mars (although a massive success) still costs millions in research funding.

Original Source: AP

A Space War would be a Seriously Messy Business

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What if there was a Pearl Harbour-like, pre-emptive strike against orbiting satellites? What if our quarrels on the ground spill into space? This is no longer a storyline for the next sci-fi movie, early warning systems are currently being developed to defend satellites, low Earth orbit satellites are being quickly and accurately shot down by the US and China, plus satellite technology is becoming more and more valuable as a strategic target. Like all wars there is a losing side, but in the event of a war in space, we’ll all be losers.

Its one thing watching a space battle in a sci-fi movie, it’s quite another to see it happen in reality. The critical thing about blowing stuff up in space is it produces a lot of mess and will leave a nasty legacy for future generations. Space debris is becoming a serious problem and should there be some form of orbital war, the debris produced may render space impassable.

As satellite technology becomes more and more important for communication and navigation, should a pre-emptive attack by an aggressive state be carried out, blowing up satellites in low Earth orbit (LEO) will become a priority. Imagine if a nation lost its ability to communicate with its armed forces around the globe, or if strategic missiles were suddenly rendered useless, the state being attacked will be electronically blinded.

In an article posted on The Space Review by Taylor Dinerman, some important factors are addressed. Significantly, should there be a large-scale attack by a rogue nation on a US LEO satellite network; the disruption caused to military communications could be catastrophic. Indeed, the disruption caused to such a satellite network may be desirable enough for small nations to pursue anti-satellite technology.

But what if the worst does happen and satellites become the primary targets for “hot” wars down here on Earth? What can be done to reduce the amount of debris produced? After all, cutting down on space debris is an international concern, having a “scorched earth” policy in space would ultimately be self-defeating. Dinerman examines some possible solutions:

  • Develop highly destructive anti-satellite missiles. If the missiles carry warheads of sufficient destructive energy, satellites may be completely pulverized, rendering the mass of the orbiter into harmless bits of dust.
  • Build an early warning system and highly manoeuvrable military-design satellites. Expensive, in money and fuel, but worth it should there be a space war.

Regardless of whether there will be a future space battle in Earth orbit, it is quickly becoming the responsibility of the military and private companies of all nations to design and build critical satellites with some built-in ability to protect themselves from attack. And this isn’t only to maintain communications or guide ballistic missiles to targets; it is to safeguard mankind’s ability to access space by reducing the risk posed by the ever increasing population of space debris currently trapped in orbit.

Should the worst happen, and the space-ways become so heavily congested with debris, at least you’ll be able to track it with Google Earth!

Source: The Space Review: “Messy battlefields” by Taylor Dinerman

Spirit Rover is Switched Off to Save NASA Money (Update)

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To save the Mars Expedition Rover (MER) program some cash, controllers will be forced to switch one of the four-year old rovers into “hibernation mode”. NASA wants to cut $4 million from the MER budget, so extreme measures are needed. Sadly, operations will need to be limited and it has been announced today that activities will be stopped on Spirit for the coming weeks. Mission scientists are obviously demoralized.

[UPDATE (03/25/08): NASA has now announced that it has “absolutely no plans” to turn off the Mars rovers, only hours after mission scientists announced they had new directives from the organization to cut $4 million from budget cuts. When more news is forthcoming I will post an article as to what is going on… ]

This appears to be the case of a mission being too successful for its own good.

The MER project was only intended to last for a few months, but the two rovers, Spirit and Opportunity, have surpassed all expectations and continued to explore the planet for four whole years. They are so efficient, that they have braved the worst dust storms, battled through technical issues and even freed themselves from quicksand, there seems to be nothing standing in their way of these super robotic troopers…

Except NASA budget cuts.

When the money runs out, the rovers have to be shut down and this is exactly what is going to happen to Spirit, currently located on a sunny slope at Gusev Crater. Even though the rovers are in the middle of an extensive exploratory phase of the Martian landscape, a NASA directive must be enforced to save $4 million from the project’s $20 million annual budget.

Shutting down Spirit isn’t the only budget-saving measure to be taken. Opportunity’s tasks will now be severely cut; limiting commands to be sent from controllers to every other day, rather than daily.

MER controllers are said to be very demoralized by these measures. Although budget cuts can never come at a “good time”, the timing of this announcement is terrible as both rovers are operating at full strength and still have vast amounts of potential.

The problem is that NASA is currently being stretched to accommodate other Mars missions currently in operation. But when should a highly successful mission like the MER project end? Up till now, most Mars surface missions are good until they break down. In the case of Spirit and Opportunity, neither is showing many signs of breaking. So for now, controllers will have to hover by the “off” switch while budget requirements are met.

Source: PhysOrg.com

Light Echos from 400 Year Old Supernova Observed for the First Time (Time-lapse Video)

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Its observations like these that really give us an idea about how big the cosmos actually is. A star in a small galaxy called the Large Magellanic Cloud (LMC), some 160,000 light years from Earth, exploded as a massive supernova 400 years ago (Earth years that is). Combining the observations from an X-ray observatory and an optical telescope, scientists are currently observing the reflected light off galactic dust, only just reaching the Earth hundreds of years after the explosion…

Shakespeare’s first run the stage production, Hamlet, will have been in full-swing. Galileo might have been experimenting with his first telescope. Guy Fawkes could have been plotting to blow up the British parliament. These events all occurred around the beginning of the 17th Century when a bright point of light may have been seen in the night sky. This point of light, in the Large Magellanic Cloud (LMC), is a massive star exploding, ending its life in a powerful supernova.

Now, 400 years after the event, we can see a “supernova remnant” (SNR), and this particular remnant is known as SNR 0509-67.5 (not very romantic I know). The remnant of superheated gas slowly expands into space and still emits X-rays of various energies. The 400 year old explosion has even been imaged in great detail by the Chandra Observatory currently observing space in X-ray wavelengths. Analysis of the SNR indicates that it was most likely caused by a Type Ia supernova after analysis of the composition of the gases, in particular the quantities of silicon and iron, was carried out. It is understood that the supernova was caused when a white dwarf star in a binary system reached critical mass, became gravitationally unstable (due to fusion reactions in the core stopping) and exploded.

When SNR 0509-67.5 exploded all those years ago, it will have radiated optical electromagnetic radiation (optical light) in all directions of space. Now, for the first time, optical Blanco 4-meter telescope at Cerro Tololo Inter-American Observatory (Chile) has observed reflected light from within the LMC originating from the supernova, 400 years after the event. Using the (reflected) optical light and X-ray emissions directly from the supernova remnant, scientists have been able to learn just how much energy was generated by the explosion.

Astronomers have even assembled a time-lapse video from observations of the light “echo” from 2001 to 2006. Although there are only five frames to the video, you can see the location of the reflected light change shape as different volumes of galactic dust are illuminated by the flash of supernova light. In each progressive frame, the clouds of gas that become illuminated will be further and further away from us, we are effectively looking further back in time as the light “echoes” bounce off the galactic matter.

An amazing discovery.

Source: Chandra X-ray Observatory

Building a Moon Base: Part 4 – Infrastructure and Transportation

In this exciting but challenging period of space exploration, the time is fast approaching for serious design concepts for the first habitats that will be built on the lunar landscape. In previous articles, we have examined the hazards associated with such an endeavor, we have looked at the structures available to us, we have even detailed a particular hangar-like structure that might use locally mined materials. Now, we look into the possible infrastructure elements that will be needed to support a viable colony on the Moon. Florian Ruess, a structural engineer who is working on the future of habitats in extreme environments, also took some time with the Universe Today to give his opinions on our future on lunar soil…

Imagine trying to build a structure on the surface of the Moon. Two of the biggest obstacles the first lunar settlers will come across are the very low gravity and the fine dust causing all sorts of construction issues. Although it seems likely that the first habitats will be built by automated processes before we even set foot on the moon, fabrication of a settlement infrastructure will be of primary concern to engineers so construction can be made as efficient as possible.

The basic, but optimal shape for a lunar habitat module linked with other modules (image courtesy of Florian Ruess)

Infrastructure will be one of the most important factors concerning mission planners. How will building materials be fabricated? How will the material be supplied to construction workers? How will precious water and food be supplied to the fledgling lunar colony? Can supply vehicles go from A to B with little effort?

Historic examples of the effectiveness of efficient transportation infrastructure can be seen in the coalescence of cities around rivers (traditionally the quickest way to transport people and material around a country). Canals were instrumental in bringing cities to life during the Industrial Revolution in the UK in the late 18th century. As railway lines linked the East and West of North America in the last half of the 19th century, acceleration in population growth was experienced by people uprooting and “homesteading” the new, accessible farmlands. Over the last 50 years, the “Southern California freeway effect” is responsible for the proliferation of gas stations, restaurants, shops, followed by residential areas for workers – eventually, whole towns and cities are based around the ease of access for transportation.

Concepts of a lunar infrastructure (credit: NASA)

Future settlement of the Moon and Mars will most likely be based on a similar principle; the success of a lunar settlement will heavily depend on the efficiency of the transport structure.

It seems likely that most transportation around the Moon will depend on wheeled methods, following from terrestrial vehicles and tried and tested “Moon buggies” from the Apollo missions in the 1960s and ’70s. There are some significant drawbacks, however. Addressing this issue, Florian Ruess, structural engineer and collaborator with Haym Benaroya (whose publication this article is based) point out some problems with this mode of transport:

For any mission there will always be the need for individual transportation and the obvious solution is some wheeled vehicle. But there are a couple of serious issues with this solution:

  • Reduced traction. 1/6 gravity and the lunar soil make traction a problem just like [the Mars Exploration Rovers] Spirit and Opportunity on Mars one can get stuck easily or need to much power to get around.
  • Dust. Apollo experience shows that a lot of dust is levitated by wheeled vehicles. This dust is hazardous to machines and humans when breathed in.”

– Florian Ruess (private communication)

So traveling around in a modified “dune buggy” might not be the answer for an established Moonbase, some form of road infrastructure would be needed if wheeled transportation is used.

Neil Armstrong's footprint in the lunar regolith (credit: NASA)

Disturbing dust on the lunar surface is far from being a minor problem. From NASA’s experience with the Apollo missions, by far the biggest contributor to dust generation was the takeoff and landing of lunar modules. 50% of the regolith is smaller than fine sand and approximately 20% is smaller than the “dusty” 0.02mm that preserved the Neil Armstrong’s first boot prints. It is this very fine component of the regolith that can cause a host of mechanical and health problems:

  1. Vision impairment
  2. Incorrect instrument readings
  3. Dust coating
  4. Loss of traction
  5. Clogging of mechanisms
  6. Abrasion
  7. Thermal control problems
  8. Seal failures
  9. Inhalation

It, therefore, seems obvious that dust creation should be kept to the bare minimum as this factor could be a severe hindrance to the infrastructure of the settlement.

Roads are would be the perfect answer to the new lunar colony. They would provide wheeled vehicles with the much-needed traction (thus having a knock-on effect with the fuel efficiency of the vehicle) and may significantly reduce the amount of dust suspension, especially if the road surface is raised above the surrounding regolith. Roads, however, have their drawbacks. They are enormously costly and may be very difficult to build. Fusing regolith to form a tough surface may be an answer, but as pointed out by Ruess, “…this requires enormous energies, which cannot be provided by solar power alone.” So an alternate form of energy would be required to perform such a construction.

(a) Basic Roman road design features, (b) 2000 road design, (c) model of force distribution (credit: Haym Benaroya, Leonhard Bernold)

Although road construction would be highly desirable, it may not be possible, at least in the early stages of lunar settlement development. One emerging development in alternative space transportation is the vertical take-off and landing method, but as previously stated, rocket-powered take-off and landing produce vast amounts of dust. But should there be multiple bases on the Moon, this might be a possibility, “…a lot of people recommend different solutions for routes that will be used frequently like getting from the landing pad to the settlement or from one settlement to the next,” Ruess adds.

Lunar habitat with a cable-based transportation infrastructure (credit: H. Benaroya, L. Bernold)

Another solution is an established form of transportation. Totally avoiding contact with the surface, thus cutting down on dust and avoiding obstacles, a lunar cable car might be a viable possibility. It seems likely that such a cable car transportation network would be highly effective. “Very large spans will be possible on the Moon and therefore infrastructure cost not exorbitant,” Ruess points out. This possibility is being seriously considered by lunar settlement planners.

Looking back on the previous articles in the series, Florian Ruess comments on whether lunar bases can be mobile and points out some of the severe difficulties facing settlement planners if locally mined materials are to be used:

I am not a big fan of mobile bases. Such a system that includes power generation, communications and especially long-term meteoroid and radiation protection does not seem feasible to me. But the wheeled vehicles could be pressurized designs capable of serving several-day-long science missions. This would be a good solution to expand the capabilities of a permanent base.

Local materials are a crucial yet difficult issue. My research so far has shown that only after a certain presence has been established and experience with lunar issues and materials has been gained we would be in a position to dare and build habitats from local materials. Certainly not before humans set foot on the Moon. And please forget about the much-cited lunar concrete! There are so many showstoppers for this imaginary material that I don’t even want to start mentioning them. The only early local material application I see is meteoroid and radiation protection using regolith as shielding material.

“Building a Moon Base” is based on research by Haym Benaroya and Leonhard Bernold (“Engineering of lunar bases“)

Plus an exclusive interview with Florian Ruess, extreme habitat structural engineer and founder of Habitats for Extreme Environments – HE2

-Florian Ruess, private communication.

Many thanks to Florian Ruess for his time in contributing to this article. For further information about his work and extreme environment habitat designs, visit his website at HE-squared.com.

For more information about the future of lunar settlement, check out the Moon Society and the collaborative resource, Lunarpedia.