Space settlement proponents and science fiction fans are likely familiar with the Stanford Torus, a gigantic donut-shaped spinning space habitat that could provide Earth-like gravity and climate for as many as 140,000 people.
Science fiction has told us again and again, we belong out there, among the stars. But before we can build that vast galactic empire, we’ve got to learn how to just survive in space. Fortunately, we happen to live in a Solar System with many worlds, large and small that we can use to become a spacefaring civilization.
This is half of an epic two-part article that I’m doing with Isaac Arthur, who runs an amazing YouTube channel all about futurism, often about the exploration and colonization of space. Make sure you subscribe to his channel.
This article is about colonizing the inner Solar System, from tiny Mercury, the smallest planet, out to Mars, the focus of so much attention by Elon Musk and SpaceX. In the other article, Isaac will talk about what it’ll take to colonize the outer Solar System, and harness its icy riches. You can read these articles in either order, just read them both.
At the time I’m writing this, humanity’s colonization efforts of the Solar System are purely on Earth. We’ve exploited every part of the planet, from the South Pole to the North, from huge continents to the smallest islands. There are few places we haven’t fully colonized yet, and we’ll get to that.
But when it comes to space, we’ve only taken the shortest, most tentative steps. There have been a few temporarily inhabited space stations, like Mir, Skylab and the Chinese Tiangong Stations.
Our first and only true colonization of space is the International Space Station, built in collaboration with NASA, ESA, the Russian Space Agency and other countries. It has been permanently inhabited since November 2nd, 2000. Needless to say, we’ve got our work cut out for us.
Before we talk about the places and ways humans could colonize the rest of the Solar System, it’s important to talk about what it takes to get from place to place.
Just to get from the surface of Earth into orbit around our planet, you need to be going about 10 km/s sideways. This is orbit, and the only way we can do it today is with rockets. Once you’ve gotten into Low Earth Orbit, or LEO, you can use more propellant to get to other worlds.
If you want to travel to Mars, you’ll need an additional 3.6 km/s in velocity to escape Earth gravity and travel to the Red Planet. If you want to go to Mercury, you’ll need another 5.5 km/s.
And if you wanted to escape the Solar System entirely, you’d need another 8.8 km/s. We’re always going to want a bigger rocket.
The most efficient way to transfer from world to world is via the Hohmann Transfer. This is where you raise your orbit and drift out until you cross paths with your destination. Then you need to slow down, somehow, to go into orbit.
One of our primary goals of exploring and colonizing the Solar System will be to gather together the resources that will make future colonization and travel easier. We need water for drinking, and to split it apart for oxygen to breathe. We can also turn this water into rocket fuel. Unfortunately, in the inner Solar System, water is a tough resource to get and will be highly valued.
We need solid ground. To build our bases, to mine our resources, to grow our food, and to protect us from the dangers of space radiation. The more gravity we can get the better, since low gravity softens our bones, weakens our muscles, and harms us in ways we don’t fully understand.
Each world and place we colonize will have advantages and disadvantages. Let’s be honest, Earth is the best place in the Solar System, it’s got everything we could ever want and need. Everywhere else is going to be brutally difficult to colonize and make self-sustaining.
We do have one huge advantage, though. Earth is still here, we can return whenever we like. The discoveries made on our home planet will continue to be useful to humanity in space through communications, and even 3D printing. Once manufacturing is sophisticated enough, a discovery made on one world could be mass produced half a solar system away with the right raw ingredients.
We will learn how to make what we need, wherever we are, and how to transport it from place to place, just like we’ve always done.
Mercury is the closest planet from the Sun, and one of the most difficult places that we might attempt the colonize. Because it’s so close to the Sun, it receives an enormous amount of energy. During the day, temperatures can reach 427 C, but without an atmosphere to trap the heat, night time temperatures dip down to -173 C. There’s essentially no atmosphere, 38% the gravity of Earth, and a single solar day on Mercury lasts 176 Earth days.
Mercury does have some advantages, though. It has an average density almost as high as Earth, but because of its smaller size, it actually means it has a higher percentage of metal than Earth. Mercury will be incredibly rich in metals and minerals that future colonists will need across the Solar System.
With the lower gravity and no atmosphere, it’ll be far easier to get that material up into orbit and into transfer trajectories to other worlds.
But with the punishing conditions on the planet, how can we live there? Although the surface of Mercury is either scorching or freezing, NASA’s MESSENGER spacecraft turned up regions of the planet which are in eternal shadow near the poles. In fact, these areas seem to have water ice, which is amazing for anywhere this close to the Sun.
You could imagine future habitats huddled into those craters, pulling in solar power from just over the crater rim, using the reservoirs of water ice for air, fuel and water.
High powered solar robots could scour the surface of Mercury, gathering rare metals and other minerals to be sent off world. Because it’s bathed in the solar winds, Mercury will have large deposits of Helium-3, useful for future fusion reactors.
Over time, more and more of the raw materials of Mercury will find their way to the resource hungry colonies spread across the Solar System.
It also appears there are lava tubes scattered across Mercury, hollows carved out by lava flows millions of years ago. With work, these could be turned into safe, underground habitats, protected from the radiation, high temperatures and hard vacuum on the surface.
With enough engineering ability, future colonists will be able to create habitats on the surface, wherever they like, using a mushroom-shaped heat shield to protect a colony built on stilts to keep it off the sun-baked surface.
Mercury is smaller than Mars, but is a good deal denser, so it has about the same gravity, 38% of Earth’s. Now that might turn out to be just fine, but if we need more, we have the option of using centrifugal force to increase it. Space Stations can generate artificial gravity by spinning, but you can combine normal gravity with spin-gravity to create a stronger field than either would have.
So our mushroom habitat’s stalk could have an interior spinning section with higher gravity for those living inside it. You get a big mirror over it, shielding you from solar radiation and heat, you have stilts holding it off the ground, like roots, that minimize heat transfer from the warmer areas of ground outside the shield, and if you need it you have got a spinning section inside the stalk. A mushroom habitat.
Venus is the second planet in the Solar System, and it’s the evil twin of Earth. Even though it has roughly the same size, mass and surface gravity of our planet, it’s way too close to the Sun. The thick atmosphere acts like a blanket, trapping the intense heat, pushing temperatures at the surface to 462 C.
Everywhere on the planet is 462 C, so there’s no place to go that’s cooler. The pure carbon dioxide atmosphere is 90 times thicker than Earth, which is equivalent to being a kilometer beneath the ocean on Earth.
In the beginning, colonizing the surface of Venus defies our ability. How do you survive and stay cool in a thick poisonous atmosphere, hot enough to melt lead? You get above it.
One of the most amazing qualities of Venus is that if you get into the high atmosphere, about 52.5 kilometers up, the air pressure and temperature are similar to Earth. Assuming you can get above the poisonous clouds of sulphuric acid, you could walk outside a floating colony in regular clothes, without a pressure suit. You’d need a source of breathable air, though.
Even better, breathable air is a lifting gas in the cloud tops of Venus. You could imagine a future colony, filled with breathable air, floating around Venus. Because the gravity on Venus is roughly the same as Earth, humans wouldn’t suffer any of the side effects of microgravity. In fact, it might be the only place in the entire Solar System other than Earth where we don’t need to account for low gravity.
Now the day on Venus is incredibly long, 243 earth days, so if you stay over the same place the whole time it would be light for four months then dark for four months. Not ideal for solar power on a first glance, but Venus turns so slowly that even at the equator you could stay ahead of the sunset at a fast walk.
So if you have floating colonies it would take very little effort to stay constantly on the light side or dark side or near the twilight zone of the terminator. You are essentially living inside a blimp, so it may as well be mobile. And on the day side it would only take a few solar panels and some propellers to stay ahead. And since it is so close to the Sun, there’s plenty of solar power. What could you do with it?
The atmosphere itself would probably serve as a source of raw materials. Carbon is the basis for all life on Earth. We’ll need it for food and building materials in space. Floating factories could process the thick atmosphere of Venus, to extract carbon, oxygen, and other elements.
Heat resistant robots could be lowered down to the surface to gather minerals and then retrieved before they’re cooked to death.
Venus does have a high gravity, so launching rockets up into space back out of Venus’ gravity well will be expensive.
Over longer periods of time, future colonists might construct large solar shades to shield themselves from the scorching heat, and eventually, even start cooling the planet itself.
The next planet from the Sun is Earth, the best planet in the Solar System. One of the biggest advantages of our colonization efforts will be to get heavy industry off our planet and into space. Why pollute our atmosphere and rivers when there’s so much more space… in space.
Over time, more and more of the resource gathering will happen off world, with orbital power generation, asteroid mining, and zero gravity manufacturing. Earth’s huge gravity well means that it’s best to bring materials down to Earth, not carry them up to space.
However, the normal gravity, atmosphere and established industry of Earth will allow us to manufacture the lighter high tech goods that the rest of the Solar System will need for their own colonization efforts.
But we haven’t completely colonized Earth itself. Although we’ve spread across the land, we know very little about the deep ocean. Future colonies under the oceans will help us learn more about self-sufficient colonies, in extreme environments. The oceans on Earth will be similar to the oceans on Europa or Enceladus, and the lessons we learn here will teach us to live out there.
As we return to space, we’ll colonize the region around our planet. We’ll construct bigger orbital colonies in Low Earth Orbit, building on our lessons from the International Space Station.
One of the biggest steps we need to take, is understanding how to overcome the debilitating effects of microgravity: the softened bones, weakened muscles and more. We need to perfect techniques for generating artificial gravity where there is none.
The best technique we have is rotating spacecraft to generate artificial gravity. Just like we saw in 2001, and The Martian, by rotating all or a portion of a spacecraft, you can generated an outward centrifugal force that mimics the acceleration of gravity. The larger the radius of the space station, the more comfortable and natural the rotation feels.
Low Earth Orbit also keeps a space station within the Earth’s protective magnetosphere, limiting the amount of harmful radiation that future space colonists will experience.
Other orbits are useful too, including geostationary orbit, which is about 36,000 kilometers above the surface of the Earth. Here spacecraft orbit the Earth at exactly the same rate as the rotation of Earth, which means that stations appear in fixed positions above our planet, useful for communication.
Geostationary orbit is higher up in Earth’s gravity well, which means these stations will serve a low-velocity jumping off points to reach other places in the Solar System. They’re also outside the Earth’s atmospheric drag, and don’t require any orbital boosting to keep them in place.
By perfecting orbital colonies around Earth, we’ll develop technologies for surviving in deep space, anywhere in the Solar System. The same general technology will work anywhere, whether we’re in orbit around the Moon, or out past Pluto.
When the technology is advanced enough, we might learn to build space elevators to carry material and up down from Earth’s gravity well. We could also build launch loops, electromagnetic railguns that launch material into space. These launch systems would also be able to loft supplies into transfer trajectories from world to world throughout the Solar System.
Earth orbit, close to the homeworld gives us the perfect place to develop and perfect the technologies we need to become a true spacefaring civilization. Not only that, but we’ve got the Moon.
The Moon, of course, is the Earth’s only natural satellite, which orbits us at an average distance of about 400,000 kilometers. Almost ten times further than geostationary orbit.
The Moon takes a surprising amount of velocity to reach from Low Earth Orbit. It’s close, but expensive to reach, thrust speaking.
But that fact that it’s close makes the Moon an ideal place to colonize. It’s close to Earth, but it’s not Earth. It’s airless, bathed in harmful radiation and has very low gravity. It’s the place that humanity will learn to survive in the harsh environment of space.
But it still does have some resources we can exploit. The lunar regolith, the pulverized rocky surface of the Moon, can be used as concrete to make structures. Spacecraft have identified large deposits of water at the Moon’s poles, in its permanently shadowed craters. As with Mercury, these would make ideal locations for colonies.
Our spacecraft have also captured images of openings to underground lava tubes on the surface of the Moon. Some of these could be gigantic, even kilometers high. You could fit massive cities inside some of these lava tubes, with room to spare.
Helium-3 from the Sun rains down on the surface of the Moon, deposited by the Sun’s solar wind, which could be mined from the surface and provide a source of fuel for lunar fusion reactors. This abundance of helium could be exported to other places in the Solar System.
The far side of the Moon is permanently shadowed from Earth-based radio signals, and would make an ideal location for a giant radio observatory. Telescopes of massive size could be built in the much lower lunar gravity.
We talked briefly about an Earth-based space elevator, but an elevator on the Moon makes even more sense. With the lower gravity, you can lift material off the surface and into lunar orbit using cables made of materials we can manufacture today, such as Zylon or Kevlar.
One of the greatest threats on the Moon is the dusty regolith itself. Without any kind of weathering on the surface, these dust particles are razor sharp, and they get into everything. Lunar colonists will need very strict protocols to keep the lunar dust out of their machinery, and especially out of their lungs and eyes, otherwise it could cause permanent damage.
Although the vast majority of asteroids in the Solar System are located in the main asteroid belt, there are still many asteroids orbiting closer to Earth. These are known as the Near Earth Asteroids, and they’ve been the cause of many of Earth’s great extinction events.
These asteroids are dangerous to our planet, but they’re also an incredible resource, located close to our homeworld.
The amount of velocity it takes to get to some of these asteroids is very low, which means travel to and from these asteroids takes little energy. Their low gravity means that extracting resources from their surface won’t take a tremendous amount of energy.
And once the orbits of these asteroids are fully understood, future colonists will be able to change the orbits using thrusters. In fact, the same system they use to launch minerals off the surface would also push the asteroids into safer orbits.
These asteroids could be hollowed out, and set rotating to provide artificial gravity. Then they could be slowly moved into safe, useful orbits, to act as space stations, resupply points, and permanent colonies.
There are also gravitationally stable points at the Sun-Earth L4 and L5 Lagrange Points. These asteroid colonies could be parked there, giving us more locations to live in the Solar System.
The future of humanity will include the colonization of Mars, the fourth planet from the Sun. On the surface, Mars has a lot going for it. A day on Mars is only a little longer than a day on Earth. It receives sunlight, unfiltered through the thin Martian atmosphere. There are deposits of water ice at the poles, and under the surface across the planet.
Martian ice will be precious, harvested from the planet and used for breathable air, rocket fuel and water for the colonists to drink and grow their food. The Martian regolith can be used to grow food. It does have have toxic perchlorates in it, but that can just be washed out.
The lower gravity on Mars makes it another ideal place for a space elevator, ferrying goods up and down from the surface of the planet.
Unlike the Moon, Mars has a weathered surface. Although the planet’s red dust will get everywhere, it won’t be toxic and dangerous as it is on the Moon.
Like the Moon, Mars has lava tubes, and these could be used as pre-dug colony sites, where human Martians can live underground, protected from the hostile environment.
Mars has two big problems that must be overcome. First, the gravity on Mars is only a third that of Earth’s, and we don’t know the long term impact of this on the human body. It might be that humans just can’t mature properly in the womb in low gravity.
Researchers have proposed that Mars colonists might need to spend large parts of their day on rotating centrifuges, to simulate Earth gravity. Or maybe humans will only be allowed to spend a few years on the surface of Mars before they have to return to a high gravity environment.
The second big challenge is the radiation from the Sun and interstellar cosmic rays. Without a protective magnetosphere, Martian colonists will be vulnerable to a much higher dose of radiation. But then, this is the same challenge that colonists will face anywhere in the entire Solar System.
That radiation will cause an increased risk of cancer, and could cause mental health issues, with dementia-like symptoms. The best solution for dealing with radiation is to block it with rock, soil or water. And Martian colonists, like all Solar System colonists will need to spend much of their lives underground or in tunnels carved out of rock.
In addition to Mars itself, the Red Planet has two small moons, Phobos and Deimos. These will serve as ideal places for small colonies. They’ll have the same low gravity as asteroid colonies, but they’ll be just above the gravity well of Mars. Ferries will travel to and from the Martian moons, delivering fresh supplies and sending Martian goods out to the rest of the Solar System.
We’re not certain yet, but there are good indicators these moons might have ice inside them, if so that is an excellent source of fuel and could make initial trips to Mars much easier by allowing us to send a first expedition to those moons, who then begin producing fuel to be used to land on Mars and to leave Mars and return home.
According to Elon Musk, if a Martian colony can reach a million inhabitants, it’ll be self-sufficient from Earth or any other world. At that point, we would have a true, Solar System civilization.
Now, continue on to the other half of this article, written by Isaac Arthur, where he talks about what it will take to colonize the outer Solar System. Where water ice is plentiful but solar power is feeble. Where travel times and energy require new technologies and techniques to survive and thrive.
Do you remember science classes from way back when? All those laws and rules made it seem like everything was logical and well behaved. Then perhaps with television and movies being a big part of your life you began to wonder whether what you saw was real and unreal. Those things on the big and small screens didn’t seem nearly as well behaved. For instance, can people hear sounds in space? Or, can travelers quickly and easily go from one star to another? If you want to get yourself back on solid footing, get a hold of the book “Hollyweird Science – From Quantum Quirks to the Multiverse” by Kevin Grazier and Stephen Cass. With it, you can sift through a lot of tropes and conceits and glean some wonderful insights of both modern science and modern cinema.
Yes, tropes and conceits are terms from the world of cinema and not of physics. Think of these terms as ‘untruths’ for entertainment that writers use to capture and hold the attention of the audience. As this book describes, writers conjure up these exigencies to meet their demands. Their main demand is to prepare a story that fits into a very limited timeframe and into a very limited budget.
And much of the first part of this book takes the reader on a journey of past and present cinema that involves detailed science. This part of the book substantiates the claim that science in the Hollywood world of cinema is weird, whether it is Superman’s kryptonite, Star Trek’s dilithium crystals or Godzilla’s shear bulk. So how does this book go about proving that the science is weird?
Ah, this is the part that you may either love or hate. The authors include science boxes at regular intervals throughout. These science boxes have the equations you may remember from your early science classes. And the equations include numbers or ratios that show how a trope or conceit is particularly untrue. That is, the authors return to all those laws and rules of science, such as the law of gravity, the formula for acceleration, and the standard chemical composition of ecosystems.
Nevertheless, most of these weird issues are ones that the audience has already accepted and even a science box won’t affect the shear enjoyment. For example, think of Torch, a human that can instantly become a flame even though there’s no fuel. While the authors do raise a general lament on the failure of cinema to faithfully follow science, they do provide some rationalization that the untruth or trope was necessary, whether to fit a timeframe or a budget. Perhaps most promising from this section of the book is that the authors indicate that the typical audience member has become much smarter. In consequence, writers put a lot more reality into their science and even the depiction of alien worlds.
Who knew that learning physics could be so much fun?
Overall, the first third of the book is a fairly light, simple read with not so many science boxes. At about a third of the way in, however, the book transitions from being a discussion of cinema entertainment, with particular attention to its science, and becomes a discussion of science with reference to cinema. Here the science boxes are more detailed and numerous. They assess the possibility of using material from the Earth to kick-start a failing Sun, as done in a movie. Or, the likelihood of the Earth’s Moon being kicked out of the solar system, also done. And there’s much detail on the holy grail of science cinema, the faster than light transportation, as happens in most science fiction cinema.
Reading through this part of the book may bring you right back to your science classes of yore and their laws and rules. That is, it will if your science classes included quantum mechanics, parallel universes and wormholes. Here in the book things get really weird as today’s science has yet to faithfully prescribe the laws. Thus, the authors introduce a whole field of science, add current investigations and then associate the science with somewhat related relevant films. Perhaps, when the science gets this challenging, then it’s a good thing that entertaining cinema can come along and at least introduce the ideas to the general public.
With all the attention that the authors give to the science in this book, the reader will quickly appreciate that the book is not just a simple list of cinema bloopers. Rather, the book’s details provide enough depth of knowledge to allow the reader to hold their own at lunch time conversations when the topic swings around to the science in the latest show or movie. Perhaps it may induce the reader to do a bit more exploring and learning, especially as many current films feature a website that defines the science, the tropes and the conceits. However, cinema is for entertainment and the authors must realize the same holds for their book. So as much as this book has lots of hard science, the authors still keep the book entertaining.
And entertainment is mostly what we want, whether from cinema or books. So even if explosions in space come with a loud bang on the sound track or people fly without space suits up and around the Moon, we the audience are content if we are entertained and we haven’t hit the ‘Oh please!’ moment. If you want to know more about this moment, take a look at the book “Hollyweird Science – From Quantum Quirks to the Multiverse” by Kevin Grazier and Stephen Cass. From it, you can make up your own mind on just what you’re ready to accept as entertaining and what is just too much expectation by the storyteller.
Elsewhen is a story about star-crossed young lovers, a love story for science fiction fans. Conceived when author/actor Gary Bullock was working at a radio astronomy site, Elsewhen follows the path of Elijah (‘Lije’) and Laura Bess, two child prodigies who fall head-over-heels in love before tragedy strikes and tears them apart. But for Lije and Laura, it seems that True Love might be able to thwart even fate…
Concepts from the more poetic end of theoretical physics are liberally peppered among the pages—musings on the directionality of time, for example—but this is by no means ‘hard’ science fiction. Scientific complexity level is about equivalent to the first Thor movie, so if you don’t know your bosons from your fermions, don’t despair.
Blending physics with a love story might seem like a difficult line to walk, but Bullock does a respectable job with his 118-page novella. Bullock’s career appears to have wended from screen writing to writing novels, and indeed, Elsewhen reads kind of like a screenplay—which I mean as both praise and as a critique.
On the side of praise, there is a good kind of inertia to the book. The plotline barrels along at a cracking pace, and given the length of the novella, it’s quite possible that you might read this cover to cover in a single night. But on the flip side, I wanted this novel to be longer. Several concepts and (particularly) characters were only loosely sketched out before the plotline whisked away to the next development.
The brevity led to my two main problems with the book. First of all, some key characters are bald rehashes of literary tropes. Some character development earlier in the novel could have, for example, fleshed out the villains in the story to make them more human and relatable.
Second, I craved more depth from the story. The many fantastical elements of the storyline open up the main characters in discussion of various concepts of philosophy and metaphysics, and I felt that more exposition here would have led to a more interesting read (and probably would have also helped with the character development problem). However, this may be less a critique of Elsewhen, and more a problem of my expectations going into this novel.
These issues aside, Elsewhen is a fun book with a clever premise. For the price of a cup of coffee, it’s easy enough to recommend for a light read.
When “nothing in our solar system can help us,” we need to “confront the reality of interstellar travel.” So says the new full trailer from the upcoming film “Interstellar.”
In a word: WOW. And at nearly 7 million views so far on YouTube, this trailer is generating a lot of interest and anticipation. Even before the release of this trailer over the weekend, “Interstellar” has been one of the most anticipated movies of the year, especially for space fans. Details about the plot have been kept fairly secret so far, but here’s what the film’s website says: Continue reading “ICYMI: Full Trailer for “Interstellar””
Actors for a new movie coming out in October 2013 received tips about life in space from NASA astronaut Cady Coleman. “Gravity” is the story of two astronauts (played by George Clooney and Sandra Bullock) whose shuttle is destroyed by a run-in with space junk during an EVA, stranding them both in orbit and struggling for survival.
While developing her role, Bullock gave Coleman a call while she was aboard the space station. At the time, the actress asked Coleman to elaborate on what it’s like living and moving about in microgravity. “I told her that I had long hair, and if you pulled a hair out and pushed it against something, you could move yourself across the space station,” said Coleman. “That’s how little force it takes.”
You can see more of their discussion below, as well as the heart-pounding trailer for the movie:
NASA says that although this dire scenario makes for gripping Hollywood entertainment, NASA actively works to protect its astronauts and vehicles from the dangers portrayed in the movie. From protective shielding and meticulous and methodical training on the ground and in space covering everything from spacewalking to fires or decompression inside the space station, NASA’s ground crews and astronauts are as prepared as they can be for potential anomaly, no matter how remote they may be.
Have you always wanted to know how a Xurian Scout Fighter compares to a Valor-class Type-2 Valkyrie Attack Fighter? Wonder no more. DeviantARTist Dirk Loechel has created what is likely the most accurate and complete size comparison chart of almost every science fiction starship, from famous Star Trek and Stars Wars battle cruisers to ships from games like Halo to vessels from obscure sci-fi books. This new chart is an updated version of one Loechel made earlier. It looks like Loechel is taking suggestions for doing another update if you find he’s missed some.
Click on the image above to have access to the large original version on DeviantART, and enjoy the diversion.
I love science fiction films and I especially love it when the “science” part leans closer to fact than fiction. (Yes, I’m looking at you, Europa Report.) Now I’ve never seen an actual catastrophe in orbit (and I hope I never do) but I have to assume it’d look a whole lot like what’s happening in the upcoming film “Gravity,” opening in U.S. theaters on October 4. This full official trailer was released today.
A disaster film sure becomes a whole lot more interesting when everything is moving 18,000 miles an hour and there’s no up or down. And, of course, space. (!!!)
If you’ve ever been involved in one, you know that even a minor vehicle accident is a confusing and scary event. Trying to desperately regain control of your own movement as you’re suddenly subjected to forces beyond your control is stressful and terrifying… now imagine it happening at 17,500 mph and 230 miles up and you’ve got an idea of what the upcoming film “Gravity” is about.
Still can’t quite picture it? Check out the latest trailer below:
Directed and written by Alfonso Cuarón and co-written with his son Jonas, “Gravity” is the story of two astronauts (played by George Clooney and Sandra Bullock) whose shuttle is destroyed by a run-in with space junk during an EVA, stranding them both in orbit.
If that wasn’t bad enough, their oxygen is running out and they have lost communication with the ground. Cast adrift in orbit, they have to figure out how to survive and get back home.
It’s like “Open Water” in space. Without the sharks. (Let’s hope things turn out better for them!)
I enjoy sci-fi and I especially enjoy when they try to get the “sci” part right. How do things move in microgravity? (Hint: really fast.) What happens when stuff smashes together? What would happen to the human body in that situation? And, most importantly for any movie, how do the people involved handle the experience?
Above all, “Gravity” is still a movie so it has to take us on a two-hour, candy-munching, soda-slurping ride. Based on this latest trailer, I’m confident that they’ve done their homework on the mechanics of movement in orbit… now let’s see if Cuarón (Children of Men, Y Tu Mamá También, Harry Potter and the Prisoner of Azkaban) has once again worked his storytelling magic to bring the characters to free-falling life.