Smithsonian.com

Who’s in the suit? Increasingly, it’s our digital selves. Photo from NASA/STS-104

Ever since the collective “YOU” became Time Magazine’s Person of the Year in 2006, campaigns to get our attention have increasingly sought out our digital selves. You can name a Budweiser Clydesdale. You can pick Lays’ new potato chip flavor. And it’s not just retail that wants your online opinions: You can vote for who will win photography contests. You can play the futures market on who will win elected offices. And with enough signatures, you can get the White House to read your petitions.

Many science endeavors rely on such crowdsourcing. With a simple app, you can let researchers know the exact date that your lilacs or dogwoods bloom, helping them to track how seasonal cycles are shifting as a result of climate change. You can join the search for ever-larger prime numbers. You can even help scientists scan radio waves in space to search for intelligent life outside of Earth. These more traditional crowdsourcing efforts allow users to brainstorm ideas and process data from computers at home.

But now, a few projects are allowing us to put our virtual selves beyond Earth’s atmosphere through recently launched space missions. Who said that rovers, space probes, a handful of astronauts and pigs were the only ones in space? No longer are we just bystanders watching spacecraft launch and cooing over images returned of other planets and stars. Now, we can direct cameras, help run experiments, even send our avatars–of sorts–to inhabit nearby planetary bodies or return to us in a time capsule.

Here are a few examples:

Asteroid Chimney Rock: On April 10 (tomorrow), the Japan Aerospace Exploration Agency will open up a campaign that allows visitors to their site the opportunity of sending their names and brief messages to the near-Earth asteroid (162173) 1999 JU₃.  Called the “Let’s meet with Le Petit Prince! Million Campaign 2,” the effort aims to get people’s names onto the Hayabusa2 mission, which will likely launch in 2014 to study the asteroid. When Hayabusa 2 lands on the asteroid, the names submitted–embedded in a plaque of sorts on the spacecraft–will stand as a testament to the idea that humans (or at least their robotic representatives) were there.

The Hayabusa2 mission, scheduled for launch in 2014, will attempt to return an asteroid sample back to Earth in 2020. Artist’s rendition by Akihiro Ikeshita/JAXA

The campaign is reminiscent of how NASA got more than 1.2 million people to submit their names and signatures, which were then etched on two dime-sized microchips and affixed to the Mars Curiosity rover. Sure, it’s a bit gimmicky–what useful function is brought by having people’s names out in space? But the idea of “tagging” a planet or an asteroid–preserving a bit of yourself on what will over decades become space junk–has powerful pull. It is why Chimney Rock, with its etchings from early explorers and pioneers, is the historical marker it is today, and why gladiators scored their names into the Colosseum before they fought to the death. For mission leaders hoping to get the public enthusiastic about space, nothing’s more exciting than a bit of digital graffiti.

Interplanetary time capsules: A key goal of Hayabusa2 is to return return a sample from the asteroid in 2020. Mission creators saw this as a perfect way to get the public to fill a time capsule. Those seeking to participate are encouraged to send to mission coordinators their thoughts and dreams for the future along with their hopes and expectations for recovery from natural disasters, the latter likely a way to get people to express their feelings on the 2011 Tohoku earthquake and tsunami that devastated Japan’s east coast. Names, messages, and illustrations will loaded onto a microchip that will not only touch down on the asteroid’s surface, but will also be a part of the probe sent back to Earth with asteroid dust.

But why stop at a mere 6-year time capsule? The European Space Agency, UNESCO, and other partners are blending crowd sourcing with space technology to create the KEO mission–so named because the letters represent common sounds across all of Earth’s languages–which will bundle thoughts and images of anyone who seeks to participate and will launch this bundle in a probe that will only return to Earth in 50,000 years.

Project operators write on KEO’s website: “Each one of us have 4 uncensored pages at our disposal: an identical space of equality and freedom of expression where we can voice our aspirations and our revolts, where we can reveal our deepest fears and our strongest beliefs, where we can relate our lives to our faraway great grandchildren, thus allowing them to witness our times.” That’s 4 pages for every person who chooses to participate.

On board will be photographs detailing Earth’s cultural richness, human blood encased in a diamond, and a durable DVD of humanity’s crowdsourced thoughts. The idea is to launch the time capsule from an Ariane 5 rocket into an orbit more than 2,000 kilometers above Earth, hopefully sometime in 2014. “50,000 years ago, Man created art thus showing his capacity for symbolic abstraction.” the website notes. And in another 50,000 years, “Will Earth still give life? Will human beings still be recognizable as such?”Another logical question: Will whatever’s left on Earth know what’s coming back to them and will be able to retrieve it?

Hayabusa2 and KEO will join capsules already launched into space on Pioneer 10 and 11 and Voyager 1 and 2. But the contents of these earlier capsules were picked by a handful of people; here, we get to choose what represents us in space, and will get to reflect (in theory) on the thoughts bound in time upon their return.

You, the mission controller and scientist: Short of going to Mars yourself, you can do the next best thing–tell an instrument currently observing Mars where to look. On NASA’s Mars Reconnaissance Orbiter is the University of Arizona’s High Resolution Imaging Science Experiment (HiRISE), a camera designed to image Mars in great detail. Dubbed “the people’s camera,” HiRISE allows you–yes, you!– to pick its next targets by filling out a form specifying your “HiWishes.”

A recently launched nanosatellite is allowing the crowdsourced winners of a crowdsourced screaming contest the chance to test whether screams can be heard in space. Launched in February, the nanosatellite’s smartphone-powered brain will broadcast the screams–no word yet on results. But you may find just listening to the yelling therapeutic! This guy’s roar got the most votes:

Mars, photo via Pixabay

Roughly 3.5 billion years ago, Mars began to shift from a wetter, warmer climate to the dry and cold planet we see today. This period of geologic change, known as the Hesperian age, was a turbulent time. The red planet saw widespread volcanic eruptions and catastrophic flooding as melted ice rushed into wide craters, forming lakes. These natural disasters carved a network of basins into its surface called outflow channels, eroding the terrain and reshaping the landscape of the planet. The exact end of this geologic period in Mars’ history is unknown, but scientists give a rough estimate of 3 billion years ago.

Later, many of these outflow channels became covered with lava, burying evidence of Mars’ geologic history. But now, a new map of the planet’s subsurface shows for the first time what one of these buried channels looks like in three dimensions. The findings, published today in the journal Science, reconstruct the Marte Vallis, the largest of the youngest channels on Mars. Marte Vallis is located in the Elysium Planitia region, an expanse of plains along the equator and the youngest volcanic region on the planet.

To create the 3D map,  the researchers used data from Shallow Radar, a device that probes for liquid or frozen water underneath Mars’ crust. Known as SHARAD, the technology is on board NASA’s Mars Reconnaissance Orbiter spacecraft, which is currently circling the planet to study its climate. SHARAD’s orbital sounding radar works in much the same way as medical imaging scans. It sends signals to the surface, some of which automatically bounce back to the spacecraft. The signals that don’t readily bounce back can penetrate Mars’ crust and register buried structures before returning to the device. The data appears in two-dimensional cross sections, which are then pieced together to build the 3D representation. In this manner, a deeply grooved set of channels was revealed.

3D visualization of the buried Marte Vallis channels underneath the surface of Mars. Image via Smithsonian Institution/NASA/JPL-Caltech/Sapienza University of Rome/MOLA Team/USGS

The system of channels, which is somewhere between 10 million to half a billion years old, spans 60 miles in width and stretches for more than 600 miles in length. From what can be seen of Marte Vallis from the surface, the channels are similar in structure to more ancient channel systems traced to the Hesperian, but the lava that had obscured many of their features made it difficult for researchers to make accurate estimates about its depth.

The new data reveals that the scale of erosion for Marte Vallis had indeed been underestimated: the 25-mile-wide main channel is at least twice as deep than earlier approximations indicated. The map shows multiple perched channels which feed into the deeper and wider main channel. These channels once lay along a series of four islands, which floods eroded into teardrop-shaped hills.

The researchers found that the geometry of the features are similar to those of the planet’s oldest channels, which are less obscured by lava, making them easier to study. This also suggests that the Marte Vallis could have been carved entirely by water, says lead study author Gareth Morgan, a geologist at the National Air and Space Museum’s Center for Earth and Planetary Studies. In fact, most Mars scientists accept that outflow channels on Mars were carved by water. Lava also carves out tunnels through thermal erosion heating up the terrain, but Morgan says that this process is implausible for the scale of erosion at the Marte Valle channels. The speed of rushing water is also more efficient at erosion that the flow of lava, which can get stuck on rock, Morgan says. In addition, lava creates tunnels that aren’t as wide—typically only several miles across—so collapsed tunnels couldn’t account for the broad size of the channels.

Using the map, researchers were also able to pinpoint the source of the floodwater: a now buried portion of the Cerberus Fossae fracture, a series of fissures in the planet’s surface. The researchers posit that water from a reservoir deep below Mars’ surface was released by nearby tectonic or volcanic activity, and it worked quickly to form the channels. These channels would have been a short-lived affair,” Morgan says. “The fracture would have connected this groundwater to the surface. After a short duration of weeks or months, the source would have been exhausted.”

But why was water in that reservoir during a time when the rest of Mars is believed to have been dry? Water, the authors believe, could have collected in aquifers below the surface during the Hesperian. This water hypothetically could have remained stable in liquid form long after the Hesperian ended. Morgan feels that the 3D map could provide more evidence to support this hypothesis, showing that Mars was wet place in the more recent—as opposed to far ancient—past.

More than 20 similar outflow channels are spread out on the surface of the planet, extending hundreds of miles in length. The most prominent are located in the Chryse Planitia, a circular volcanic plain in the northern hemisphere of Mars. The largest, the Kasei Valles, runs for 1,500 miles along the plain.

Cataclysmic floods like the ones that shaped Mars’ channels aren’t unique to the red planet. Approximately 14,000 years ago, the largest known flood on Earth sprang from Lake Missoula, a prehistoric body of water that existed at the end of the last Ice Age in present-day Montana. The waters eroded part of the landscape of Washington state, forming the Channeled Scablands, a terrain that resembles Martian outflow channels. Marte Vallis’ main channel is estimated to be between 226 and 371 feet deep, a depth that’s comparable to the Channeled Scablands.

So if Mars’ expansive outflow channels were formed by gushing water, the question remains: Where did it all ago?

Some of it vaporized, drifted to the planet’s poles, and precipitated as ice on polar caps, Morgan says. Similar to the ones we have on Earth, the polar ends on the Red Planet are covered in miles-thick layers of ice. The water also could have pooled into shallow areas below the surface, where it also froze—in 2008, NASA’s Phoenix mission confirmed that ice exists in the porous soil that makes up much of the planet’s surface.

Another possibility, Morgan says, is that the ancient water again escaped deep underground, forming a large reservoir that awaits its chance to flood again.

A meteorite, newly discovered in Morocco, contains ten times as much water as many Martian meteorite discovered previously. Image via Agee et. al.

Last year, noted meteorite collector Jay Piatek traveled to Morocco and bought a single stone, less than a pound in weight, that had been discovered in the country some time earlier. When he passed it on to researchers at the University of New Mexico to perform a mineral analysis, they found something unexpected.

The meteor seemed to have originated on Mars, but the rock’s composition didn’t exactly match any of the well-studied meteorites from there found previously. When the researchers compared it to data from soil and rock samples obtained by Curiosity and other recent Martian rovers, though, they realized that rather than originating in the planet’s mantle, as the others had, it appeared to have come from the Martian crust.

Most intriguingly, when they analyzed the basaltic breccia rock even more closely, they discovered it contained a large quantity of water molecules locked in its crystalline structure. While previous studies of Martian meteorites have suggested the presence of water on the red planet, this sample’s analysis, published today in Science, revealed that it contained 10 times more water than any Martian meteorite examined before.

The discovery of the water molecules in the rock at concentrations of 6000 parts per million could indicate the presence of liquid water sometime during Mars’ history. “The high water content could mean there was an interaction of the rocks with surface water either from volcanic magma, or from fluids from impacting comets during that time,” study co-author Andrew Steele of the Carnegie Institute said in a statement.

Apart from the presence of water, the researchers say that information they’ve gleaned over the course of a year-long analysis of the meteor—the first ever linked to the Martian crust—could significantly impact our understanding of the planet’s geology as a whole. The meteorite is primarily composed of chunks of basalt cemented together, indicating that it formed from rapidly cooling lava, likely on the planet’s crust. While we’ve found meteorites from the Moon that match this composition, we haven’t seen anything like it from Mars previously.

Already, the researchers determined that the specimen is roughly 2.1 billion years-old, formed during Mars’ Amazonian epoch, a time period from which we had no previous rock samples. “It is the richest Martian meteorite geochemically,” Steele said. “Further analyses are bound to unleash more surprises.”

The levels of radiation astronauts experience over the course of an extended mission in deep space could lead to dementia and Alzheimer’s. Image via NASA.

NASA has big plans for manned travel in deep space. Although missions haven’t been officially announced yet, experts speculate that the agency plans to establish a space station on the far side of the moon sometime in the next decade, a stepping stone towards landing on an asteroid in 2025 and potentially trying to reach Mars sometime around 2033.

Getting to Mars, though, would require astronauts to endure a round-trip (or possibly one-way) journey that could be as long as three years—which could be particularly worrisome given the results of a study on the health effects of cosmic radiation published today in PLOS ONE. Although we’ve known for some time that the radiation experienced by space travelers could pose problems over the long term, this new study is the first to establish a link with an increased chance of Alzheimer’s disease and dementia.

The researchers, a group from NASA and the University of Rochester, came to the finding by testing a specific type of cosmic radiation—high-mass, high-charged (HZE) iron particles—on mice. This kind of radiation is of particular concern, because its high speed (a result of the force of the exploding stars it’s originally expelled from, light-years away) and large mass mean that it’s tricky to protect against.

Here on Earth, we’re largely protected from it and other types of radiation by our planet’s atmosphere and magnetic field, but even a short time in deep space means much higher levels of exposure, and we haven’t yet figured out how to construct a shield that effectively blocks it. ”Because iron particles pack a bigger wallop it is extremely difficult from an engineering perspective to effectively shield against them,” M. Kerry O’Banion, the paper’s senior author, said in a statement. “One would have to essentially wrap a spacecraft in a six-foot block of lead or concrete.”

After producing radioactive particles that generate this type of radiation using a particle accelerator at the Brookhaven National Laboratory on Long Island, the researchers exposed the mice to varying doses of the radiation, including levels comprable to what astronauts would experience on a mission to Mars. The breed of mice they used has been the subject of numerous studies on dementia and Alzheimer’s, so scientists have a relatively good understanding of how rapidly the disease and related symptoms develop over time.

But when the researchers put the mice through a series of behavioral tests—seeing if they were capable of remembering objects or specific locations—those that had been exposed to greater levels of radiation were far more likely to fail, demonstrating signs of neurological impairment far more early in life than is typical in the breed. Additionally, autopsies of these mice revealed that their brains contained higher levels of beta amyloid, the “plaque” considered a hallmark of Alzheimer’s disease.

This result doesn’t mean we have to abandon dreams of deep space travel—or even that this kind of radiation definitively leads to accelerated neurological degeneration—but it does show that cosmic radiation is going to be a graver concern the longer space missions get. Ingenious engineering has addressed many of the difficulties of space flight, but this remains a problem to be solved.

“These findings clearly suggest that exposure to radiation in space has the potential to accelerate the development of Alzheimer’s disease,” O’Banion said. “This is yet another factor that NASA, which is clearly concerned about the health risks to its astronauts, will need to take into account as it plans future missions.”

A graphic data readout of the a collision of two protons, briefly producing a Higgs Boson, from the Large Hadron Collider. Image via CERN

The year 2012 was a major one for science. We saw scientists develop a new type of drug to combat HIV, figure out how to store digital data in DNA—fitting an astonishing 700 terabytes of information into a single gram of it—and even invent a coating for the inside of condiment bottles that could eliminate our stuck-ketchup-headaches once and for all (though, admittedly, this one is a little less groundbreaking than the others). Yet a few milestones in particular—discoveries, technological feats, realizations, and inventions—stand out:

1. The Higgs Boson: The landmark discovery by the European Organisation for Nuclear Research (CERN) of the once-mythical particle might be the most significant scientific discovery of our lifetimes, but it’s also one of the most surprising. Stephen Hawking, the Einstein of our time, famously bet Michigan physicist Gordon Kane $100 that it would never be found.

In an interview with The Atlantic, physicist Lawrence Krauss explained why so many experts had agreed with Hawking, arguing that the existence of the Higgs—a particle (and associated field) that makes certain types of elementary particles behave as though they had mass—was just too convenient, as it was originally posited simply to explain away an apparent difficulty in an otherwise appealing theory in theoretical physics.

The theory seeks to unite all physical forces under the same set of rules. But how can electromagnetic forces–governed by massless photons–fit under the same theoretical umbrella as the weak force, which is governed by bosons with discernible mass that control radioactive decay? Efforts to answer this conundrum gave birth to  the Higgs boson. Krauss noted,”It seemed too easy…It seemed to me that introducing an invisible field to explain stuff is more like religion than science…Great, I invented invisible hobgoblins to make things right.”

Incredibly, in this case, it turned out the hobgoblins were real.

An artist’s rendering of the theorized Earth-like planet, potentially capable of containing liquid water. Image via University of Hertfordshire/J. Pinfield

2. Earth-Like Planets: 2012 featured a ton of exoplanet discoveries, but the sighting of HD 40307g was without a doubt the most unexpected and exciting.  The planet, bigger than earth but not so large as to be a gas giant, seems to orbit in its sun’s “goldilocks zone” (not too hot and not too cold), making it potentially capable of hosting liquid water, considered a prerequisite for life as we know it.

Even better, it’s just 42 light-years away: distant by human standards, but fairly close by compared many of the astronomical objects, making future projects to observe the planet much more feasible.

A composite image of self-portraits taken by Curiosity on Mars. Image via NASA/JPL-Caltech/MSSS

3. Curiosity Reaches Mars: Okay, the mission itself wasn’t too surprising—it’s been in the works since 2004—but what was so astonishing was the sudden surge of public interest in the rover and in space exploration as a whole. For decades following the manned Apollo missions of the 1960s and 70s, general enthusiasm for space science had slowly ebbed. After Curiosity’s successful landing, though, it surged. Among other things, video of NASA engineers celebrating the feat went viral and the official Curiosity twitter account garnered some 1.2 million followers.

People are so interested in Curiosity‘s exploits, in fact, that even an engineer’s throwaway line about “a discovery for the history books” pumped up expectations so much that we were bound to be disappointed by the actual finding: that early Martian soil samples seem to be representative of what we know of the planet as a whole, and that its chemistry is complex enough to have potentially once supported life. Bigger news might come over the next few years, but as project scientist John Grotzinger said, “Curiosity’s middle name is patience.”

For many Americans, Superstorm Sandy drove home the idea that climate change is real. Image via NASA

4. Climate Change Is Even Worse Than We Thought: After decades of warnings from scientists that our greenhouse gas emissions will soon wreak havoc with the climate, we’re now starting to see the consequences—and they sure aren’t pretty. As a whole, experts are saying that the even the most frightening climate scenarios have proved to be too conservative in their analysis of how rising carbon dioxide concentrations will alter precipitation patterns, drive ocean acidification, lead to more powerful storms and, in general, make most parts of the planet grow warmer.

One silver lining might be that the public is now starting to acknowledge climate change as a present-day problem, rather than a hypothetical trend that could take effect in the future. Sadly, this has come only after record-breaking heat waves, droughts and the tragic impacts of Hurricane Sandy. Although the most recent international climate talks in Doha accomplished little, there are hopes that this shift in opinion could lead to a long-awaited change in policy sometime soon.

A digital rendering at the atomic level of a new type of water desalinization method developed at MIT, which uses a one-atom-thick sheet of graphene (blue) to filter impurities (green and purple ) from water molecules (red and white). Image via David Cohen-Tanugi

5. A New Way to Desalinate Seawater: With world populations expected to keep growing and potable water projected to grow more scarce over the coming century, a practical and cheap means of desalinating sea water is one of materials science’s holy grails. In July, MIT researchers announced the development of a new method of desalinization using one-atom-thick sheets of graphene, a pure carbon substance. Their method could be far cheaper and less energy-intensive than existing systems—potentially providing a way to solve many of the world’s water problems once and for all.