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A ‘Blue Hole’ To The Northern Lights

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A little-known meteorological phenomenon makes a tiny village in Arctic Sweden one of the best places on Earth to consistently see the Aurora Borealis.

“I’m not so sure we’ll see them,” said my videographer colleague Erik Jaråker, as he looked at the fog all around. I was driving us up the single-lane highway towards one of Sweden’s northernmost villages, Abisko, located 250km north of the Arctic Circle. We were caught in the middle of a snowstorm with zero visibility, and all around us, the mountains of Abisko National Park had become a sea of white.

We were heading up to photograph the elusive Northern Lights – nature’s spectacular light show, also known as the Aurora Borealis. The displays occur when explosions on the sun’s surface, called solar flares, collide with gases in the Earth’s atmosphere to create shimmering bands of red, green and purple. To witness this Aurora activity, we needed frigid, clear, cloudless skies, not the winter storm we were currently slogging through.

“Trust me,” I assured him confidently. “We’ll see them.”

I’d been here before under similar storm conditions, and I’d quickly learned that Abisko is home to a “blue hole“, a patch of sky that extends 10 to 20 sq km over the village, Lake Torneträsk and Abisko National Park and that remains clear regardless of surrounding weather patterns. This phenomenon makes Abisko one of the best places in the world to consistently witness the Aurora Borealis.

“Abisko, and northern Sweden, is indeed an ideal place to watch it,” said Erik Kjellström, professor in climatology at the Swedish Meteorological and Hydrological Institute, in an email. “This is due to the fact that it lies within the Auroral oval and it has a very long dark season – auroral observations are reported from mid-August to April – so there are plenty of Northern Lights around. The only thing needed is cloud-free conditions.” And, he added, Abisko has those in spades thanks to its position on the eastern side of the Scandinavian Mountain Range, which runs along the Norway-Sweden border.

Auroral observations are reported from mid-August to April in Abisko (Credit: Lola Akinmade Åkerström)

Håkan Grudd, research support coordinator and deputy station manager of the Abisko Scientific Research Station, explained further. “The dominating wind direction in this area is from the west, which means that moist air masses from the Atlantic have to rise to higher (colder) altitudes to pass over the Scandinavian Mountains. When this happens, clouds form and the air loses moisture through precipitation. In Abisko, on the leeside of the mountains, the air is now drier and sinks to lower altitudes – clouds disintegrate, hence the ‘blue hole’.”

So, it’s no wonder Abisko draws professional photographers like me and Erik, as well as travellers who want to check off their bucket-list item of seeing the Aurora Borealis.

That’s what drew photographer and entrepreneur Chad Blakley too. In 2008, as young newlyweds, he and his Swedish wife, Linnea, wanted a change from their corporate lives in the US. Combining his love for the outdoors with an opportunity to better understand Linnea’s culture, Blakely found work as part of the cleaning staff at the popular STF Abisko Turiststation hotel in the national park.

“I learned about the blue hole by experiencing it,” said Blakley, who, in the early days of his career, spent every night possible photographing the Northern Lights in the national park. “You could see a hole in the clouds directly over the village, while the sky on the horizon in all directions was often cloudy and full of snow.”

Abisko is home to a “blue hole” – a patch of sky that remains clear regardless of surrounding weather patterns (Credit: Lola Akinmade Åkerström)

In 2010, he and Linnea started an Aurora Borealis tourism company, Lights Over Lapland. And for those who couldn’t make it up to the remote region of Sweden, they set up a still-camera webcam that has been running for more than a decade and takes a picture every five minutes for an annual viewership of between 8 and 10 million. The company later added a live HD video camera, so that people could watch the lights in real time.

“We have seen Auroras consistently, nearly every single clear night, for more than 10 years,” Blakley shared. “And I am proud to say that the blue hole has helped Abisko gain a reputation for Aurora sightings.”

Blakley is in the process of installing the world’s first real-time, 8k, 360-degree Aurora webcam that will allow viewers to watch the Auroras live using a virtual reality (VR) camera and VR glasses next season.

Rosen: “Seeing how people express their feelings after seeing the lights makes me feel I have the best job in the world” (Credit: Lola Akinmade Åkerström)

The Northern Lights are Abisko’s main draw during the winter months, but the microclimate also provides other spectacular weather events too, such as very rare “moonbows”, also known as lunar rainbows and lunar halos, which occur when moonlight reflects and refracts through water droplets and ice crystals in the air surrounding the blue hole.

However, for Anette Niia and Ylva Sarri, who are members of Sweden’s indigenous Sámi community, Abisko is much more than its blue hole. There are about 70,000 Sámi living in the Arctic and subarctic parts of Norway, Sweden, Finland and the Kola Peninsula in Russia – a region collectively known as Sápmi. Both women have spent time in Abisko since childhood because it is also a reindeer herding area for their families. Niia explained that the area’s microclimate results in thinner snow during winter, which means spring arrives early here – and therefore food for reindeer and other animals. “The blue hole is something tourism companies talk about,” she said. “For us Sámi, Abisko is special for different reasons.”

Still, she and Sarri also have a connection to tourism here – their families’ ancestors were mountain guides for visitors starting in the early 1900s. Today, the women are the cofounders of Scandinavian Sami Photoadventures, which leads several outdoor experiences in Abisko, including Northern Lights tours. “We as guides know that when we arrive at Miellejohka stream, which flows down from Cuonjavaggi [valley], and go past it, you can go from a full snowstorm to clear skies within 100m,” said Niia. “That’s magic!”

And that was exactly what happened when Erik and I finally arrived in Abisko: dense snow clouds hovered over the mountains encircling us, but we saw clear blue skies directly overhead. 

On my first trip to Abisko several years ago, I remember scientist-turned-photographer Peter Rosén telling me that children were not supposed to look at or whistle at the dancing Auroras, or point at them in awe, otherwise the lights would come down and take them away.

Folktales said children were not supposed to look at the Auroras, otherwise the lights would come down and take them away (Credit: Lola Akinmade Åkerström)

Born and bred in Sweden, Rosén had grown up with these stories. Then in 1998, his career as an environmental researcher with the Climate Impacts Research Centre of Umeå University brought him to Abisko. He spent 13 years studying climate change in the Arctic through the Abisko Scientific Research Station. (In 2021, it was recognised as a Centennial Observing Station by the World Meteorological Organization.)

When he arrived in Abisko, Rosén quickly learned about the blue hole and became fascinated by the Northern Lights. He produced his first photographs of the Auroras in 2001, which are now part of permanent installations in galleries around northern Sweden, including the ICEHOTEL in the town of Jukkasjärvi. “My colleagues used to call me a ‘free-time researcher, full-time photographer’,” he joked.

By 2012, Rosén had quit his work in environmental science to become a full-time photographer and run Lappland Media, teaching travellers how to properly photograph the lights. He recalls one of his guests, who had dreamed of seeing the lights since she was five years old. She had sought them across Canada, Norway and Finland, but to no avail. On her first night in Abisko, she broke down and cried after seeing what Rosén considered a really weak Aurora. Over the coming nights, they witnessed strong spectacular displays together.

Perched close to the summit is the remote Aurora Sky Station, a 20-minute chairlift ride up from its base (Credit: Lola Akinmade Åkerström)

“Seeing how people express their feelings after seeing the lights makes me feel I have the best job in the world,” added Rosén. “I’ve never regretted leaving my life as a researcher, because I’m now living my dream.” 

I remember my own feeling of awe my first time I saw the lights in Abisko, at the foothills of Mount Nuolja, 900m above sea level. Perched close to the summit is the remote Aurora Sky Station, a 20-minute chairlift ride up from its base. There’s no better location to see the blue hole spread over the sparkling lights of Abisko and frozen Lake Torneträsk in the valley below.

This time, as Erik and I ascended the mountain, finally riding the chairlift into pitch darkness after driving through that storm, the experience evoked a feeling of reverence for what we were about to witness: ethereal green lights dancing and folding in the heavens like curtains above us.

Source: BBC Travel

How To Make The Universe Think For Us

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Physicists are building neural networks out of vibrations, voltages and lasers, arguing that the future of computing lies in exploiting the universe’s complex physical behaviors.

Inside a soundproofed crate sits one of the world’s worst neural networks. After being presented with an image of the number 6, it pauses for a moment before identifying the digit: zero. Peter McMahon, the physicist-engineer at Cornell University who led the development of the network, defends it with a sheepish smile, pointing out that the handwritten number looks sloppy. Logan Wright, a postdoc visiting McMahon’s lab from NTT Research, assures me that the device usually gets the answer right, but acknowledges that mistakes are common. “It’s just this bad,” he said.

Despite the underwhelming performance, this neural network is a groundbreaker. The researchers tip the crate over, revealing not a computer chip but a microphone angled toward a titanium plate that’s bolted to a speaker. Other neural networks operate in the digital world of 0s and 1s, but this device runs on sound. When Wright cues up a new image of a digit, its pixels get converted into audio and a faint chattering fills the lab as the speaker shakes the plate. Metallic reverberations do the “reading” rather than software running on silicon. That the device often succeeds beggars belief, even to its designers.

“Whatever the function of the shaking metal is, it shouldn’t have anything to do with classifying a handwritten digit”.

Peter McMahon

The primitive reading ability of the device, which the Cornell group unveiled in a paper in Nature in January, gives McMahon and others hope that its distant descendants could revolutionize computing.

When it comes to conventional machine learning, computer scientists have discovered that bigger is better. Stuffing a neural network with more artificial neurons — nodes that store numerical values — improves its ability to tell a dachshund from a Dalmatian, or to succeed at myriad other pattern recognition tasks. Truly tremendous neural networks can pull off unnervingly human undertakings like composing essays and creating illustrations. With more computational muscle, even grander feats may become possible. This potential has motivated a multitude of efforts to develop more powerful and efficient methods of computation.

McMahon and a band of like-minded physicists champion an unorthodox approach: Get the universe to crunch the numbers for us. “Many physical systems can naturally do some computation way more efficiently or faster than a computer can,” McMahon said. He cites wind tunnels: When engineers design a plane, they might digitize the blueprints and spend hours on a supercomputer simulating how air flows around the wings. Or they can stick the vehicle in a wind tunnel and see if it flies. From a computational perspective, the wind tunnel instantly “calculates” how wings interact with air.

Two men look at a computer screen.
Peter McMahon and Tatsuhiro Onodera are members of a team at Cornell that has programmed a variety of physical systems to accomplish learning tasks.Dave Burbank for Cornell University

A wind tunnel is a single-minded machine; it simulates aerodynamics. Researchers like McMahon are after an apparatus that can learn to do anything — a system that can adapt its behavior through trial and error to acquire any new ability, such as classifying handwritten digits or distinguishing one spoken vowel from another. Recent work has shown that physical systems like waves of light, networks of superconductors and branching streams of electrons can all learn.

“We are reinventing not just the hardware,” said Benjamin Scellier, a mathematician at the Swiss Federal Institute of Technology Zurich in Switzerland who helped design a new physical learning algorithm, but “also the whole computing paradigm.”

Learning to Think

Learning is an exotic process; until about a decade ago, brains were the only systems that did it well. It was the structure of the brain that loosely inspired computer scientists to design deep neural networks, now the most popular artificial learning models.

A deep neural network is a computer program that learns through practice. The network can be thought of as a grid: Layers of nodes called neurons, which store values, are connected to neurons in adjacent layers by lines, or “synapses.” Initially, these synapses are just random numbers known as “weights.”

When you want the network to read a digit — 4, say — you make the first layer of neurons represent a raw image of the 4, perhaps storing the shade of each pixel as a value in a corresponding neuron. Then the network “thinks,” moving layer by layer, multiplying the neuron values by the synaptic weights to populate the next layer of neurons. The neuron with the highest value in the final layer indicates the network’s answer. If it’s the second neuron, for instance, the network guesses that it saw a 2.

To teach the network to make smarter guesses, a learning algorithm works backward. After each trial, it calculates the difference between the guess and the correct answer (which, in our example, would be represented by a high value for the fourth neuron in the final layer and low values elsewhere). Then an algorithm steps back through the network layer by layer, calculating how to tweak the weights in order to get the values of the final neurons to rise or fall as needed. This procedure, known as backpropagation, lies at the heart of deep learning.

Through many guess-and-tweak repetitions, backpropagation guides the weights to a configuration of numbers that will, through a cascade of multiplications initiated by an image, spit out the digit written there.

An infographic explains how a vibrating metal plate can classify handwritten digits.
Merrill Sherman/Quanta Magazine

But compared to whatever goes on in the brain, the digitized version of learning that happens in artificial neural networks looks dramatically inefficient. On less than 2,000 calories a day, a human child learns to talk, read, play games, and much more in a few years. On such a restricted energy diet, the groundbreaking GPT-3, a neural network capable of fluent conversation, would have taken a millennium to learn to chat.

From a physicist’s perspective, a large digital neural network is simply trying to do too much math. Today’s biggest behemoths must record and manipulate more than half a trillion numbers. The universe, meanwhile, constantly pulls off tasks far beyond the limits of computers’ meager bookkeeping abilities. A room might have trillions of trillions of air molecules bouncing around; that’s an impossible number of moving pieces for a computer to track in a full-fledged simulation of collisions, but the air itself has no trouble deciding how to behave from moment to moment.

The challenge is to build physical systems that can naturally pull off both of the processes needed for AI — the “thinking” involved in (say) classifying an image, and the “learning” needed to classify such images correctly. A system that mastered both tasks would leverage the universe’s ability to act mathematically without actually doing math.

“We never compute 3.532 times 1.567 or something,” Scellier said. “It’s done, but implicitly, just by the laws of physics directly.”

The Thinking Part

McMahon and his collaborators have made progress on the “thinking” half of the puzzle.

While setting up his lab at Cornell in the final months of the pre-pandemic world, McMahon mulled over a curious finding. For years, the top-performing image-recognition neural networks had been getting ever deeper. That is, networks with more layers were better able to take in a bunch of pixels and put out a label, such as “poodle.” The trend inspired mathematicians to study the transformation (from pixels to “poodle”) that the networks were achieving, and in 2017 several groups proposed that the networks were acting like approximate versions of a smooth mathematical function. In math, a function turns an input (often a position along the x-axis) into an output (the y-value, or height, of a curve at that position). In a specific type of neural network, more layers do better because the function is less jagged, moving closer to some ideal curve.

The research got McMahon thinking. Perhaps with a smoothly changing physical system, one could sidestep the blockiness inherent in the digital approach.

The trick was to find a way to domesticate a complicated system — to adapt its behavior with training. McMahon and collaborators chose the titanium plate as one such system because its many patterns of vibrations blend incoming sound in convoluted ways. To make the plate act like a neural network, they fed in one sound that encoded the input image (a handwritten 6, for example), and another representing the synaptic weights; peaks and troughs needed to hit the titanium plate at precisely the right moments for the device to merge the sounds and give the answer — such as a new sound that’s loudest in the sixth millisecond, representing the classification “6.”

A triptych of photos. In the first, a microphone points at a black box containing a small metal plate. In the second, two hands hold a circuit board. In the last, a green laser illuminates mirrors and other optical components.
A team at Cornell University has trained three different physical systems to “read” handwritten digits: From left, a vibrating titanium plate, a crystal and an electronic circuit.
Rob Kurcoba for Cornell University (left and center); Charlie Wood for Quanta Magazine (right)

The group also implemented their scheme in an optical system — where the input image and weights are encoded in two beams of light that get jumbled together by a crystal — and in an electronic circuit capable of similarly shuffling inputs. In principle, any system with Byzantine behavior will do, though the researchers believe the optical system holds particular promise. Not only can a crystal blend light extremely quickly, but light also contains abundant data about the world. McMahon imagines miniaturized versions of his optical neural network someday serving as the eyes of self-driving cars, identifying stop signs and pedestrians before feeding that information to the vehicle’s computer chip, much as our retinas perform some basic visual processing on incoming light.

The Achilles heel of these systems, however, is that training them requires a return to the digital world. Backpropagation involves running a neural network in reverse, but plates and crystals don’t readily unmix sounds and light. So the group constructed a digital model of each physical system. Reversing these models on a laptop, they could use the backpropagation algorithm to calculate how to adjust the weights to give accurate answers.

With this training, the plate learned to classify handwritten digits correctly 87% of the time. The circuit and laser reached 93% and 97% accuracy, respectively. The results showed “that not only standard neural networks can be trained through backpropagation,” said Julie Grollier, a physicist at the French National Center for Scientific Research (CNRS). “That’s beautiful.”

The group’s quivering metal plate has not yet brought computing closer to the shocking efficiency of the brain. It doesn’t even approach the speed of digital neural networks. But McMahon views his devices as striking, if modest, proof that you don’t need a brain or computer chip to think. “Any physical system can be a neural network,” he said.

The Learning Part

Ideas abound for the other half of the puzzle — getting a system to learn all by itself.

Florian Marquardt, a physicist at the Max Planck Institute for the Science of Light in Germany, believes one option is to build a machine that runs backward. Last year, he and a collaborator proposed a physical analogue of the backpropagation algorithm that could run on such a system.

To show that it works, they digitally simulated a laser setup somewhat like McMahon’s, with the adjustable weights encoded in a light wave that mixes with another input wave (encoding, say, an image). They nudge the output to be closer to the right answer and use optical components to unmix the waves, reversing the process. “The magic,” Marquardt said, is that “when you try the device once more with the same input, [the output] now has a tendency to be closer to where you want it to be.” Next, they are collaborating with experimentalists to build such a system.

But focusing on systems that run in reverse limits the options, so other researchers are leaving backpropagation behind entirely. They take encouragement from knowing that the brain learns in some other way than standard backpropagation. “The brain doesn’t work like this,” said Scellier. Neuron A communicates with neuron B, “but it’s only one-way.”

A woman stands in a lab wearing a floral shirt.
Julie Grollier, a physicist at the French National Center for Scientific Research, has implemented a physical learning algorithm that’s seen as a promising alternative to backpropagation.Christophe Caudroy

In 2017, Scellier and Yoshua Bengio, a computer scientist at the University of Montreal, developed a unidirectional learning method called equilibrium propagation. To get a sense of how it works, imagine a network of arrows that act like neurons, their direction indicating a 0 or 1, connected in a grid by springs that act as synaptic weights. The looser a spring, the less the linked arrows tend to snap into alignment.

First, you twist arrows in the leftmost row to reflect the pixels of your handwritten digit and hold them fixed while the disturbance ripples out through the springs, flipping other arrows. When the flipping stops, the rightmost arrows give the answer.

Crucially, you don’t have to train this system by un-flipping the arrows. Instead, you connect another set of arrows showing the correct answer along the bottom of the network; these flip arrows in the upper set, and the whole grid settles into a new equilibrium. Finally, you compare the new orientations of the arrows with the old orientations and tighten or loosen each spring accordingly. Over many trials, the springs acquire smarter tensions in a way that Scellier and Bengio have shown is equivalent to backpropagation.

“It was thought that there was no possible link between physical neural networks and backpropagation,” said Grollier. “Very recently that’s what changed, and that’s very exciting.”

Initial work on equilibrium propagation was all theoretical. But in an upcoming publication, Grollier and Jérémie Laydevant, a physicist at CNRS, describe an execution of the algorithm on a machine called a quantum annealer, built by the company D-Wave. The apparatus has a network of thousands of interacting superconductors that can act like arrows linked by springs and naturally calculate how the “springs” should be updated. The system cannot update these synaptic weights automatically, though.

Closing the Circle

At least one team has gathered the pieces to build an electronic circuit that does all the heavy lifting — thinking, learning and updating weights — with physics. “We’ve been able to close the loop for a small system,” said Sam Dillavou, a physicist at the University of Pennsylvania.

A man looks at a glowing circuit.
Sam Dillavou, a physicist at the University of Pennsylvania, tinkers with a circuit that can modify itself as it learns.Jacob F. Wycoff

The goal for Dillavou and his collaborators is to emulate the brain, a literal smart substance: a relatively uniform system that learns without any single structure calling the shots. “Every neuron is doing its own thing,” he said.

To this end, they built a self-learning circuit, in which variable resistors act as the synaptic weights and neurons are the voltages measured between the resistors. To classify a given input, it translates the data into voltages that are applied to a few nodes. Electric current courses through the circuit, seeking the paths that dissipate the least energy and changing the voltages as it stabilizes. The answer is the voltage at specified output nodes.

Their major innovation came in the ever-challenging learning step, for which they devised a scheme similar to equilibrium propagation called coupled learning. As one circuit takes in data and “thinks up” a guess, an identical second circuit starts with the correct answer and incorporates it into its behavior. Finally, electronics connecting each pair of resistors automatically compare their values and adjust them to achieve a “smarter” configuration.

The group described their rudimentary circuit in a preprint last summer, showing that it could learn to distinguish three types of flowers with 95% accuracy. Now they’re working on a faster, more capable device.

Even that upgrade won’t come close to beating a state-of-the-art silicon chip. But the physicists building these systems suspect that digital neural networks — as mighty as they seem today — will eventually appear slow and inadequate next to their analog cousins. Digital neural networks can only scale up so much before getting bogged down by excessive computation, but bigger physical networks need not do anything but be themselves.

“It’s such a big, fast-moving and varied field that I find it hard to believe that there won’t be some pretty powerful computers made with these principles,” Dillavou said.

Source: Quanta Magazine

A Stunning Vision Of The Possibilities Of Humanity’s Expansion Into Space

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The US astrophysicist and author Carl Sagan was able to make complex scientific questions thoroughly arresting and human – at times even poetic. Set to awe-inspiring digital recreations of strange yet not unfamiliar worlds elsewhere in our solar system, Wanderers takes Sagan’s timeless words on the human instinct for exploration, and imagines what the next stage might look like: to Mars and beyond into space.

Director: Erik Wernquist

How Far Beyond Earth Will We Go To Safeguard Our Species?

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The human future in the cosmos could be all but limitless, if we don’t destroy ourselves first. The same would be true of intelligent aliens elsewhere in the Universe, assuming they exist: how far they travel depends strongly on how long they survive as a species. That survival variable, which the US astronomer Frank Drake incorporated into his famous equation on the likelihood of technological civilisations beyond Earth, is unknowable at present because we are the only such civilisation yet identified.

Let’s be optimistic and assume that humans are persistent, working their way through the manifest problems of mastering their tools – or at least mastering them long enough to plant colonies off-world, so that our destruction in one place doesn’t mean the death of the species.

There’s a lot of real estate to consider across the star lanes of the Milky Way. Take a sphere 100 light-years in radius, with the Earth at its centre: within it, there exist about 14,000 stars. Beyond that, we don’t know the frequency of habitable planets in our entire home galaxy of 200 billion stars, but current indications are that they’re plentiful, with some estimates running into the tens of billions. If we can begin planting even a few colonies elsewhere in our solar system, and eventually on planets around other suns, our species becomes ferociously hard to eliminate. Kill off one branch and the others persist: learning (we hope) from the sad experience of their forebears; trying new social experiments; pushing technologies to ever higher levels of sophistication; finding out about life elsewhere; and continuing to explore.

Our expansion into the galaxy will begin slowly, for the stars are immensely distant. Scatter 200 billion grains of salt – each representing a single star – into an approximation of the Milky Way and, in our neighbourhood, each grain of salt would be seven miles from its nearest counterpart. To reach Alpha Centauri, the triple-star system closest to our own, with a human crew we need to travel at least at 10 per cent of lightspeed (about 30,000 kilometres per second), making for a four-decade crossing. With the help of some form of suspended animation, the journey might be made easier.

Ten per cent of lightspeed is an attractive goal. It’s fast enough to reach the nearest stars in a single human lifetime, but not so fast that collisions with interstellar gas and dust cannot be protected against. We’ll need to tune up those technologies and learn to shield our crews from galactic cosmic rays. Deceleration at the destination is a huge problem, but possibilities exist. Perhaps the most plausible of these is using a magnetic field generated by a superconducting loop, a so-called ‘magsail’, that can open in the latter phases of the mission to brake over years against the stream of charged particles emitted by the target stars.

As to how to get to 10 per cent of lightspeed in the first place, numerous ideas are bruited about. If we had to make a choice right now, the technology with the highest likelihood of success is probably a vast sail. This would be a ‘lightsail’, driven by a powerful laser or microwave station in close proximity to the Sun; it would ride photons from the beam, acquiring their momentum. Strategies exist to tighten, or ‘collimate’, the beam through a huge lens in the outer solar system, or through a series of smaller lenses that can keep the beam on the departing spacecraft long enough for it to reach its substantial percentage of lightspeed. There are other possible interstellar propulsion strategies, from antimatter to fusion to interstellar ramjets.

To help the crew survive the journey, we can explore nanotechnology, artificial intelligence, and uploaded consciousness.

Whether it takes one or five or 20 centuries to make it happen, an outpost around another star could eventually grow into its own culture of star-faring. Now the timeframe widens. Give each colony 1,000 years to reach the point where it can begin building starships of its own. The species not only survives but begins to branch out from colonies around the nearby stars, one hop at a time, a slow spread across the Milky Way that is achievable within the known laws of physics.

No Star Trek engines here, although we can’t assume that future breakthroughs will not happen. The point is that even if they don’t, expansion into the galaxy is still feasible. If we’re willing to take our incessant drive to make everything happen in our own lifetimes off the table, then an even slower, and perhaps more likely, form of expansion is possible. Our experience building human habitats in space points to huge future space ‘arcologies’ – self-sustaining, city-size ships of the kind once imagined by the US physicist and futurist Gerard O’Neill, with thousands of people living in artificial, Earth-like environments.

A kilometres-long ‘worldship’ of this sort might travel much more slowly than our lightsail, perhaps a mere half a per cent of lightspeed (which is still 1,500 kilometres per second). Many of its inhabitants, living through generations aboard the vessel, might well decide after exploration of a new system that planet-based life is less appealing than a habitat they can control at all levels. Our descendants could one day explore planets but choose not to settle on them, living off space-based resources.

Our galaxy is 100,000 light-years across. Will we encounter other civilisations as we hop from star to star? Perhaps, and there might be numerous worlds we need to bypass as a result. The US astrophysicist Michael Hart has argued that a slow wave of expansion could cross the Milky Way within a few million years. By then, our spreading descendants probably would have differentiated so much from each other that we would no longer recognise them. They might no longer even be biological. Yet each of them would be a direct result of our civilisation, having embarked upon a celestial migration that can be, if we choose, all but unbounded.

In opposition to this optimistic scenario, the original question of survival persists. There are Sun-like stars billions of years older than our own. If it were possible to spread throughout the Milky Way, wouldn’t some civilisation have already done it? The rough passage through technological immaturity might be impassable. Still, we have no choice but to try, to stay alive long enough to get off-world in meaningful numbers before war or accident does us in. Above all else, interstellar flight is a human back-up strategy.

This article was originally published at Aeon and has been republished under Creative Commons.

Over 5,000 Exoplanets Have Now Been Discovered

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What do planets outside our solar system, or exoplanets, look like? A variety of possibilities are shown in this illustration. Scientists discovered the first exoplanets in the 1990s. As of 2022, the tally stands at just over 5,000 confirmed exoplanets.

This week, the NASA Exoplanet Archive logged the 5,000th confirmed planet outside of our solar system. This marks a huge advance since the first exoplanet discovery in 1992, when astronomers Aleksander Wolszczan and Dale Frail announced the discovery of two planets orbiting the pulsar PSR 1257+12. Now, the Archive contains confirmed sightings of planets in a wide range of shapes and sizes—from “hot Jupiters” to “super Earths”—but they still haven’t found any solar systems just like our own. In many cases, all astronomers know about these distant planets is their size and how far away from their stars they orbit. 

The TESS (Transiting Exoplanet Survey Satellite) mission currently in orbit may eventually add ten thousand more candidates to the lists of possible planets. The Nancy Grace Roman Space telescope and ESA’s ARIEL mission, both planned for launch later this decade, could add thousands more. And the James Webb Space Telescope, currently undergoing commissioning, will attempt to characterize the atmospheres of some of the planets astronomers have already discovered. 

Astronomer Jessie Christiansen, the NASA Exoplanet Archive Project science lead, joins John Dankosky to talk about what we know about planets around distant suns, and how researchers are working to learn more about these far-off worlds.

Source: Science Friday

This ’70s Artist Painted Our Future In Space

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Forty years ago, artist Rick Guidice teamed up with NASA scientists to envision the space civilizations of the future.

Before computer-illustrating software, aerospace engineers and astronomers turned to the skillful hands of technical illustrators to depict future space missions. Los Gatos-based artist Rick Guidice was among them. In 1971, he went from drawing earthbound buildings at an architectural design firm to painting celestial bodies and space settlements for NASA Ames Research Center in Mountain View, California.

Guidice was born and raised in San Jose, California, not far from the tech start-up companies sprouting across Silicon Valley. He began doing architectural illustrations when he was just 16-years-old, later studying fine art at the Academy of Art College in San Francisco. Between stints illustrating game advertisements for Atari and military maneuvers for the United States Air Force, Guidice worked for more than a decade alongside NASA scientists, illustrating missions and research so that their work could be shared with the public.

“Exterior of Double Cylinder Settlement,” by Rick Guidice, 1975. The structure has three long mirrors that revolve around the two cylinders (each is 20 miles long and four miles in diameter) to recreate day and night. The pods circling the ends of the cylinders are miniature environments ideal for growing the different types of crops that would be needed to support the million inhabitants of the colony. Image courtesy of NASA Ames Research Center and New Museum Los Gatos

Sometimes that meant filling in the details of a picture when the science was still developing. For example, Guidice remembers receiving fuzzy photos of Jupiter and Saturn—the source material available at the time—and being asked to paint NASA’s Pioneer probes zooming past the planets. “I drew paintings of these missions and what these planets would possibly look like without them being seen before,” he says.

Now a selection of Guidice’s work is on display at New Museum Los Gatos in California. The exhibit, which runs through February 14, 2016, focuses on his depictions of space settlements.

“Torus Wheel Settlement,” by Rick Guidice, 1976. The Stanford Torus Wheel Settlement is a ring-shaped colony meant to orbit Earth (there are two pictured here, one in the foreground and one in the distance). The habitat is a tube, 427 feet in diameter, bent in a wheel shape. The six inner spokes connect the sides of the tube across a distance of more than a mile. The tube spins once per minute to create gravity at levels similar to Earth’s and has a large mirror that can tilt to adjust sunlight levels. Image courtesy of NASA Ames Research Center and New Museum Los Gatos

In the 1970s, NASA was building up the space shuttle program to send humans beyond Earth’s atmosphere. That got some researchers thinking big about what could come next, such as structures capable of supporting whole cities and civilizations in space. During the summers of 1975-1977, scientists gathered at NASA Ames and Stanford University to design space settlements that incorporated only existing technology. The researchers asked how people would grow food, generate energy, and build colony infrastructures in outer space.

“The scientists wanted to know what would it be like if this earth became uninhabitable, and we had to turn to space,” says April Gage, an archivist working at NASA Ames. “What would it look like?”

It was Guidice’s job to illustrate several space colony concepts discussed in the Stanford sessions, including the O’Neill Double Cylinder (1975), the Bernal Sphere (1976), and the Stanford Torus Wheel (1976). While some colonies were intended to accommodate about 10,000 to 20,000 people, the O’Neill Double Cylinder could house on the order of a million, and was designed to generate its own gravitational pull, as well as simulate weather patterns found on Earth.

“Double Cylinder Settlement Interior,” by Rick Guidice, 1975. The tunneled interior of the O’Neill Double Cylinder was the first painting that Guidice was commissioned to produce. It remains his favorite among the collection partly because he was able to work with one of the fathers of space settlements, Princeton University physicist Gerard O’Neill. O’Neill requested that the interior have 500 square miles of sprawling green fields, designed to resemble an idyllic French countryside. Image courtesy of NASA Ames Research Center and New Museum Los Gatos

“If you think about the International Space Station, maybe four to five people are on that station,” says Gage. “When you look at these colonies, they are about 100 times larger. [The researchers] were looking at this using the technology of 1975. It’s fascinating to think about.”

While Guidice had no formal science training, he attended meetings with NASA’s mission directors and scientists to make sure he accurately reflected the technology discussed in the sessions. His depictions of gargantuan, space-roaming colonies might resemble the CGI-generated machines and hovercrafts seen in today’s science fiction movies. But back then, everything had to be done by hand, he says. “It was just drawn on paper with pencil [and paint], but it was done a long time ago in a very romantic fashion, you might say.” Each painting took him about three weeks to complete.

“Bernal Sphere,” by Rick Guidice, 1976. The Bernal Sphere was named after physicist and futurist John Desmond Bernal, who described an iteration of a spherical space ark in his 1929 book, “The World, the Flesh and the Devil.” Image courtesy of NASA Ames Research Center and New Museum Los Gatos

Guidice liked to paint with acrylics and often used warm, bold colors to give a luster to gases and stars. When Marianne McGrath, the curator of the space settlement exhibit at New Museum Los Gatos, came across his paintings, she was struck by how he transformed the science behind the designs into beautiful visions. “It’s not so cold or dark or vast,” she says. “The stars are almost within reach in these paintings.”

The three different colonies don’t appear as tin cans floating in outer space, but as a second home where people would want to live, McGrath says.

“Electromagnetic Mass Driver,” by Rick Guidice, 1977. In addition to illustrating space settlements, Guidice depicted the electromagnetic mass drivers that might one day make the mining of asteroids and moons possible. The mined material would be used to construct the colonies. Image courtesy of NASA Ames Research Center and New Museum Los Gatos

None of these settlements were ever constructed, but the colony concept lives on in NASA Ames’ annual Space Settlement Contest, which asks students up to 18-years-old from around the world to design their own space colonies. Recent research papers have also proposed scaled-down iterations of these colonies, residing within Earth’s orbit.

When Guidice’s paintings were first revealed to the public in the late 1970s, many people were surprised by how similar living in space seemed to how we live on Earth. That was by design, says Guidice. This portrayal of space colony life “is pleasurable to look at,” he says. What’s more, “it’s still something that looks into the future. When you look at it today, you get the same feeling and reaction of possibility as we did back then.”

Source: Science Friday

Solar Orbiter Heads For Closest Point To The Sun

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Never before has the space probe been this close to the Sun: In a few days, Solar Orbiter will venture to within 48 million kilometers of our star.

After two years in space, ESA’s spacecraft Solar Orbiter, to which NASA is also contributing, is heading for the best vantage point of its flight path so far. Next Saturday, March 26, only about 48 million kilometers will separate the probe from the Sun. That is less than a third of the distance between Earth and Sun. In the days around the so-called perihelion passage, the space probe is expected to record its most valuable data to date; the images of the hot solar corona will have the highest resolution of all times. Solar Orbiter will be able to exploit one of its key advantages: the simultaneous view into different layers of the Sun. The scientists involved hope that among other things this will provide new insights into how the smallest bursts of radiation in the corona arise from the magnetic fields of the visible solar surface. The Max Planck Institute for Solar System Research (MPS) in Germany has contributed to four of the mission’s ten scientific instruments.

Only 48 million kilometers will lie between Solar Orbiter an the Sun on March 26th.
Only 48 million kilometers will lie between Solar Orbiter an the Sun on March 26th.© ESA/ATG medialab

An enormous span of 150 million kilometers lie between Earth and Sun. Only few space probes have so far ventured within less than a third of this distance from our central star. From the end of March, Solar Orbiter will join this exclusive group: On Saturday, March 26, the spacecraft will fly past the Sun at a distance of about 48 million kilometers. This is only a few million kilometers more than the distance reached by the twin probes Helios A and B in the 1970s. Only NASA’s Parker Solar Probe has flown closer to the Sun, reaching a distance of just 8.5 million kilometers last year.

“Unlike its predecessors, Solar Orbiter is equipped with unusually comprehensive instrumentation,” explains MPS Director Prof. Dr. Sami K. Solanki.

The ten scientific instruments not only analyze the electromagnetic fields and solar particles that flow around the spacecraft, but for the first time can look at the Sun itself from a great proximity. For example, the instrument PHI (Polarimetric and Helioseismic Imager), which was developed and built under the lead of the MPS, observes the magnetic fields and flow velocities at the solar surface; EUI (Extreme-Ultraviolet Imager), SPICE (Spectral Imaging of the Coronal Environment) and the coronagraph Metis, to which the MPS contributed, provide information from the hot solar corona.

Radiation bursts and solar wind

There, EUI’s telescopes have in recent months been able to detect tiny bursts of radiation known as “campfires”. The phenomenon occurs more frequently than previously thought and could help to explain how the puzzlingly high temperatures of about one million degrees in the solar corona are generated. The visible solar surface is much “cooler” at about 6000 degrees. Data taken by PHI and EUI during their commissioning in 2020 and 2021 show that often closely adjacent regions of different magnetic polarity on the solar surface are the origin of this phenomenon. There is much to suggest that structural changes in these spatially confined magnetic fields are instrumental in supplying energy to the “campfires.” “According to our evaluations, however, other yet unknown processes must also play a role,” says MPS scientist Dr. Fatima Kahil, who analyzed these data. “We very much hope that the better-resolved data from the upcoming perihelion transit will help us better understand these processes,” she adds.

© ESA / S. Poletti
© ESA / S. Poletti

During the days around March 26, Solar Orbiter will also look at the Sun’s polar regions. So far, the spacecraft has left the orbital plane in which Earth and the other planets orbit the Sun by four degrees; by the end of the mission, that number is expected to rise to more than 30 degrees. This will make it possible to look at the Sun’s poles for the first time.

“Although Solar Orbiter’s view of the poles is not yet optimal, the timing is particularly favorable for such observations at the moment,” explains MPS scientist Prof. Dr. Hardi Peter, a member of the SPICE, EUI and Metis teams. In its approximately eleven-year cycle, the Sun’s activity has not yet reached its maximum. During this comparatively quiet phase, the fast solar wind emerges rather frequently from regions near the poles. With supersonic speeds of about 750 kilometers per second, these solar particles chase through space. Joint measurements by Solar Orbiter’s in situ instruments, which analyze these particles at the spacecraft’s location, and instruments looking at the Sun could provide insight into the acceleration mechanism. At the next perihelion transit in about six months, the fast solar wind should have already decreased further. Then, however, spontaneous eruptions of solar particles will occur more frequently.

And yet closer

Solar Orbiter’s current, highly elliptical orbit will change little over the next three years: About every six months, the spacecraft will reach its closest point to the Sun. However, with its next perihelion transit, due in October of this year, Solar Orbiter will move yet a little closer to the Sun, to 42 million kilometers. By then, Solar Orbiter will also have surpassed the Helios A and B probes.

Source: MPS

See The First-Ever Image Of A Black Hole In The Heart Of The Milky Way

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Observation with the Event Horizon Telescope improves our understanding of the processes at the galactic centre

It sits deep in the heart of the Milky Way, is 27,000 light years from Earth, and resembles a doughnut. This is how the black hole at the centre of our galaxy appears in the image obtained by researchers using the Event Horizon Telescope (EHT). The team has thus provided evidence that, as suspected, this object belongs to the family of cosmic gravity traps. The radio data from the observatories connected in the worldwide EHT network were obtained from two supercomputers: one at the Max Planck Institute for Radio Astronomy in Bonn and one at the Haystack Observatory in Massachusetts. The Apex telescope of the Bonn Institute and the 30-metre antenna of the Institut de Radioastronomie Millimétrique (IRAM), which belongs to the Max Planck Society, were also involved in the observation.

Cosmic ring of fire: This is the first image of Sagittarius A*, the supermassive black hole at the centre of the Milky Way. It was taken by the Event Horizon Telescope (EHT), a network that combines radio observatories around the world into a single virtual telescope the size of the Earth. The EHT is named after the “event horizon”, the boundary of the black hole beyond which no light can escape. Although the event horizon itself is not visible because it does not emit light, glowing gas swirling around the black hole shows a tell-tale signature: a dark central region (shadow) surrounded by a bright ring-shaped structure. The image captures light bent by the strong gravity of the black hole and is four million times more massive than the sun. The image is an average of the various images extracted by the EHT collaboration from their observations in April 2017. The images can also be clustered into four groups based on similar features. An averaged, representative image for each of the four clusters is shown in the bottom row. Three of the clusters show a ring structure but, with differently distributed brightness around the ring. The fourth cluster contains images that also fit the data but do not appear ring-like. The bar graphs show the relative number of images belonging to each cluster. Thousands of images fell into each of the first three clusters, while the fourth and smallest cluster contains only hundreds of images. The heights of the bars indicate the relative contributions of each cluster to the averaged image at top.  © EHT collaboration
Cosmic ring of fire: This is the first image of Sagittarius A*, the supermassive black hole at the centre of the Milky Way. It was taken by the Event Horizon Telescope (EHT), a network that combines radio observatories around the world into a single virtual telescope the size of the Earth. The EHT is named after the “event horizon”, the boundary of the black hole beyond which no light can escape. Although the event horizon itself is not visible because it does not emit light, glowing gas swirling around the black hole shows a tell-tale signature: a dark central region (shadow) surrounded by a bright ring-shaped structure. The image captures light bent by the strong gravity of the black hole and is four million times more massive than the sun. The image is an average of the various images extracted by the EHT collaboration from their observations in April 2017. The images can also be clustered into four groups based on similar features. An averaged, representative image for each of the four clusters is shown in the bottom row. Three of the clusters show a ring structure but, with differently distributed brightness around the ring. The fourth cluster contains images that also fit the data but do not appear ring-like. The bar graphs show the relative number of images belonging to each cluster. Thousands of images fell into each of the first three clusters, while the fourth and smallest cluster contains only hundreds of images. The heights of the bars indicate the relative contributions of each cluster to the averaged image at top. © EHT collaboration

The recently published image is the long-awaited direct view of the object at the centre of our galaxy known as Sagittarius A*. For many years, researchers have been examining this area of the Milky Way and observing stars that orbit an invisible, compact, and massive object. For this work, Andrea Ghez from the University of California and Reinhard Genzel from the Max Planck Institute for Extraterrestrial Physics in Garching were awarded the Nobel Prize in 2020.

“Our discovery shows that the object at the galactic centre is indeed a black hole”, says Anton Zensus, Director at the Max Planck Institute for Radio Astronomy and founding chair of the Supervisory Board of the EHT. The image is the first direct visual proof of this. The black hole itself is not visible in the image because it does not emit any radiation. But the glowing gas around it shows a tell-tale signature – a dark central region (shadow) surrounded by a bright ring-like structure. Their light is bent by the immense gravity of the black hole.

“We were amazed at how well the size of the observed ring matched the predictions of Einstein’s general theory of relativity”, says EHT project scientist Geoffrey Bower from the Institute of Astronomy and Astrophysics at Academia Sinica in Taipei. The observations would greatly have improved the understanding of the physical processes taking place at the centres of galaxies and would provide insights into how such giant gravity traps interact with their surroundings.

Because the black hole at the centre of the Milky Way is 27,000 light years away from Earth, it appears to us in the sky about as big as a doughnut on the moon. In order to image it, the team created the powerful EHT, which links eight (now 11) radio observatories around the world into a single Earth-sized virtual telescope. Using interferometry, the astronomers observed the object Sagittarius A* during several nights in April 2017. At a wavelength of 1.3 millimetres, they collected data for many hours at a time – similar to the long exposure time of a camera. These data were analysed by two correlators – high-performance computers located at the Max Planck Institute for Radio Astronomy and the Haystack Observatory.

The Max Planck Institute was also involved in the campaign with an antenna. “The contribution of our Apex telescope was essential for perfectly calibrating the changing brightness of the source and providing definitive proof of the black hole shadow at the galactic centre”, says Director Karl Menten.

Worldwide network: When the researchers collected the data from the centre of the Milky Way in 2017, the Event Horizon Telescope consisted of eight observatories spread across the globe.  © EHT collaboration
Worldwide network: When the researchers collected the data from the centre of the Milky Way in 2017, the Event Horizon Telescope consisted of eight observatories spread across the globe. © EHT collaboration

The current observation follows the 2019 image of a black hole (M 87*) at the centre of the galaxy Messier 87, which lies at a much greater distance from Earth. The two black holes are similar – although the one at the centre of the Milky Way is more than one thousand times smaller and much lighter than M 87*. “We are dealing with two completely different types of galaxies and two different masses of black holes. But near their edges, they look amazingly similar”, says Sera Markoff, co-chair of the Council of Sciences of the EHT and professor of theoretical astrophysics at the University of Amsterdam.

This time, the evaluation of the data was much more difficult than with the galaxy M 87, 55 million light years away – even though the centre of the Milky Way is much closer (27,000 light years). The gas swirls around the two black holes at practically the same speed – almost as fast as light. But while it takes days to weeks to orbit the larger object M 87*, it orbits of the much smaller Sagittarius A* in just a few minutes. “The brightness and appearance of the gas around Sagittarius A* thus changed rapidly during our observation”, says Chi-kwan Chan from the University of Arizona. “It’s like trying to take a sharp image of a dog vigorously wagging its tail”.

The researchers had to develop sophisticated new methods in order to explain the gas movements around the Sagittarius A* black hole, which “weighs” around four million solar masses. In contrast, M 87*, weighing six and a half billion solar masses, was an easier and more stable target. In addition, Earth is in the galactic plane; this causes a scattering effect in the radio measurements. Hot gas with charged particles and magnetic fields in the line of sight also complicate the analysis.

The image of Sagittarius A* is thus an average of various images that the team extracted from the data. Maciek Wielgus and Michael Janßen, both from the Max Planck Institute for Radio Astronomy, played a major role in the calibration. For tests of general relativity and proof of an event horizon, their colleague Gunther Witzel compiled the results of other observations.

Concentrated computing power: The scientists used this high-performance computer at the Max Planck Institute for Radio Astronomy to analyse the data from the Event Horizon Telescope. A second correlator is located at the Haystack Observatory in the US.  © MPIfR
Concentrated computing power: The scientists used this high-performance computer at the Max Planck Institute for Radio Astronomy to analyse the data from the Event Horizon Telescope. A second correlator is located at the Haystack Observatory in the US. © MPIfR

The EHT collaboration includes more than 300 researchers from 80 institutes worldwide. Over the past five years, the team has developed complex instruments and compiled a unique library of numerically simulated black holes to compare with observations. Among other things, these serve to test the theories of gravitation.

According to Michael Kramer, Director at the Max Planck Institute and one of the project leaders of the Black Hole Cam project, the earlier image of M 87* was only partially suitable for this purpose. “For Messier 87, we had no reliable prior knowledge about the mass of the black hole. In the current case, it is quite different. Thanks to previous measurements such as those by Reinhard Genzel, we know both the distance and the mass of Sagittarius A* quite precisely. We were thus able to calculate the expected shadow size in order to compare it with the observations. And it fits quite well.” The Black Hole Cam project was funded by the European Research Council (ERC) and plays an important role within the EHT collaboration.

Using the images of the two differently-sized black holes, the researchers can compare the two objects and check how they differ. The new data can also be used to test theories and models about how gravity and matter behave in the extreme environment of supermassive black holes. This is not yet fully understood but apparently plays a key role in the formation and evolution of galaxies.

IRAM Director Karl Schuster emphasizes the many years of joint pioneering work between the Max Planck Institute for Radio Astronomy and his institute in Grenoble, France. “The results from the Event Horizon Telescope are an ideal complement to the results obtained by Reinhard Genzel’s group at the Max Planck Institute for Extraterrestrial Physics in the infra-red range with the Gravity instrument”. Meanwhile, measurements with the Event Horizon Telescope continue. Eleven observatories were involved in a major campaign in March 2022. “Of course, we are all quite excited to see what the EHT observations in 2021 and 2022 will reveal with the participation of our powerful Noema observatory”, says Schuster.

ER / HOR / NJ

Source: Max-Planck-Gesellschaft

Every Moment And Blink Of An Eye, The Universe Does These

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How long do we spend blinking? And how many times do we blink a day?

According to technology research, blinks last on average about a tenth of a second which is 100 milliseconds and we blinks about 518,017,359 times in our entire life. We know that the average person blinks 15 to 20 times a minute.

“A LOT CAN HAPPEN IN THE BLINK OF AN EYE.”

Source: melodysheep

When we look up at night, the universe seems pretty quiet. But that perspective is an illusion; in reality, there are millions of world-shattering events happening every instant across the cosmos. This short film explores just how much is going on every moment in our ridiculously enormous universe.

In the fraction of a second it takes to blink your eyes, thousands of stars will be born, hundreds will explode and die, millions of planets will form, and our universe will expand by half a million kilometers in diameter. And these numbers only account for the observable universe — not for what could be happening beyond, where some scientists believe there could be an infinite expanse of space.

THINK NEXT TIME YOU BLINK.

The Secret History of the Moon

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Where did the moon come from?

The Moon has drawn out our sense of wonder since before we were fully human. Where did it come from? What secrets are written in its rocks?

In this epic video, filmmaker John D. Boswell explores the secret history of the moon—what we think we know, what still puzzles us, and how new theory may help reconcile the two.

Where did the moon come from?

The leading theory suggests the moon was formed after a massive collision between a Mars-sized planet Theia and Earth in the early days of the solar system. Theia was smashed apart and reformed in Earth’s orbit as the moon. Called the giant impact theory, the general idea is solid but the exact details remain a work in progress. In recent years, scientists have proposed new ideas to further sharpen science’s best lunar creation story.

For most of our history, its story was cloaked in myth and mystery. Only now are the vivid details coming into focus. This video takes you back 4.5 billion years to witness the dramatic ways which the moon could have formed, according to the latest mind-blowing theories. By reading the clues written in Moon rocks, we are closer than ever to knowing its full story. But the Moon still holds its secrets close. What else is it hiding?

As the moon is the only substantial body in the solar system that we have travelled to and retrieved rocks from, its samples are valuable to scientists. Dr Snape has studied the ratios of isotopes of lead and uranium in rocks returned by the Apollo missions and from lunar meteorites. This ratio acts as a deep-time clock that he has used to calculate when a rock formed. 

‘The moon has a record and acts as a beautiful lab for understanding early planetary processes. This will be applicable to Mars, Mercury or Venus, places that are hard for us to access, and it can even tell us about our own planet,’ said Dr Snape.

Earth is not quite so useful because plate tectonics bury and recycle rocks. 

‘This is why we love the moon so much,’ he said. ‘It is a treasure trove, geologically speaking.’