In 1960, famed theoretical physicist Freeman Dyson made a radical proposal. In a paper titled “Search for Artificial Stellar Sources of Infrared Radiation” he suggested that advanced extra-terrestrial intelligences (ETIs) could be found by looking for signs of artificial structures so large, they encompassed entire star systems (aka. megastructures). Since then, many scientists have come up with their own ideas for possible megastructures.
Like Dyson’s proposed Sphere, these ideas were suggested as a way of giving scientists engaged in the Search for Extra-Terrestrial Intelligence (SETI) something to look for. Adding to this fascinating field, Dr. Albert Jackson of the Houston-based technology company Triton Systems recently released a study where he proposed how an advanced ETI could use rely on a neutron star or black hole to focus neutrino beams to create a beacon.
There’s a remote chance that inexplicable light variations in a star in the Northern Cross may be caused by the works of an alien civilization.
1,480 light years from Earth twinkles one of the greatest mysteries of recent times. There in the constellation Cygnus the Swan, you’ll find a dim, ordinary-looking point of light with an innocent sounding name — Tabby’s Star. Named for Louisiana State University astronomer Tabetha Boyajian, who was the lead author on a paper about its behavior, this star has so confounded astronomers with its unpredictable ups and downs in its brightness, they’ve gone to war on the object, drilling down on it with everything from the Hubble to the monster 393.7-inch (10-meter) Keck Telescope in Hawaii.
Tabby’s Star was uncovered by the Kepler Space Telescope during its examination of of more than 150,000 stars in the Milky Way. Kepler sought out stars accompanied by planets. By recording tiny, repeating fading of the star’s light as a planet passes in front a star, astronomers could determine the planet’s size, orbit and much more. All told, Kepler nabbed more than 2,300 new planets orbiting a host of stars in the constellations Lyra and Cygnus.
Among the stars Kepler viewed in its survey was one KIC 8462852 (Tabby’s Star). Unlike the others, its light dimmed in a completely unpredictable way. Things in orbit produce repeatable patterns, so astronomers began searching for alternative explanations. Might the star be variable? Lots of stars undergo physical changes such as pulsations or even explosions that cause them to vary in brightness. Nope. Based on its type, a stable star similar to the sun, and the fact that most of the time, it remains shining with a steady light, it didn’t fit the pattern.
The star dims by as much as 22% for days at a time at irregular intervals. Stars fade and re-brighten, but not in the way this star does according to astronomers. Researchers ruled out many possibilities including instrumental errors, starspots (like sunspots but on other stars), dust rings seen around young, evolving stars (this is an older star) and pulsations that can cloak it with light-absorbing dust clouds. Dust clouds don’t work because they’d warm up in the star’s light and radiate heat that we could detect with infrared telescopes. We see no excess of glowing dust, ruling that possibility out, too.
Casting about for potential answers, Boyajian and team hit on the hypothesis that an enormous cloud of comets might be behind the light fluctuations. Imagine these comets, fragile creatures that they are, breaking up into fragments that cascade into smaller pieces over time, creating a host of irregular and chaotic variations in Tabby’s light.
While that may be a reach, there’s even a stranger possibility. Jason Wright, an assistant professor of astronomy at Penn State, would like us to consider an alien civilization as the cause. Although the possibility is a remote one, he asks us to consider that an alien civilization may be building a megastructure known as a Dyson Sphere around its home star. A Dyson Sphere is a hypothetical sphere constructed around a star. Built of enormous solar panels, it would capture the star’s energy and convert it into electricity to power a technological civilization.
Now imagine if you will, thousands of huge panels in various stages of construction and position orbiting Tabby’s Star, and you just might have an explanation for its mysterious ups and downs. Far-fetched? Of course. But there may be a way to prove it.
A technologically advanced civilization would presumably need to communicate over long distances just like humans do. We use radio and TV, both of which transmit at very specific and narrow frequencies. Every time you go up and down the radio dial, each station you hear is beaming powerful radio waves at a specific frequency or vibration rate. Natural processes are more casual with a broader spread of frequencies. If we could detect a powerful signal at a specific frequency coming from Tabby’s Star, it could potentially be an indication of an alien species at work transmitting their own version of Dancing with the Stars.
So how do we do this? How can even know what frequencies they’ll be using to transmit? Well, you take the Green Bank Radio Telescope, the largest fully steerable radio telescope on the planet, and hook it up with a new SETI instrument that can look at an enormous swath of bandwidth simultaneously in billions of different radio channels. That’s exactly what happened Wednesday night (Oct. 26) as part of the Breakthrough Listen project, a $100 million initiative by Russian tycoon Yuri Milner to search for intelligent life in the universe.
University of California Berkeley astronomers devoted eight hours of scope time last night “listening” to Tabby’s Star for potential signs of an extraterrestrial civilization. They’ll spend two more nights in the coming two months at it and then analyze the data, a process that will take more than a month. Perhaps then we’ll finally get an answer. I hope it’s an alien one, but of course that’s a long shot. Stay tuned.
**** My new book, Night Sky with the Naked Eye, will be published on Nov. 8, but you can pre-order right now at these online stores. Just click an icon to go to the site of your choice – Amazon, Barnes & Noble or Indiebound. It’s currently available at the first two outlets for a very nice discount:
Last fall, astronomers were surprised when the Kepler mission reported some anomalous readings from KIC 8462852 (aka. Tabby’s Star). After noticing a strange and sudden drop in brightness, speculation began as to what could be causing it – with some going so far as to suggest that it was an alien megastructure. Naturally, the speculation didn’t last long, as further observations revealed no signs of intelligent life or artificial structures.
But the mystery of the strange dimming has not gone away. What’s more, in a paper posted this past Friday to arXiv, Benjamin T. Montet and Joshua D. Simon (astronomers from the Cahill Center for Astronomy and Astrophysics at Caltech and the Carnegie Institute of Science, respectively) have shown how an analysis of the star’s long-term behavior has only deepened the mystery further.
To recap, dips in brightness are quite common when observing distant stars. In fact, this is one of the primary techniques employed by the Kepler mission and other telescopes to determine if planets are orbiting a star (known as Transit Method). However, the “light curve” of Tabby’s Star – named after the lead author of the study that first detailed the phenomena (Tabetha S. Boyajian) – was particularly pronounced and unusual.
According to the study, the star would experience a ~20% dip in brightness, which would last for between 5 and 80 days. This was not consistent with a transitting planet, and Boyajian and her colleagues hypothesized that it was due to a swarm of cold, dusty comet fragments in a highly eccentric orbit accounted for the dimming.
However, others speculated that it could be the result of an alien megastructure known as Dyson Sphere (or Swarm), a series of structures that encompass a star in whole or in part. However, the SETI Institute quickly weighed in and indicated that radio reconnaissance of KIC 8462852 found no evidence of technology-related radio signals from the star.
Other suggestions were made as well, but as Dr. Simon of the Carnegie Institute of Science explained via email, they fell short. “Because the brief dimming events identified by Boyajian et al. were unprecedented, they sparked a wide range of ideas to explain them,” he said. “So far, none of the proposals have been very compelling – in general, they can explain some of the behavior of KIC 8462852, but not all of it.”
To put the observations made last Fall into a larger context, Montet and Simon decided to examine the full-frame photometeric images of KIC 8462852 obtained by Kepler over the last four years. What they found was that the total brightness of the star had been diminishing quite astonishingly during that time, a fact which only deepens the mystery of the star’s light curve.
As Dr. Montet told Universe Today via email:
“Every 30 minutes, Kepler measures the brightness of 160,000 stars in its field of view (100 square degrees, or approximately as big as your hand at arm’s length). The Kepler data processing pipeline intentionally removes long-term trends, because they are hard to separate from instrumental effects and they make the search for planets harder. Once a month though, they download the full frame, so the brightness of every object in the field can be measured. From this data, we can separate the instrumental effects from astrophysical effects by seeing how the brightness of any particular star changes relative to all its neighboring stars.”
Specifically, they found that over the course of the first 1000 days of observation, the star experienced a relatively consistent drop in brightness of 0.341% ± 0.041%, which worked out to a total dimming of 0.9%. However, during the next 200 days, the star dimmed much more rapidly, with its total stellar flux dropping by more than 2%.
For the final 200 days, the star’s magnitude once again consistent and similar to what it was during the first 1000 – roughly equivalent to 0.341%. What is impressive about this is the highly anomalous nature of it, and how it only makes the star seem stranger. As Simon put it:
“Our results show that over the four years KIC 8462852 was observed by Kepler, it steadily dimmed. For the first 2.7 years of the Kepler mission the star faded by about 0.9%. Its brightness then decreased much faster for the next six months, declining by almost 2.5% more, for a total brightness change of around 3%. We haven’t yet found any other Kepler stars that faded by that much over the four-year mission, or that decreased by 2.5% in six months.”
Of the over 150,000 stars monitored by the Kepler mission, Tabby’s Starr is the only one known to exhibit this type of behavior. In addition, Monetet and Cahill compared the results they obtained to data from 193 nearby stars that had been observed by Kepler, as well as data obtained on 355 stars with similar stellar parameters.
From this rather large sampling, they found that a 0.6% change in luminosity over a four year period – which worked out to about 0.341% per year – was quite common. But none ever experienced the rapid decline of more than 2% that KIC 8462852 experienced during that 200 days interval, or the cumulative fading of 3% that it experienced overall.
Montet and Cahill looked for possible explanations, considering whether the rapid decline could be caused by a cloud of transiting circumstellar material. But whereas some phenomena can explain the long-term trend, and other the short-term trend, no one explanation can account for it all. As Montet explained:
“We propose in our paper that a cloud of gas and dust from the remnants of a planetesimal after a collision in the outer solar system of this star could explain the 2.5% dip of the star (as it passes along our line of sight). Additionally, if some clumps of matter from this collision were collided into high-eccentricity comet-like orbits, they could explain the flickering from Boyajian et al., but this model doesn’t do a nice job of explaining the long-term dimming. Other researchers are working to develop different models to explain what we see, but they’re still working on these models and haven’t submitted them for publication yet. Broadly speaking, all three effects we observe cannot be explained by any known stellar phenomenon, so it’s almost certainly the result of some material along our line of sight passing between us and the star. We just have to figure out what!”
So the question remains, what accounts for this strange dimming effect around this star? Is there yet some singular stellar phenomena that could account for it all? Or is this just the result of good timing, with astronomers being fortunate enough to see a combination of a things at work in the same period? Hard to say, and the only way we will know for sure is to keep our eye on this strangely dimming star.
And in the meantime, will the alien enthusiasts not see this as a possible resolution to the Fermi Paradox? Most likely!
Now, I’m no futurist, but I think I can predict one thing. Humans love to use energy, and in the future, we’re going to use even more of the stuff.
Let’s hope it’s clean energy, like that handy source of photons in the sky: the Sun. Not dirty forms of energy, like screams, unobtainium, liquid Shwartz, or using humans as batteries.
Once we really get our hands on a clean, unlimited source of energy, you can expect our usage to grow and grow until every human on Earth is using as much energy as a small country.
We will climb our way up through the Kardashev scale of energy usage, from Type 1, to Type II to Type III. Type III! Can you even imagine what would happen at that point?
Oh, you have no idea what I’m talking about? No problem.
The Kardashev Scale was originally developed by the Soviet astronomer Nikolai Kardashev in 1964. He looked at the advancement of humanity’s need for energy, and then just extrapolated when what our future energy demands would look like – and how they’d be supplied.
He broke them into three types. A Type I civilization would have complete and total mastery over all the energy of its planet. A Type II civilization would be masters of all the energy produced by their home star, and a Type III civilization would own all the energy in their home galaxy.
It was a pretty clever way to categorize the mighty capabilities of future civilizations, and it’s fueled the imagination of many sci-fi writers.
Where are we now along the Kardashev Scale? How long will it take for us to unlock each civilization level? Assuming we survive, of course.
Kardashev estimated that the total energy usage of a Type I civilization based on the amount of sunlight that falls on Earth. Our planet receives about 2 x 10^17 watts of power from the Sun.
Is that a lot? Is sure sounds like a lot. In 2013, the total human power consumption was 12.3 terawatts. So, doing a little math, we get about 1/14,000th the total potential power output that falls on the Earth.
It sounds like we’ve got a long way to making up that difference. But wait a second, we’re in the realm of exponential growth now, which has a surprising way of sneaking up on you.
Freeman Dyson, the famous physicist, estimated that it’ll only take about 200 years to fully utilize the energy falling on the Earth. That seems amazing, but when you consider that Germany was able to pump out 25 gigawatts of power in April, 2015, it doesn’t stretch your imagination too far.
Where do we go from there?
Kardashev estimated a compounding energy usage of 1% per year. And so, if you extrapolate forward from our current energy usage, he figured it would take about 3,200 more years to reach Type II status, where we’re extracting 100% of the energy pouring out of the Sun – all 4 x 10^26 watts.
Probably by using Dyson sphere, cloud or other Dyson-related polygon. We might have to dismantle all the planets to do it, but that’s just what we’ll do to keep up with our ravenous energy needs.
I know you look around your house, see your various appliances, and you’re unable to imagine how you could use that much power. But trust me, you will. You might have nanofactories, spinning out furniture made of pure diamond. Or a massive, planet-sized computer calculating the answer to life the universe and everything. Or a console that’ll let you play Witcher 3 without dropping frames. When energy is cheap and clean, all kinds of impossible ideas become reasonable.
Continuing this 1% compounding energy usage, Kardashev figured we’d be using up all the energy of our host galaxy within a few hundred thousand years – 10^37 watts -, but that’s mostly because of the time it takes to travel to from star to star. The Milky Way measures 120,000 light-years across, so even colonizing the entire galaxy couldn’t happen faster than that.
Imagine an entire galaxy, with every solar system completely dismantled and every star enclosed in a Dyson cloud of energy extracting solar cells. And yet, constant growth inevitably predicts it.
Is that it? Is that as much as a future civilization could colonize? Hardly, they would really just be getting started. A future civilization with that much energy at their disposal would be able to expand outward at just shy of the speed of light, eventually colonizing everything that the laws of physics would enable them to get to.
Eventually the expansion of the Universe, accelerated by dark energy would bring their colonization to a stop. Galaxies would drop over the cosmic horizon, forever out of reach. Vast cosmic power with no where else to go.
Thanks to Kardashev, we’ve got a great way of considering our place in the Universe. Assuming we don’t wipe ourselves out, we’ve got a bright future ahead.
In the list of crazy hypothetical ideas, terraforming the Sun has to be one of the top 10. So just how would someone go about doing terraforming our sun, a star, if they wanted to try?
In our series on terraforming other worlds, we’ve covered Mars, Venus, the Moon and Jupiter. Even though I solved the problem of how to terraform Jupiter (you’re welcome, science), you wanted to take things to the next level and you demanded I sort out how to terraform the Sun. Seriously? The Sun. Fine… here we go.
Let’s see what we’ve got to work with here. It’s a massive ball of plasma, containing 333,000 times more mass than the Earth. It’s about 74% hydrogen and 25% helium with a few other trace elements. There’s no solid surface to stand on it, so we need to fix that.
The average temperature on the surface of the Sun is about 5,500 Celsius, while the average temperature on Earth is about 15 C. Iron boils at only 2,800 degrees, so… that’s probably too hot. We’ll need to cool it down.
The gravity on the surface of the Sun is 28 times the gravity of Earth. If you could stand on the surface of the Sun, which you can’t, you’d be crushed flat. Okay, so we’ll add reduce the gravity… check.
There’s no breathable atmosphere, there’s no solid ground, the Sun generates deadly X-rays. Oh, and don’t forget about the terrible sunburns from the ultraviolet radiation.
So, what’s the list? Hot fire unbreathable pressure cooker goo surface gravity crushing machine. Sounds impossible, or does it?
First, the gas. As we covered in a previous episode, scientists have actually considered ways that you might extract the hydrogen and helium off of a star like the Sun, known as “stellar lifting”. There are a few ways you could work this. You could zap the surface of the Sun with a powerful laser, increasing the speed of solar wind in that area, forcing the Sun to throw its mass off into space.
Another method is to set up powerful magnetic fields around the Sun’s poles, and channel its hydrogen into jets that blast out into space. I’m not sure how you actually set up those magnetic fields, but that’s not my problem.
Once you’re done with the Sun, you’ve stripped away all its hydrogen and helium gas. What are you left with? About 5,600 times the mass of the Earth in heavier elements, like oxygen, silicon, gold, etc. Great!
Except 5,600 sounds like a lot. Jupiter is only 316 times the mass of the Earth. We’re looking to reform a “planet” with more than 10 times the mass of Jupiter. And not only that, but we had to kill the Sun to make this work. You monsters.
This is a terrible idea. What else could we do? If you’re a science fiction fan, you’ve heard of a Dyson Sphere. If not, you’ve got some TNG to catch up on.
First proposed by Freeman Dyson, you cover an entire Sun in a metal ball. Instead of the measly amount of energy that falls on Earth, this would allow you to capture 100% of the energy released by the Sun: 384 yottawatts.
According to Dyson and a variety of matheletes, you could dismantle all planets in the Solar System and build a sphere at a distance of 1 Earth radii at 8 to 20 centimeters thick. That would give you a surface area 550 million times more than the Earth.
Although, building an actual rigid sphere is probably unfeasible because it would be pretty unstable and eventually collapse. It probably makes more sense to build a swarm of satellites surrounding the Sun, capturing its energy.
We did a whole video on Dyson Spheres. Check it out here.
So there you go. I just terraformed the Sun. I’m terrified about your next suggestion: how could you terraform a black hole? I guess that’ll be the next video.
Would you like to live on my imagined terraformed Sun? If not, what about a Dyson Sphere or swarm?
Beam us up, Scotty. There’s no signs of intelligent life out there. At least, no obvious signs, according to a recent survey performed by researchers at Penn State University. After reviewing data taken by the NASA Wide-field Infrared Survey Explorer (WISE) space telescope of over 100,000 galaxies, there appears to be little evidence that advanced, spacefaring civilizations exist in any of them.
First deployed in 2009, the WISE mission has been able to identify thousands of asteroids in our solar system and previously undiscovered star clusters in our galaxy. However, Jason T. Wright, an assistant professor of astronomy and astrophysics at the Center for Exoplanets and Habitable Worlds at Penn State University, conceived of and initiated a new field of research – using the infrared data to assist in the search for signs of extra-terrestrial civilizations.
And while their first look did not yield much in the way of results, it is an exciting new area of research and provides some very useful information on one of the greatest questions ever asked: are we alone in the universe?
“The idea behind our research is that, if an entire galaxy had been colonized by an advanced spacefaring civilization, the energy produced by that civilization’s technologies would be detectable in mid-infrared wavelengths,” said Wright, “exactly the radiation that the WISE satellite was designed to detect for other astronomical purposes.”
This logic is in keeping with the theories of Russian astronomer Nikolai Kardashev and theoretical physicist Freeman Dyson. In 1964, Kardashev proposed that a civilization’s level of technological advancement could be measured based on the amount of energy that civilization is able to utilize.
To characterize the level of extra-terrestrial development, Kardashev developed a three category system – Type I, II, and III civilizations – known as the “Kardashev Scale”. A Type I civilization uses all available resources on its home planet, while a Type II is able to harness all the energy of its star. Type III civilizations are those that are advanced enough to harness the energy of their entire galaxy.
Similarly, Dyson proposed in 1960 that advanced alien civilizations beyond Earth could be detected by the telltale evidence of their mid-infrared emissions. Believing that a sufficiently advanced civilization would be able to enclose their parent star, he believed it would be possible to search for extraterrestrials by looking for large objects radiating in the infrared range of the electromagnetic spectrum.
These thoughts were expressed in a short paper submitted to the journal Science, entitled “Search for Artificial Stellar Sources of Infrared Radiation“. In it, Dyson proposed that an advanced species would use artificial structures – now referred to as “Dyson Spheres” (though he used the term “shell” in his paper) – to intercept electromagnetic radiation with wavelengths from visible light downwards and radiating waste heat outwards as infrared radiation.
“Whether an advanced spacefaring civilization uses the large amounts of energy from its galaxy’s stars to power computers, space flight, communication, or something we can’t yet imagine, fundamental thermodynamics tells us that this energy must be radiated away as heat in the mid-infrared wavelengths,” said Wright. “This same basic physics causes your computer to radiate heat while it is turned on.”
However, it was not until space-based telescopes like WISE were deployed that it became possible to make sensitive measurements of this radiation. WISE is one of three infrared missions currently in space, the other two being NASA’s Spitzer Space Telescope and the Herschel Space Observatory – a European Space Agency mission with important NASA participation.
WISE is different from these missions in that it surveys the entire sky and is designed to cast a net wide enough to catch all sorts of previously unseen cosmic interests. And there are few things more interesting than the prospect of advanced alien civilizations!
To search for them, Roger Griffith – a postbaccalaureate researcher at Penn State and the lead author of the paper – and colleagues scoured the entries in the WISE satellites database looking for evidence of a galaxy that was emitting too much mid-infrared radiation. He and his team then individually examined and categorized 100,000 of the most promising galaxy images.
And while they didn’t find any obvious signs of a Type II civilization or Dyson Spheres in any of them, they did find around 50 candidates that showed unusually high levels of mid-infrared radiation. The next step will be to confirm whether or not these signs are due to natural astronomical processes, or could be an indication of a highly advanced civilization tapping their parent star for energy.
In any case, the team’s findings were quite interesting and broke new ground in what is sure to be an ongoing area of research. The only previous study, according to the G-HAT team, surveyed only about 100 galaxies, and was unable to examine them in the infrared to see how much heat they emitted. What’s more, the research may help shed some light on the burning questions about the very existence of intelligent, extra-terrestrial life in our universe.
“Our results mean that, out of the 100,000 galaxies that WISE could see in sufficient detail, none of them is widely populated by an alien civilization using most of the starlight in its galaxy for its own purposes,” said Wright. “That’s interesting because these galaxies are billions of years old, which should have been plenty of time for them to have been filled with alien civilizations, if they exist. Either they don’t exist, or they don’t yet use enough energy for us to recognize them.”
Alas, it seems we are no closer to resolving the Fermi Paradox. But for the first time, it seems that investigations into the matter are moving beyond theoretical arguments. And given time, and further refinements in our detection methods, who knows what we might find lurking out there? The universe is very, very big place, after all.
The research team’s first research paper about their Glimpsing Heat from Alien Technologies Survey (G-HAT) survey appeared in the Astrophysical Journal Supplement Series on April 15, 2015.
Our civilization will need more power in the future. Count on it. The ways we use power today: for lighting, transportation, food distribution and even entertainment would have sounded hilarious and far fetched to our ancestors.
As our technology improves, our demand for power will increase. I have no idea what we’ll use it for, but I guarantee we’ll want it. Perhaps we’ll clean up the oceans, reverse global warming, turn iron into gold, or any number of activities that take massive amounts of energy. Fossil fuels won’t deliver, and they come with some undesirable side effects. Nuclear fuels will only provide so much power until they run out.
We need the ultimate in energy resources. We’ll want to harness the entire power of our star. The Soviet astronomer Nikolai Kardashev predicted that a future civilization might eventually harness the power of an entire planet. He called this a Type I civilization. A Type II would harness the entire energy output of a star. And a Type III civilization would utilize the power of their entire galaxy. So let’s consider a Type II civilization.
What would it actually take to harness 100% of the energy from a star? We’d need to construct a Dyson Sphere or Cloud and collect all the solar energy that emanates from it. But could we do better? Could we extract material directly from a star?
You bet, it’s the future!
This is an idea known as “stellar lifting”. Stealing hydrogen fuel from the Sun and using it for our futuristic energy needs. In fact, the Sun’s already doing it… poorly. Stars generate powerful magnetic fields. They twist and turn across the surface of the star, and eject hydrogen into space. But it’s just a trickle of material. To truly harness the power of the Sun, we need to get at that store of hydrogen, and speed up the extraction process.
There are a few techniques that might work. You can use lasers to heat up portions of the surface, and increase the volume of the solar wind. You could use powerful magnetic fields to carry plasma away from the Sun’s poles into space.Which ever way it happens, once we’ve got all that hydrogen. How do we use it to get energy? We could combine it with oxygen and release energy via combustion, or we could use it in our space reactors and generate power from fusion.
But the most efficient way is to feed it to a black hole and extract its angular momentum. A highly advanced civilization could siphon material directly from a star and send it onto the ergosphere of a rapidly spinning pet black hole.
Here’s Dr. Mark Morris, a Professor of Astronomy at UCLA. He’ll explain:
“There is this region, called the ergosphere between the event horizon and another boundary, outside. The ergosphere is a very interesting region outside the event horizon in which a variety of interesting effects can occur. For example, if we had a black hole at our disposal, we could extract energy from spinning black holes by throwing things into the ergosphere and grabbing whatever comes out at even higher speeds.”
This is known as the Penrose process, first identified by Roger Penrose in 1969. It’s theoretically possible to retrieve 29% of the energy in a rotating black hole. Unfortunately, you also slow it down. Eventually the black hole stops spinning, and you can’t get any more energy out of it. But then it might also be possible to extract energy from Hawking radiation; the slow evaporation of black holes over eons. Of course, it’s tricky business.
Dr. Morris continues, “There’s no inherent limitation except for the various problems working in the vicinity of a massive black hole. One can’t be anywhere near a black hole that’s actively accreting matter because the high flux of energetic particles and gamma rays. So it’s a hostile environment near most realistic black holes, so let me just say that it won’t be any time soon as far as our civilization is concerned. But maybe Type III civilizations so far beyond us that it exceeds our imagination won’t have any problem.”
A Type 3 civilization would be so advanced, with such a demand for energy, they could be extracting the material from all the stars in the galaxy and feeding it directly to black holes to harvest energy. Feeding black holes to other black holes to spin them back up again.
It’s an incomprehensible feat of galactic engineering. And yet, it’s one potential outcome of our voracious demand for energy.
It’s a big galaxy out there. Even the most skeptical scientist has to accept that if a civilisation like our own exists, then there’s a good chance we’re not the only one to have ever done so. When most people think about SETI (the search for extraterrestrial intellgence), they imagine someone like Ellie Arroway searching the skies for radio transmissions. But what about looking in other ways? Perhaps a highly advanced alien civilisation might build structures large enough for us to see. Continue reading “Hunting for Alien Megastructures”