If Aliens Looked at Earth from Far Away, What Might They See?
Whether aliens could detect our modern civilization depends on what signs they’re looking for—and, crucially, their distance from us
How far out into the cosmos would signs of our civilization reach? The answers might surprise you.
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So far astronomers have discovered nearly 6,000 exoplanets—worlds that orbit stars other than our sun. If that number already feels ridiculously large, you’d better brace yourself: through extrapolation, there could be hundreds of billions of planets in our galaxy alone. Some fraction of them will be like Earth, though at the moment we don’t yet know what that fraction is. Still, with a total that huge, even a small fraction can yield a lot of habitable planets.
Could they detect us?
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Phrased that way, in the most general sense, the answer is “yes.” By this I mean that there’s no physical reason why you couldn’t build an immense telescope, one far, far larger than any currently in existence, that would be capable of taking a detailed image of a planet from a great many light-years away. The engineering task may be considerable, but it’s not technically impossible. Then it might only be a matter of seeing city lights at night, for example, to confirm that aliens—that is, us, because we’d be alien to them—exist.
Actually, it may be even easier than that. A much smaller telescope need not resolve the planet; just observing it well enough to watch it get brighter and dimmer as city lights at night rotate into and out of view might be good enough. And that “smaller” telescope would only have to be, oh, let’s say, ridiculously huge instead of overwhelmingly so.
The reason to wonder about this, though, is that it flips the script on what’s usually asked, which is how we can detect them, given our current level of technology. We can’t know their level in advance, but we do know our own—so it makes sense to assume their tech is equivalent to ours and then to ask from what distance they could spot us.
A team of astronomers headed by Sofia Sheikh of the SETI Institute has run the numbers and published its results in the Astronomical Journal. (SETI stands for the search for extraterrestrial intelligence.) The researchers looked at various methods of detecting our various so-called technosignatures, and the answer unsurprisingly depends on which specific one any aliens would be looking for. Many of these ideas have been individually investigated before, but this latest analysis examines them collectively and consistently to arrive at some fresh insights.
One example of a technosignature is radio. Since its inception in the mid-20th century, SETI has focused on detecting artificial radio signals from space. Radio waves are easy to make and detect, and they can pass at the speed of light through interstellar space scarcely impeded by any gas and dust that might be in the way. That makes radio a nearly ideal carrier for galactic-range communication.
The astronomers divided radio signals into four categories: first, pointed but intermittent broadcasts to space, essentially “we are here” messages; second, intentional and persistent targeted signals sent to our planetary probes in deep space that continue on into the galaxy; third, persistent omnidirectional signals, such as “leakage” emissions from cell-phone towers, as well as radio and television stations; and fourth, signals from artifacts, such as low-power downlinks from our interplanetary probes.
Unsurprisingly, signals in the first category can be detected from the farthest away because the power involved in the transmission is highest. Sheikh and her colleagues estimate that these can be spotted at a staggering 12,000 light-years from Earth! That’s a maximum distance, but several billon stars lie in its volume. If you want to be found, this is probably the way to go.
The other methods don’t fare as well. For the second category, the maximum distance is more like 65 light-years, which still contains thousands of stars. The third category only gets out to four light-years, which isn’t even as far as the closest star to the sun. (That star, Proxima Centauri, is 4.25 light-years distant.) That jibes with recent research on radio emissions from cell-phone towers. The fourth one, which would include signals from our spacecraft, such as the Voyager 1 probe, has a detection limit of just under a light-year away. That actually surprised me, given how weak the signal is now, when the spacecraft is “only” about 25 billion kilometers away. Voyager 1’s 23-watt transmitter is already dimmed to less than a billionth of a billionth of a watt, as seen from our world!
Clearly radio is the method of choice for aliens looking for Earth. But there are other signatures.
One outcome of our modern civilization is an imprint on our atmosphere. Besides carbon dioxide, quite a few other chemicals have been dumped into our air by industry and other anthropogenic sources. Altering our planet’s climate is not great, to say the least, but it does make a signature detectable from space. And that signature could be especially obvious for an interstellar observer located along our solar system’s ecliptic, the plane of Earth’s orbit around the sun: from that perspective, they would see our planet pass directly in front of our star once every year, slightly dimming its light. This is called a transit, and it has been the most successful method so far for discovering exoplanets.
Such transits can also be used to remotely analyze a world’s air. As starlight (or in our case, sunlight) passes through a planet’s upper atmosphere, certain wavelengths of light will be absorbed by molecules there, creating a fingerprint of sorts that can be measured. We already do this for some transiting exoplanets now with the James Webb Space Telescope (JWST). And proposed future telescopes such as NASA’s Habitable Worlds Observatory are meant to scan the atmospheres of dozens of potentially Earth-like exoplanets that may exist around nearby stars (even if they don’t transit, as seen from our solar system!).
In their new study, the SETI Institute astronomers focused on the remote detection of nitrogen dioxide, or NO2, a conspicuous by-product of fossil-fuel burning. Given the current levels in our polluted air, they find that we could detect such a signature from a distance of 5.7 light-years. Only the Alpha Centauri system is within that range, which limits any aliens’ options for sniffing us out. Still, it’s an impressive technological achievement to be able to do this sort of search at all.
Most other types of technosignatures fare worse. A JWST clone perched somewhere in the vicinity of Neptune’s orbit could detect the infrared glow of heat that emanates from our cities, but farther out, that trail grows cold. At about 100 times that distance, the optical gleam of Earth’s city lights would fade to black—better but still far short of even our next nearest star.
Lasers are easier to detect and are already being tested by NASA and the European Space Agency right now for in-space satellite communication. Still, under reasonable assumptions, a laser’s beam of focused light would be too dim to detect from a distance of just under six light-years, which is not enough to be spotted even at Barnard’s Star, the second-closest star system to our own.
Phil Plait is a professional astronomer and science communicator in Virginia. His column for Scientific American, The Universe, covers all things space. He writes the . Follow him online.
Source: www.scientificamerican.com