The Fermi Paradox: Why Silence From Space Makes Sense
Brian Keating and Shawn Ryan unpack the Fermi Paradox — from cosmic scale to civilization lifespans — and why silence might be the expected answer.
Written by AI. Nadia Marchetti

Photo: AI. Ondine Ferretti
In 1950, Enrico Fermi sat down to lunch at Los Alamos with some colleagues and, somewhere between the soup and whatever physicists building the atomic bomb ordered for a main course, asked a question that science still hasn't answered: Where is everybody?
Seventy-five years later, it remains one of the most uncomfortable questions in science — not because we've looked and found nothing, but because we've barely looked at all. That distinction matters enormously, and it sits at the center of a recent conversation between cosmologist Brian Keating and podcast host Shawn Ryan on Keating's Into the Impossible channel.
The pair work through the Fermi Paradox with the kind of layered thinking the question deserves — not as a gotcha for UFO believers or a reassurance for skeptics, but as a genuine reckoning with what our silence might mean.
The Numbers Problem
Start with the scale. Keating lays it out plainly: our galaxy has roughly 100 billion stars. The observable universe contains roughly 100 billion galaxies. Multiply those together, add a rough estimate of planets per star, and you get somewhere around 10²⁴ planets — a number so large it stops feeling like a number and starts feeling like a philosophical provocation.
"And then you think, well, what if only 1% of them have life on it?" Keating says. "That's 10 to the 22nd power. It's an insane number."
The math points firmly toward a crowded universe. So why the silence?
One answer is almost embarrassingly straightforward: we can only detect civilizations that have technology capable of broadcasting across interstellar distances. The Drake equation — formulated by radio astronomer Frank Drake in the 1960s — tries to quantify exactly this. It's less a calculator than a framework for naming what we don't know: how many stars form planets, how many planets develop life, how much of that life develops intelligence, and how long those intelligent civilizations actually survive. Plug in optimistic numbers and the galaxy teems with neighbors. Plug in pessimistic ones and we might be alone in the observable universe. The equation doesn't resolve the paradox; it just maps the uncertainty with precision.
The Light-Speed Prison
Even setting aside whether other civilizations exist, Keating makes a point about detection that tends to get glossed over in popular treatments of this topic: we are, in practical terms, deaf and blind.
Voyager — humanity's most traveled object — has been traveling for decades and is only about one light-day from Earth. The nearest star is roughly four light-years away. That gap is not a rounding error. It means that any physical visit to another star system is, with current technology, not a generational project but a geological one.
Radio signals are faster, obviously — they travel at the speed of light. But that introduces its own humbling constraint. The 1936 Berlin Olympics produced what Keating describes as the first globally transmitted television signal to leak into space. That broadcast is now approximately 90 light-years out. Within that sphere, there are perhaps a few thousand stars, some of which may have planets. But even if one of those planets received the signal today and immediately replied, we wouldn't hear back for another 90 years. The round-trip physics alone imposes a timeline that makes casual cosmic conversation implausible.
"That is such a tiny, microscopic number," Keating says of the volume of space our signals have reached. "That's like a shot glass out of the Pacific Ocean in terms of how much the vastness of the universe is."
That image sticks with me. We have announced ourselves to a shot glass. We're expecting the ocean to write back. And we've been at this for less than a century.
The Self-Destruction Hypothesis
If the silence isn't about distance or detection, maybe it's about duration. Keating references a paper — discussed publicly by physicist Sabina Hossenfelder and others — suggesting that the average lifespan of a technological civilization may need to be around 5,000 years or less to account for the silence we observe. Five thousand years puts us barely past the construction of the Egyptian pyramids. It's not long.
The mechanism that keeps erasing civilizations, in this framing, is depressingly familiar. Keating notes that conflict operates at every scale of biological organization — from bacteria secreting toxins to establish territorial dominance, all the way up to nation-states deploying weapons of mass destruction. The pattern appears consistent across the full spectrum of life as we know it.
This brings us to the concept of the Great Filter — the idea, developed by economist Robin Hanson, that something in the chain from simple chemistry to galaxy-spanning civilization acts as a bottleneck, eliminating most candidates before they can make themselves known. The unresolved question is whether that filter lies in our past (which would be reassuring — we survived it) or in our future (which would not be). The silence doesn't tell us which.
Are They Watching, Unbothered?
Then there's the Zoo Hypothesis — the possibility that advanced civilizations are aware of us and have simply chosen not to intervene. Keating illustrates this with a characteristically grounded analogy: the difference between a zoo gorilla and a gorilla observed from a distance at a wildlife park. In the zoo, there's a sign asking you not to knock on the glass. At the wildlife park, you're so far away the glass is irrelevant. You observe without disturbing.
Maybe we're the gorillas. Maybe something is watching from the equivalent of the wildlife park — close enough to observe, far enough not to trigger any anxiety about being seen.
But Keating is skeptical, and his reasoning cuts straight through the romanticism of that idea:
"We might not be able to do anything for them. We might not provide any resources. They're going to eat us."
It's a blunt pivot from the gentle zoo metaphor to something considerably darker — and it captures the asymmetry that sits beneath a lot of optimistic contact scenarios. An entity capable of interstellar travel or observation would be so far beyond us technologically that the notion of mutual benefit becomes hard to model. An ornithologist, as Keating puts it, needs the birds far more than the birds need the ornithologist. And birds, crucially, don't care whether you study them.
What the Silence Actually Tells Us
Here's what I keep returning to, after sitting with this conversation: the Fermi Paradox is routinely framed as a mystery demanding an extraordinary answer — a Great Filter, a dark forest of predatory civilizations, a simulation, a zoo. But Keating and Ryan's discussion keeps pulling back to something more basic. Our detection capability is genuinely primitive. Our signals have reached a vanishingly small fraction of the galaxy. The civilizations that could contact us may have come and gone before our sun formed, or may not yet exist, or may exist on timescales that make 5,000-year technological civilizations look like mayflies.
"We will not be able to find aliens unless they send us information or come and visit us," Keating says. It sounds obvious. It isn't. It's actually a rigorous statement about the structural limits of SETI as currently practiced.
None of this means they're not out there. Keating is careful about that. The absence of evidence within our shot-glass-sized corner of the Pacific is not evidence of absence across the ocean. Even researchers deeply invested in the search — Keating cites Harvard astronomer Avi Loeb as an example — stop short of claiming definitive proof of anything, in either direction. That epistemic honesty is rarer than it should be in this conversation.
The Nobel Prize digression Keating takes near the end of the conversation — about Alfred Nobel reading his own premature obituary in a Paris newspaper in 1888, horrified by the legacy it described, and redirecting his fortune accordingly — is ostensibly about self-reinvention. But it lands differently in context. Nobel looked at what the world would remember him for and decided to change the ending. The Fermi Paradox, at its most uncomfortable, asks whether civilizations get the chance to do the same.
Maybe the silence is the answer. Maybe it's just the distance. Maybe it's both.
By Nadia Marchetti, Unexplained Phenomena Correspondent
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