[ExI] They're Made out of Meat

Wed May 27 12:34:13 UTC 2026

On Tue, May 26, 2026 at 12:53 PM Jason Resch via extropy-chat <
extropy-chat at lists.extropy.org> wrote:

*> As to the size of the total universe (which includes the parts we cannot
> see) our leading cosmological theories say that it is infinite, which means
> there is not only other intelligent life out there but exact duplicates of
> earth, our solar system and even the Milky Way. Unfortunately this doesn't
> help answer the question of how near or far the closest intelligent life is
> to us, but it at least tells us that we're not alone in this universe
> (though we might be alone in the observable universe).*

*Actually, although we can't calculate the minimum distance we'd need to go
in an infinite universe to find intelligent life, we CAN calculate the
maximum distance we'd need to go, that's because if we assume that
spacetime is not continuous but is limited by the Planck length and the
Planck time, then there are only a finite number of ways that matter can be
arranged, so matter configurations must repeat. Physicist Max Tegmark
figures that a duplicate of our exact observable universe must exist about
10^10^115 meters away, that's a thousand trillion googolplex meters. This
is without even taking Hugh Everett's Many-Worlds idea into consideration,
or the eternal inflation idea, or the string theory landscape idea.  *

*Parallel Universes
<https://space.mit.edu/home/tegmark/PDF/multiverse_sciam.pdf>*

*John K Clark*
5th

>
> On Tue, May 26, 2026, 10:39 AM BillK via extropy-chat <
> extropy-chat at lists.extropy.org> wrote:
>
>> On Mon, 25 May 2026 at 19:41, John Clark <johnkclark at gmail.com> wrote:
>>
>>> <snip>
>>> *And that is one reason why I have never been impressed with the
>>> fine-tuning argument. Our universe may be a rare winner, but it's not a
>>> unique winner. *
>>> *John K Clark*
>>> --------------------------------------
>>>
>>
>>
>> I asked Gemini to discuss the point that our universe was so enormous
>> *because* creating intelligent life was so difficult.
>>
>
> It depends what you mean by the size of the universe. If what you mean is
> the size of the observable universe (~46 Gly radius) then that size is a
> direct consequence of how long it takes intelligent life to evolve. Because
> it took billions of years for us to evolve since the big bang, the
> observable universe must appear to us to be billions of light years across.
>
> As to the size of the total universe (which includes the parts we cannot
> see) our leading cosmological theories say that it is infinite, which means
> there is not only other intelligent life out there but exact duplicates of
> earth, our solar system and even the Milky Way.
>
> Unfortunately this doesn't help answer the question of how near or far the
> closest intelligent life is to us, but it at least tells us that we're not
> alone in this universe (though we might be alone in the observable
> universe).
>
> Jason
>
>
>
> Gemini produced a fascinating story that implied that the Fermi Paradox is
>> because Humanity could indeed be alone in this universe.
>> Full Report below.
>> BillK
>>
>> Gemini 3.5 Flash (Extended Thinking) -
>>
>> Your insight aligns perfectly with a profound argument in modern
>> cosmology. You are essentially framing the universe as a *massive
>> parallel processing supercomputer* running billions of trillions of
>> chemical and biological experiments simultaneously.
>>
>> If the probability of intelligent life emerging on any single planet is
>> infinitesimally small, a universe containing only a few galaxies would
>> almost certainly remain completely sterile. To guarantee at least one
>> "winner" in the cosmic lottery, the casino has to be unimaginably vast.
>>
>> This perspective bridges the gap between physics and evolutionary biology
>> through what is known as the *Anthropic Principle*, and it explains why
>> the sheer emptiness and scale of the cosmos is not a design flaw, but a
>> structural feature required for us to be here to witness it.
>> 1. The Physics Link: Why Age Equals Size
>>
>> In 1961, the physicist Robert Dicke pointed out a fundamental constraint
>> that connects the size of the universe directly to the existence of
>> physicists.
>>
>> Under the laws of our universe, you cannot have a universe that is both
>> *old* and *small*. Because space has been expanding since the Big Bang,
>> a universe’s physical size is a direct function of its age.
>>
>>    -
>>
>>    *The Stellar Bottleneck:* To get carbon, oxygen, and iron, you have
>>    to wait for the first generation of massive stars to live, die, and
>>    explode. To get a stable rocky planet, you have to wait for those heavy
>>    elements to coalesce into a secondary star system. This cosmic
>>    manufacturing process takes billions of years.
>>    -
>>
>>    *The Expansion Equation:* By the time gravity and nuclear physics
>>    have cooked up the chemical ingredients for life, the universe *must*
>>    have been expanding for roughly 14 billion years.
>>
>> Because it expanded at that rate for that long, the observable universe
>> *had* to grow to its current size of roughly 93 billion light-years
>> across. Its vastness is a mathematical byproduct of the time required to
>> build a single carbon atom.
>> 2. The Biological Link: The "Hard Steps" Model
>>
>> This is where your "trial and error" premise comes into play. In 1983,
>> astrophysicist Brandon Carter introduced the *"Hard Steps" model*, which
>> attempts to calculate the mathematical probability of intelligent life
>> evolving before its host star dies.
>>
>> If the transition from raw chemistry to a technological civilization
>> requires passing through several incredibly difficult evolutionary
>> bottlenecks, each step acts as a filter.
>>
>> Consider the historical "lottery tickets" our own planet had to scratch:
>>
>>    1.
>>
>>    *Abiogenesis:* Transitioning from organic soup to a self-replicating
>>    molecule (RNA/DNA).
>>    2.
>>
>>    *The Eukaryotic Leap:* Two primitive cells merging into a complex,
>>    compartmentalized cell (which happened only *once* in Earth's
>>    history, via a bizarre endosymbiotic fluke).
>>    3.
>>
>>    *Multicellularity:* Cells learning to coordinate rather than compete.
>>    4.
>>
>>    *Encephalization:* Developing high-energy, complex brains capable of
>>    abstract thought and tool use.
>>
>> If each of these steps is a wildly improbable "sampling error" in the
>> genetic timeline, the odds of a single planet successfully clearing all of
>> them might be 1 in a trillion, or 1 in a septillion.
>> 3. The Universe as a Massively Parallel Roll of the Dice
>>
>> If the odds of intelligent life developing on a habitable planet are 1 in
>> 10^22, then a small universe with only a few billion planets will almost
>> always result in total failure. The "trial and error" experiments will all
>> return a null result.
>>
>> By scaling the universe up to contain an estimated *10^24 stars* (and
>> likely just as many planets), the laws of physics essentially purchased
>> enough lottery tickets to overcome the statistical impossibility of the
>> biological bottlenecks.
>>
>> The universe isn't vast because we are insignificant; the universe is
>> vast because it needed to run an astronomical number of concurrent, failed
>> experiments just to hit the jackpot once.
>>
>> The Consequence: Cosmic Solitude
>>
>> This framework cleanly reframes the *Fermi Paradox* (the question of why
>> we don't see signs of interstellar alien civilizations).
>>
>> If the universe's scale is exactly matched to the low probability of the
>> "Hard Steps," then the expected number of intelligent civilizations per
>> observable universe might be very close to *one*. We might look out into
>> a terrifyingly quiet, empty universe because the mathematical machinery
>> required to produce even a single technological species demands an entire
>> cosmic horizon's worth of space and time to succeed.
>>
>> If this "parallel processing" model is correct, it suggests our existence
>> is a highly localized statistical fluke that exhausted the universe's
>> creative margin.
>>
>> ---
>>
>
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