There are **100,000 Earth-like planets capable of intelligent life ...
Here's a couple of recent links, somewhat zany, in different direct...
Enrico Fermi was an Italian-American physicist. He was awarded the ...
Travelling to distant Galaxies to meet other intelligent civili...
**Fermi is famous for his guesstimations** and his impressive abili...
### Where is everybody? *"So there are 100 Earth-like planets in...
The Drake equation provides an estimate of the number of communicat...
“WHERE
I EVERYBODY
A NACCOUNTO FERMI
QUESTI
b
EriM Jon
ABSTR
I
Fermi’s
famouquestion ocentrt debaa bt prev
o fextraterrestriacivilizatioaroduria luncconve
withEm iKonopinskiEdwaTellea nHerbY oi t s u
o f1950Fermicompanioo thad ah aprovaccoo t
incident.
Parto fthecurrentdebateabouttheexistencea nprevaleno extraterre
conc
interstellartravelandsettlement.
1-3I n1975MichaeH aargut h
interst
traw o
b efeasiblefora technologicallyadvancedcivilizatioa nthaa migratwouf it G a
i na fewmillionyears.4Sincethatintervali shorcomparewitt ha go t hGalh t h
concludedthattheabsenceo fsettIerso revidenco theiengineerprojei t S o
Systemmeantthattherearen ocxtraterrestrials.
Newman,Sagan,andShklovski2”5recallthaa legeno scien
say
t hEnrF ea s
thequestion,“Wherearethey?duringa visit L oAlamodurit hSecW oW o
shortlythereafter.Fermi’squestionhasbeenmentionei severothrecpublicb
historicalbasisfortheattributionhasnotbee
established
Thant t hexcelmemo
HansMark,whohadhearda retellinga t
Los
Alamoi t hearl1950w nowlmoF e
didmaketheremarkduringa lunchtime
conversation
abou195H icompanw e
E m
Konopinski,EdwardTeller,andHerbertYorkA lthrehavprovidaccouo t inci
W ebeginwithKonopinski: Ihaveonlyfragmentarrecollectiabot hocca. . . I
d ohavea fairlyclearmemoryo fhowthediscussioo extra-terrestrg ostarted
Enrico,Edward,HerbYork,andI werewalkingt Iunca FullLodg
“WhenI joinedtheparty,I foundbeingdiscusseevidenaboflyisaucT h
immediatelybroughtt om yminda cartoonI h arecentlseei t hN eYork
expla
whypublictrashcansweredisappearing
from
t hstreeto N e
Yor
CitT hN Y op a
weremakinga fussaboutthat.Thecartoonshowewhaw aevidena flysausiti
thebackgroundand,streamingtowardit,‘littlgreemen(endoww iantencar
thetrashcans.MoreamusingwasFermi’scommentthai w aa verreasonthes ii
accountedfortwoseparatephenomena:t hreporto flyinsaucea w ea
t h
disapp
o fthetrashcans.Thereensueda discussiona t whethet hsaucecousome
exc
t
speedo flight.
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Tellerremembers:“Myrecollectiono ft heveninvolviFer. . . i cleb o npar
T obeginwith,I wasthereattheincident.I believi occurrshortaftt he o t w o
a visito fFermit otheLaboratory,which
quite
possiblmighhavb edura sum
IrememberhavingwalkedoverwithFerma nothert t hFullLod
f o
lunW h
w ewalkedover,therewasa conversationwhicI believt hav
bee
quibria supe
o na subjectonlyvaguelyconnectedwithspactravelI hava vagrecollecw hm
notb eaccurate,thatw etalkedaboutflyingsaucera nt hobviostatemt ht
fly
saucersarenotreal.I alsorememberthatFermexplicitlraist hquesti
a n
I t hh
directedi ta tme,‘Edward,whatd oyouthink?H oprobabi i
tha
witht hn et y e
w eshallhaveclearevidenceo fa materialobjecmovinfastthalighI remet hm
answerwas10-6.Fermisaid,‘Thisi smucht olowT hprobabili m ol it per
(thewellknownfigurefora Fermimiracle.)
Konopinskisaysthath edoesnotrecallt hnumericavalue“excet ht hcha
rapidlya sEdwardandFermibouncedargumentso feacothe
Tellercontinues:“Theconversation,
according
t m memorw ao nvaguconn
withastronauticspartlyo naccounto fflyingsaucermighb d ut extraterrepeo
(hereI believetheremarkswerepurelynegative)partlbecauexceedligvelow o
makeinterstellartravelonedegreemorereal
“WethentalkedaboutotherthingswhichI d n orememba nmayapproxie i
o fu ssatdowntogetherforlunch.
Konopinskia nYora rquicertt ht hw e
o n
fouro fthem.
2
“Itwasafterw ewerea ttheluncheon
table,Konopinsk
recall“thFersurpu
withthequestion‘butwherei severybody?I w ah iw ao puttii t hd rlauf ru
York,whodoesnotrecallthepreliminaryconversatioo t h
wal
t FulLodd o
rememberthat“virtuallyaproposo fnothingFermsaid‘Dony oe vwonw h
everybodyis?Somehow. . .
w eallknewh meanextra-terrestria
Tellerremembersthequestioni nmucht hsamway“Thdiscussh a
noth
t d w
astronomyo rwithextraterrestrialbeings.I thini w asomdown-to-etopT hi t
middleo fthisconversation,Fermicameo uwitt hquitunexpecquest‘Whi
everybody?. . .
Theresulto fhisquestionw ageneraIaughterbecao t h
stra
f a
t h
i
spiteo fFermi’squestioncomingfromthecleablueeveryboarout htabseet
understanda toncethath ewastalkingabout
extraterrestria
lif
Id onotbelievethatmuchcameo fthisconversationexceperhaa statet ht
distancest othenextlocationo flivingbeingsmaybvergreaa nthaindea f a o
galaxyi sconcerned,w earelivingsomewherei t h
sticks
f aremovf rt h
metrop
areao fthegalacticcenter.
YorkbelievesthatFermiwassomewhatmorexpansiva n“follou w ia sero
calculationso ntheprobabilityo fearthlikeplanetst h
probabili
o l igiva eart
probabilityo fhumansgivenlife,thelikelyrisa n
duratio
o higtechnola s o H
concludedo nthebasiso fsuchcalculationsthaw ought hav
bee
visil oa a m
timesover.A SI recall,h ewento nt oconcludethat hreasow hadnb evisim ib
thatinterstellarflighti simpossible,or,
i f
i i possible
alway
judgt b n ow ot eff
o rtechnologicalcivilizationdoesn’tlastlonenougf oi t happe Y oconfet b e
hazyabouttheselastremarks.
I nsummary,Fermididaskthequestion,a nperhapn osurprisinisss tdeb
todaywereparto fthediscussion.Certainly,t hlino argume
tha
Y orememb e
familiara decadelatera stheDrake-Greenbank
Equation.6
A finalpoint:thedateo ftheconversation.Yori cleareo t hdat Tconverw
eitheri nthesummero f1950,1951,o r
1952,
ver
probabl
195a nt opla. . . w hI
wasvisitingIASLi nconnectionwiththe
forthcoming
Greenhoutests—specift
Georgeshot. TheGeorgetestoccurred
o n
M a8 1951suggesti1 9datSurv
correspondencefromthetimeindicatesthaFermw aa annusummvisidurt y e
i nquestion.Unfortunately,attendanceandtraverecordf othoyeah ab edest
However,w ehavetheevidenceo fthecartoonKonopinsk
mention
Drab A lD ui w
publishedi ntheMay20,1950,issueo f
TheNewYorkerI
seem
qui
proba
t ht
incidento fFermi’squestionoccurredi nt hsummeo 1950
I a mgratefult oHansMarkandt othethreesurvivinparticipaf otheaccouT h
accounts,togetherwithm yletterso finquiry,a r
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LosAlamosNationalLaboratory
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DearErie
M yrecollectiono ftheeventinvolvingFermithay owrott m aboi cleb
onlypartial.
T obeginwith,I wastherea ttheincident.I believi occurr
short
aftt e
o fthewaro na visito fFermit otheLaboratory,whicquitpossibmigh ab e
duringa summer.
1 rememhavingwalkedoverwithFermia nothert t hFullLodf o
lunch.Whilew ewalkedover,therewasa conversationwhicI beliet h ab eq u
briefandsuperficialo na subjectonlyvaguelyconnectewitspac
trave
I h aa
vaguerecollection,whichmaynotb eaccurate,thaw talkeaboflyisauca
theobviousstatementthattheflyingsaucersa rn orealI als
rememb
t h
Fer
explicitlyraisedthequestion,andI thinkh e
directed
i a m e~~Edwaw hd
y o
think.Howprobablei si tthatwithinthenextt eyearw shalhavcle
evide
o
a materialobjectmovingfasterthanlight?!tI remembetham answw a~llO
Fermisaid,“Thisi smuchtoolow.Theprobabilityi morlikt epercen( tw e
knownfigurefora Fermimiracle).
ThisincidentI haveclearlyi nmindandI believi w ao t hsamoccasw h
theotherquestionarosewhichyouhavementioned.ThilattepoinhowevI a n
certainof.
A tanyrate,theconversation,accordingt m memoryw aonlvagucome
withastronauticspertlyo naccounto fflyingsaucermighb d ut extraterre
people(hereI believetheremarkswerepurelynegative)partlbecauexceel i
velocitywouldmakeinterstellartravelone
degree
morreal
W e
t htalkabooththiwhichI d n oremembea nmay
approxim
eighto fu ssatdowntogetherforlunch.Thediscussioh anothit d w iastro
o rwithextraterrestrialbeings.I thinki twassomdown-to~artopi
Then,i nthemiddleo fthisconversation,Fermcamo uwitt hqui
unexpe
question“Wherei severybody?llWhatI a msureo i thayouquot Ty oa rrig
thenwherei severybody?”,i swrong.Fermi
did
n ot ih iquestit a nconvers
whichwasthengoingon.Theresulto fhisquestionw a
genera
laughtbecao t
strangefactthati nspiteo fFermi%questioncominfrot h
clea
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aroundthetableseemedt ounderstanda toncethah w atalkiabo
extraterre
An.EquslQqwtmua-wdc.afmns.~ammuiwm
~945W*Tde@ins(415)422-110Twx910-3WS3391L
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Dr.EricM .Jones
Page2
August13,1984
life.I
d n obelit hm uc ao t h
conver
e xp ea s t
that hdistant t hn eloca
o flivinbeingm ab vergrea n
tha
indeed,a sfara sourgalaxyi sconcerned,w a rlivinsomewhei t hsticf
removedfromthemetropolitanareao fthegalacticenter
I canfullyconfirmthatthequestionw abroughu b Fermi FullLoda
lunch,probablybefore1950.
Hopingthatthisi stheinformationyouwanted
Witbesregar
Edwar
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P.S.Goodo fyout oaska
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Therei a storyaboutFermi’s
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i L oAlsmothai makt
roundsi ntheSETI(searchforextraterrestrialintelligencommun
whichhas,unfortunately,littleaolidbasis
I w aSagw hfiru s
i ti nhisbookwithShklovski,butCarlh a
forgotte
wheo f rw hh
heardit.
HansMarkhasgivenm ea
secondhand
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h eheardi ntheearlyfifties;EdwardTelleh aalsprovidh ir e
ollectiono ftheevent.
Severalpeoplehavsuggestthay omigb
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T hw at hstoi b et ot hd ai t t lun
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o earthplant probao l ig ia e at
probabio humg il it l i
r i
a d uo h
technola na o H conco t b ao s cal
t hw ougt h ab evisl oa a m t io A
I recah w eo t conct ht r ew h ab
viaimigb t hintersf li impoo i i
i poaaialwjudt b n w ot e fo
tech
civilizdoesl al oenof i t h a
I a m
haziabothel arem
a o
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REFERENCES
1 .M .H .HartandB .Zuckerman(eds.),
Ext ra t errest ri
Wbe
A r
T b(PergP r
Inc.,NewYork,1982),p .182.
2 .W .T .NewmanandC .Sagan,Ic a r u4 6293-3(1 9 8
3 .E .M .Jones,Ic a r t z s 4 6 ,328-336(1981).
4 .M .H .Hart,
Qua rterly Journa l
oftbeRoyalAstronomicaZSo
1 6128-(19
5 .I .S .ShklovskiandC .Sagan,
In t e l l ig eLz Yi t bUnive(Holden-
Inc
S Fran
1968),p .448.
6 .W .Sullivan,
WeAreNotAlone(Mc G r a w -HBooCo.NewYor196
7 .F .D .Drake,“TheRadioSearchforIntelligentExtraterrestriLifei Cur
Asp
o
Exobiology,G
MamikunianandM .H Brigg(eds.,JePropulsLaboratech
report32-428(1965),pp.323-346.
1

Discussion

### Where is everybody? *"So there are 100 Earth-like planets in the Universe for every grain of sand in the world. Think about that next time you’re on the beach."* There are 100,000 Earth-like planets capable of intelligent life in our Galaxy, the Milky Way. How come we have never made an "encounter" with extraterrestrial life? Any ideas? *(feel free to comment below)* Enrico Fermi was an Italian-American physicist. He was awarded the Nobel Prize in Physics in 1938. He is the creator of the world's first nuclear reactor and worked on the Manhattan project during WW II. Fermi is famous for his back of the envelope calculations and his impressive ability to estimate the magnitude of answers to complex problems. A great example of this ability is this article he wrote guesstimating the power dissipated by the explosion of the first atomic bomb with simple sheets of paper: **[My observations during the explosion at Trinity](http://fermatslibrary.com/s/my-observations-during-the-explosion-at-trinity)** ![Fermi Teller](https://i.imgur.com/16Spiv9.jpg) *Edward Teller (left) with Enrico Fermi in 1951.* You can learn more about Fermi here: [Enrico Fermi](https://en.wikipedia.org/wiki/Enrico_Fermi) **Fermi is famous for his guesstimations** and his impressive ability to estimate the magnitude of answers to complex problems. He had an uncanny ability to take problems apart and describe them in simple terms. Fermi tried to inculcate this facility in his students. Some famous Fermi questions: - How many grains of sand are there on the world’s beaches? - How many piano tuners are there in Chicago? - How far can a crow fly without stopping? - How many atoms of Caesar's last breath do you inhale with each lungful of air? The Drake equation provides an estimate of the number of communicating civilizations in the Milky Way. The equation is composed of 7 terms. The first 6 are used to compute the rate at which intelligent civilizations are being created and the final term identifies how long each lasts on average as a broadcasting civilization. The Drake equations can be written as: $$ N = R × f_p × n_e × f_l × f_i × f_c × L $$ where: - N is the number intelligent civilizations that are broadcasting their presence - $R$ is the yearly rate at which stars form in the Galaxy - $f_p$ is the fraction of stars that possess planets - $n_e$ is the number of planets with environments suitable for life - $f_l$ is the fraction of suitable planets on which life actually develops - $f_i$ is the fraction of these planets on which life develops intelligence - $f_c$ is the fraction of intelligent life-forms that develop a culture capable of interstellar communication - $L$ is the time that such a culture will devote to communication There is a lot of uncertainty associated with the parameters and the Drake equation can give a very wide range of values, depending on the assumptions and the values. To learn more about the Drake equation: - [Drake equation tutorial](http://www.astrodigital.org/astronomy/drake_equation.html) - [SETI - The Drake Equation](http://www.seti.org/drakeequation) - [Drake equation](https://en.wikipedia.org/wiki/Drake_equation) Here's a couple of recent links, somewhat zany, in different directions regarding Fermi's paradox: Dissolving the Fermi Paradox (Future of Humanity Institute, Oxford) https://spectrum.ieee.org/tech-talk/computing/hardware/computing-and-the-fermi-paradox-a-new-idea-emergestheyre-all-asleep Runaway consumerism explains the Fermi Paradox https://www.edge.org/q2007/q07_print.html#miller What Donald Trump Teaches Us About the Fermi Paradox http://nautil.us/blog/what-donald-trump-teaches-us-about-the-fermi-paradox There are **100,000 Earth-like planets capable of intelligent life in our Galaxy**, the Milky Way. (*see guestimations below*) ### Where is everybody? How come we have never made an "encounter" with extraterrestrial life? Any ideas? 🤓 🤔 (*Feel free to comment below*) --------------------- In this matter I tend to go with the hypothesis that there's extraterrestrial life in other places in the Universe but we just haven't been able to detect it. It's also very unlikely that we are the most developed civilization out there so I agree with Freeman Dyson's theory that a sufficiently developed species will try to harness a large part of the energy produced by a star by enclosing it in some sort of shell - [a Dyson Sphere](https://en.wikipedia.org/wiki/Dyson_sphere). This will shift the energy emission spectrum around the star towards infrared which in theory should be detectable at a relatively long distance. We just need to map a large portion of sky for a long enough time to capture the signals from these spheres :) Most likely because there's a more advanced civilization that is able to simulate a Universe where we are the single intelligent species (also called the Planetarium hypothesis). This grew stronger in me after reading [Nick Bostrom's paper](http://fermatslibrary.com/s/are-you-living-in-a-computer-simulation) that has been featured a few months ago. It seems to depend a lot on how mobile everyone is, or how long they've been sending out messages. Are all 100,000 civilizations whizzing around in FTL ships or just sending signals out at *only* the speed of light? Assuming the latter makes the situation a lot harder. If we imagine sending ships in all directions looking for a planet with intelligent life, we can estimate the number of planets we would need to visit as a binomial random variable. If we visit N planets, where we expect $\lambda = \frac{1e5}{1e11}$ planets to harbour intelligent life, the probability of finding intelligent life is: $p = 1 - Bino[0,N,\lambda] = 1-(1-\lambda)^N$ Alternatively, $N = \frac{\text{log}(1-p)}{\text{log}(1-\lambda)}$ So now we know how many planets we have to visit, how far do we have to travel? If the Milky Way is approximately a 150k-light year diameter disk, with all the planets equally spaced out and us in the center (all not true, so our number may be generous to us), then the radius of our search from Earth must be: $R\approx\sqrt{\frac{N}{N_{total}}}\frac{150}{2}\text{kly} = \sqrt{\frac{\frac{log(1-p)}{log(1-\lambda)}}{1e11}}75\text{kly}$ $R\approx\frac{0.75}{\sqrt{10}}\sqrt{\frac{log(1-p)}{log(1-\lambda)}}$light years You can plot this to see how the distance changes with your confidence of finding life. Searching in all directions is pretty similar to sending a message into space. The earliest man-made radio signals from about 150 years ago have a 1-in-3 chance of reaching an intelligent civilization (if they're still strong enough). You need to travel 200 light years in all directions to have a 50/50 likelihood. Being 99% sure requires a 510 light year search radius. Unless our neighborhood aliens are mobile and able to come find us, or very old and have been transmitting information for a long time (which isn't so crazy), it seems pretty unlikely that we'll find them soon. Travelling to distant Galaxies to meet other intelligent civilization would take billions of years and is practically impossible. So let's focus on our home Galaxy, the Milky Way. **How many intelligent civilizations are there in our Galaxy?** We can *guesstimate* the number of planets harboring intelligent life in the Milky Way: - there are **$100 \times 10^{9}$ Stars in our Galaxy** ⭐️ - if 5% of all stars are Sun-like then there are **$5 \times 10^{9}$ Sun-like stars in our Galaxy** ☀️ - if 20% of all Sun-like stars are orbited by an Earth-like planet then there **$10^{9}$ Earth-like planets** 🌎 - if only 1% of these Earth-like planets harbor life then there would be **$10\times 10^{6}$ planets with life in the Milky Way** 🐋 - if 1% of those develop intelligent life then **there are 100,000 intelligent civilizations in our Galaxy** 🤓 If there are 100,000 intelligent civilization in the Milky Way, then the question arises **where are all the Aliens?** This is the **Fermi Paradox**. You can learn more about the Fermi Paradox: - [Fermi Paradox](https://en.wikipedia.org/wiki/Fermi_paradox) - [SETI - The Fermi Paradox](https://www.seti.org/seti-institute/project/details/fermi-paradox) - [Wait But Why - The Fermi Paradox](https://waitbutwhy.com/2014/05/fermi-paradox.html)