Where are they (E.T.I.) anyway?

Similar documents
The Search for Extraterrestrial Intelligence

The Jamie Drake Equation

The Search for Extraterrestrial Intelligence

Lecture #26: Searching for Other Civilizations. SETI = Search for Extra-Terrestrial Intelligence Searching for signals from other beings

Primary KS1 1 VotesForSchools2018

The Search for Extraterrestrial Intelligence (SETI)

AST 205. Lecture 23. December 8, 2003 SETI, Interstellar Travel and the Fermi Paradox. Assignments for week of Dec 8

Lecture 40: SETI. Astronomy Winter This lecture is about SETI, the Search for Extra- Terrestrial Intelligence.

Extraterrestrial Life Group Discussion

Searching for Life: Chapter 20: Life on Other Worlds. Life in the Universe. Earliest Fossils. Laboratory Experiments.

Copyright 2009 Pearson Education, Inc. Life in the Universe

What is Astrobiology?

Lecture #26: Plan. Cosmology: Search for Intelligent Life in the Universe. The Great Unanswered Questions (cont d)

The Quest for Extraterrestrial Signals. Ron Maddalena National Radio Astronomy Observatory Green Bank, WV

Lecture Outlines. Chapter 28. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Are We Alone? Dreams of Life Elsewhere

Search Strategies. Basic Problem: where to look? Possible Scenarios Powerful, omnidirectional beacons

Chapter 24 Life in the Universe. Earliest Life Forms. When did life arise on Earth? Fossils in Sedimentary Rock. Fossils in Sedimentary Rock

Measuring Distances to Galaxies. Galaxies in Motion. Hubble s Law. Galaxy Redshifts. Type Ia Supernovae. Supernovae are Good Standard Candles

! Communication, 2.!

Sociological Factors. Putting it all Together: How far away? How many stars to search?

Search Strategies. Basic Problem: where to look? Possible Scenarios Powerful, omnidirectional beacons

Young Solar-like Systems

Chapter 24: Life in the Universe

PH104 Lab 2 Measuring Distances Pre-Lab

Nov 17, 2003 Astronomy 100 Fall _tips_ html

The evolution of a Solar-like system. Young Solar-like Systems. Searching for Extrasolar Planets: Motivation

Part I---Introduction: planets, and habitable planets

The Physical Basis of Life

Simon P. Balm Astro 5 Test #3 Sample Questions

Final Exam. 12:30 2:30 pm, Friday, May 6th, in this room. Written Questions covering all the material from this semester.

Lab 4. Habitable Worlds: Where Should NASA Send a Probe to Look for Life?

ASTR 380 The Drake Equation

NSCI EXTRASOLAR PLANETS (CONTINUED) AND THE DRAKE EQUATION. Dr. Karen Kolehmainen Department of Physics, CSUSB

Extrasolar Planets What are the odds?

THE SIZE AND SCALE OF THE UNIVERSE

Ultimate Events. Galaxy clustering in ever deeper surveys. Models of universe and its fates

WHERE ARE THEY? The Fermi Paradox

Physics can only take us so far!

Star. Planet. Chapter 1 Our Place in the Universe. 1.1 A Modern View of the Universe Our goals for learning: What is our place in the universe?

Decoding an Extraterrestrial Message

ASTR 380 The Drake Equation

CONNECTIONS to the COSMOS: the search for life beyond Earth

Homework 13 (not graded; only some example ques!ons for the material from the last week or so of class)

(Astro)Physics 343 Lecture # 14: the Search for Extra Terrestrial Intelligence


Galaxies and The Milky Way

It is a very human trait to wonder where we are in this universe. Usually, the only hint of the vastness of the universe comes at night.

Astrobiology: The Semester in Review

Life on Other Worlds: The Drake Equation Author: Meagan Morscher GK-12 Reach for the Stars Fellow, Northwestern University

The Search for Extra-terrestrial. Is there anybody out there?

Intelligent Life in the Universe

Astronomy 330 HW 2. Outline. Presentations. ! Kira Bonk ascension.html

Cosmology Overview (so far): Cosmology Overview (so far): The Age of the Universe. The Big Bang. The Age of the Universe

-- Lewis Carroll, Alice in Wonderland

January December. Journey Back in Time. Review: The ScienCfic Search for Origins How did our world come to be? 4/27/10

ABCs of Space By: John Kraus

ASTR : Stars & Galaxies (Spring 2019)... Study Guide for Midterm 1

4 Decoding the Arecibo Message

ASTRONOMY 202 Spring 2007: Solar System Exploration. Instructor: Dr. David Alexander Web-site:

Start with known facts and reasonable guesses. More on order of magnitude Astronomy How many piano tuners are there in Boulder County?

Our Place in the Universe (Chapter 1) The Structure and Size of the Universe

Astronomy 1504 Section 10 Final Exam Version 1 May 6, 1999

What s the longest single-shot exposure ever recorded of any object or area of space by Hubble?

ASTR 380: Life in the Universe - Astrobiology Professor Sylvain Veilleux

Detection of Earth-like planets

The Physical Basis of Life. The Origin of Life on Earth. Information Storage and Duplication

Sex in Space: Astronomy 330 TR Noyes Laboratory 217. Outline. Discussion Class

Other migration processes. New transiting hot Jupiters from last week. First success from CoRoT. Kozai mechanism

Planets, Stars and Galaxies Section 1 Mon. & Weds. 3:35-4:50. Prof. Todd Adams. Welcome! Department of Physics Florida State University

Ari Schjelderup David Schaffer PHYS /30/11 The Big Bang Theory

HOW COMMON IS LIFE IN THE UNIVERSE?

SOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES

MITOCW watch?v=gfbgoivnyuw

Bell s spaceship paradox

Planet discovery accounced Feb. 3

N = R *! f p! n e! f l! f i! f c! L

Section 3- The history and future of space exploration

TAKEN FROM HORIZONS 7TH EDITION CHAPTER 1 TUTORIAL QUIZ

12/5/ Life on Earth. Chapter 19: Life in the Universe. When did life arise on Earth? Earliest Life Forms. Important Stuff (Section 001)

Notes 9: Extrasolar Planets and Exo-biology

AST 309 part 2: Extraterrestrial Life. The Search For Extraterrestrial Intelligence (SETI)

Life on a New Planet

[02] Quantitative Reasoning in Astronomy (8/31/17)

what scientist believe happened to form the universe, and it is called the Big Bang Theory.

Phys 214. Planets and Life

Alternative Standard Frequencies for Interstellar Communication. C Sivaram. Indian Institute of Astrophysics. Bangalore , India

Search for Extra-Terrestrial Intelligence

Introduction to Astronomy

ASTRO 114 Lecture Okay. What we re going to discuss today are what we call radiation laws. We ve

Monday, January 30, 2012 First exam Friday. First Sky Watch due. Review sheet posted. Reading posted under announcements on web page, Chapter 6 -

How Did the Universe Begin?

News English.com Ready-to-use ESL / EFL Lessons

HOW TO GET LIGHT FROM THE DARK AGES

Wallace Hall Academy Physics Department. Space. Pupil Notes Name:

Sex in Space: Astronomy 330 TR English Building. Outline. Astro 330: Sex in Space? Be Careful of Science. ! The Drake equation

Hubble s Law: Finding the Age of the Universe

Phys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 1

Mike Garrett. Sir Bernard Lovell Chair, Prof. of Astrophysics. Director Jodrell Bank Centre for Astrophysics

Astronomy 330 HW 2. Outline. Presentations. ! Alex Bara

Transcription:

Welcome to Class 1: Drake EquaCon, SETI & Fermi Paradox Is it crazy to search for intelligent life? Where are they (E.T.I.) anyway? What would you like to spend most of our last class on? 1. Early SETI, Modern search methods, listen vs transmisng. 2. 2 Methods used by SETI and two problems. How these problems are being addressed.. 2 statements of Fermi s Paradox, and the three categories of solucons. Remember to set your channel to 80! 1 2 Opinion QuesCon: Has this class changed your view on life elsewhere? 1. I am a stronger believer in extraterrestrial life. 2. I am scll a strong believer in extraterrestrial life.. I did believe, but now I am not so certain there is life elsewhere. 4. I never believed and scll don t believe in ET life.. I didn t believe, but I think I do believe in ET life now. Remember to set your channel to 80! He designed an equacon to escmate: Who is this man? Number of Civilizations in the Milky Way capable of interstellar communication NOW. Your book has simplified the Drake EquaCon to: # = N hp x f life x f civ x f now N hp = Number of habitable planets in the Milky Way. F life = FracCon of those planets which will develop life. F civ = FracCon of those which develop Civilized life. F now = FracCon of those planets with Civilized life NOW. Let s consider some possible values for the Drake EquaCon.. Frank Drake Frank Drake also designed the first contact message sent to nearby stars. He was director of Arecibo Radio Telescope, and sent the message from there in 1974. (7 yrs ago) 4 N hp : How many habitable planets are in the Milky Way presently? (recall, there are a few 100 billion stars in the M.W.) F life : What fraccon of those planets develop life (of any kind)? 1. 200 billion 2. 1 billion. 1 million. 1/100th 4. 1,000. None 6

F civ : What fraccon of life- bearing planets developed civilizacons capable of communicacon at SOME Cme?. 1/100th. None F civ : What fraccon of those life- bearing planets capable of communicacon exist NOW?. 1/100th. None 7 8 What does this lead to? Early claims to communicate with E.T.I. MulCply together the classes four most popular input values: N hp x f life x f civ x f now = Total number of intelligent civilizacons from whom we could potencally get a signal now. 9 Marconi Early pioneers of electricity, Marconi and Tesla, also introduced radio (electro magnecc radiacon) communicacon. They both thought they where hearing E.T.I. Tesla Unfortunately, the radio wavelengths they were working at (AM radio, khz) cannot pass through (from outside or inside) Earth s ionosphere. 10 PRS : Why do we listen rather than send out a signal? Are we missing signals from E.T.I.? 1. Stay hidden from E.T. 2. Faster. Easier 4. Cheaper. All of the above 1. We don t know which direccon in the sky they are. 2. We assume they d use `light, but we don t know what kind of electromagnecc radiacon they are using.. We don t know how strong those signals are, or how far away they are coming from. 4. Is the signal concnuous, or does it stop and start every year, every minute?. Do we need to go back and re- observe all direccons? 11 12

INCREASING NOISE What FREQUENCY should we be listening? QUIET Where the universe is most quiet! But WHERE.. There is an infinite number of stacons : A civilized life would have astronomers who have built radio telescopes to observe H (hydrogen) and OH (hydroxyl) in the Galaxy. Even in this range, there exists an infinite number of FREQUENCIES to listen, depending on how broad a band (the `bandwidth ) you will consider to listen. There is also the amount of TIME you listen, and which DIRECTION you listen. 1 What DIRECTION should we be listening? How about starcng with nearby sun- like stars with exo- planets? All the stars listed here have exoplanets and are within 60 light years of Earth. This would be a TARGETED search A SURVEY search would sweep the sky randomly. 14 Challenges facing SETI sciencsts SETI sciencsts design unique radio receivers to work with radio telescope from 1000-0,000 MHz. Problem 1: SETI gets limle Cme to do targeted searches. Most of their Cme is looking where the telescopes happen to be looking (piggy backing other astronomy programs for free ). Arecibo SETI InsCtutes new SETI@Home Problem 2: NOISE H, OH lines fall HERE! Man- made, terrestrial noise is gesng louder and covering a greater amount of the frequency range. The Allen Telescope Array Mobile Phones have wiped out the special H, OH quiet zone! The FIRST, high- powered, DEDICATED, SETI- search radio telescopes. (Funded in part by Paul Allen, Microson co- founder). This allows for deeper, significant, TARGETED searches listening for E.T.I. MHz Frequency Limle can be done. SETI may need to move to the far side of the Moon. 1 This is what a signal would look like above. However, this one is due to terrestrial transmimers 16 F civ : fraccon of life- bearing planets developing commuicacng civilizacons = INTELLIGENCE.. 1/100th. None A philosophical argument about E.T.I. We are NOT special Intelligence has occurred elsewhere in our Galaxy We should be surrounded by evidence of this intelligence (civilizacons) Intelligence is an observed phenomenon which came about through natural causes. Given the vast age and number of planets in the Galaxy, intelligent civilizacon, more sophisccated than us, exists and would have colonized the encre Galaxy by now. We have no credible evidence that such a civilizacon exists in the Galaxy. 17 Where is everybody? THERE IS NO E.T.I. This is known as Fermi s Paradox 18

What is a paradox? Def. An argument that apparently derives self- contradictory conclusions by valid deduccon (through reasoning) from accepted premises. CriCcal premises leading to Fermi s Paradox 1) Intelligent civilizacons exist through out the Galaxy and have colonized the Galaxy by now. 2) Those intelligent civilizacons would communicate to us in such a way that we would know of their existence. Opinion: Premise 1. How sure are we that intelligent civilizacons would have colonized the en@re Galaxy? 1. Given the size and age of the Galaxy, absolutely yes. 2. Given the age of the Galaxy, its very likely.. Even with the age of the Galaxy, it is unlikely given its size. 4. I vote no. I don t believe any civilizacon has ever existed that can colonize the Galaxy. 19 20 Opinion: Premise 2: Provided such a colonizing civilizacon does exist, how sure are we it would communicate itself to us? 1. Absolutely 2. Probably. Maybe 4. No, probably not. Fermi s Paradox depend on BOTH premises to be absolutely true. 21 Possible solucons to Fermi s Paradox 1) We are alone. Humans are unique (or at least the first). 2) We aren t alone, but nobody has colonized the Galaxy Why? ColonizaCon of the Galaxy isn t so easy: a) Technological reasons (space is simply too big) b) Sociological reasons (they don t want to, waste of resources) c) CivilizaCons self destruct or die out before they get that far. ) They have colonized the Galaxy, but they are hiding it from us. (this is the Zoo Hypothesis) 22 What do YOU think is the solucon to Fermi s Paradox? 1. No E.T.I. exist. 2. CivilizaCons exist, but none have colonized the encre Galaxy yet.. The Galaxy HAS been colonized, but we ve not been asked to join the `club yet.. Final in class quiz!! 2

1. The Drake equacon tells us how many civilizacons in the Milky Way 2. We know Marconi & Tesla were not hearing E.T.I. because 1. are trying to communicate with us. 2. are capable of communicacng with us. 1. Their receivers were not sensicve enough. 2. They where hearing lightning.. The atmosphere blocks the radio waves where they were listening. 4. The noise in their system was too high. 2 26. SETI sciencsts selected radio frequencies to listen because 4. SETI sciencsts piggy bag on telescopes used by astronomers. What does this mean? 1. The receivers are most sensicve there 2. They can build big radio telescopes. We know E.T.I. would be sending signals there. 4. It is the quietest part of the electromagnecc spectrum. 1. They obtain the same data as the astronomers. 2. They are looking in the same direccon as the astronomers.. They use the same detectors as the astronomers. 4. All of the above. 27 28. The Fermi Paradox can be resolved by amacking/falsifying the 1. conclusions 2. contradiccon. deduccon 4. premises 29