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Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

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Page 1: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Astronomy190 - Topics in Astronomy

Astronomy and Astrobiology

Lecture 21: Search for Extraterrestrial Intelligence

Ty Robinson

Page 2: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Questions of the Day

• What is the Drake Equation, and why is it useful?

• Even if life arises, will it inevitably evolve towards intelligence?

• What are the methods SETI uses to search for intelligence today?

Page 3: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Are We Alone?

Page 4: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson
Page 5: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

The Drake EquationEstimating the number of civilizations in the Milky Way with which we might hope to communicate

Nc = Ns x fp x Ne x fl x fi x fc x L

Page 6: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

The Drake Equation

number of stars in the galaxy(~200 billion)

Nc = Ns x fp x Ne x fl x fi x fc x L

Page 7: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

The Drake Equation

QuickTime™ and a decompressor

are needed to see this picture.

fraction of stars that have planets(> 10%)

Nc = Ns x fp x Ne x fl x fi x fc x L

Page 8: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

The Drake Equation

number of terrestrial planets per planetary system in the Habitable Zone

QuickTime™ and a decompressor

are needed to see this picture.

Nc = Ns x fp x Ne x fl x fi x fc x L

Page 9: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

The Drake Equation

fraction of such planets on which life actually evolved

QuickTime™ and a decompressor

are needed to see this picture.

Nc = Ns x fp x Ne x fl x fi x fc x L

Page 10: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

The Drake Equation

fraction of inhabited worlds that develop intelligent life

Nc = Ns x fp x Ne x fl x fi x fc x L

Page 11: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

The Drake Equation

fraction of worlds with intelligent beings that produce a civilization capable of interstellar communication

QuickTime™ and a decompressor

are needed to see this picture.

Nc = Ns x fp x Ne x fl x fi x fc x L

Page 12: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

The Drake Equation

the lifetime of such civilizations (divided by the age of the galaxy)

Nc = Ns x fp x Ne x fl x fi x fc x L

Page 13: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Fermi Paradox

What if Nc is much larger than 1?

Where are they?

Page 14: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Alone in the galaxy?

What if Nc is less than 1?

Is anybody out there?

Page 15: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

fi : the Question of Intelligence

Is the evolution of intelligence inevitable?

Nc = Ns x fp x Ne x fl x fi x fc x L

Page 16: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

fi : the Question of Intelligence

• two schools of thought1. intelligent (radio telescope building) life is rare

• we’ve had life for 3.5 Gyrs, but radio and TV signals for only the last 50 yrs.

• intelligence evolved as the result of random chance

• remember: evolution is not goal-oriented!

Page 17: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

fi : the Question of Intelligence

• two schools of thought2. there is evolutionary pressure for intelligence

• natural selection promotes greater intellectual capability

• if humans hadn’t developed technology-building intelligence, something else would have

• maybe there is a widespread selection pressure for intelligence

Page 18: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Convergent Evolution• organisms of different evolutionary backgrounds

that occupy similar ecological niches will eventually come to resemble one another

Is there an evolutionary trend favoring intelligence?

• maybe intelligence increases fitness so much that if that niche is not filled, species will be selected for intelligence via convergent evolution

Page 19: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Measuring Intelligence

big brainsmall brain

EQ= encephalization quotient

Page 20: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Evolution to Higher Intelligence?

Enc

epha

lizat

ion

Quo

tient

(E

Q)

Time (millions of years ago)

Page 21: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Evolution to Higher Intelligence?

Page 22: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Intelligence = Technology?

Page 23: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

The Search for Extraterrestrial Intelligence

Page 24: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Radio SETI: Where to look?

• a “hailing signal” would need to have a narrow bandwidth signal component– easier to see against “noise” from interstellar gas, distant

galaxies, the radio receiver

• first proposed to be tuned to 1420 MHz, the

frequency of H gas in the interstellar medium– for comparison: NPR is at 94.9 MHz

Page 25: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Categories of Signals• signals used for local communication where

intelligent beings live

• signals used for communication between a civilization’s home world and some other site

• intentional signal beacons

Page 26: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Finding and Decoding Signals• some things to look for:

1,679 bits

23 x 73

–broadcast in a strong, narrow wavelength–flashing on/off or switching frequencies–repetition–prime numbers? π? e?

Page 27: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Where do we look?

• targeted search– not all locations in space are

equally probable for intelligent life

• sky survey– no assumptions made about where they might be

located

Page 28: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Questions of the Day

• What is the Drake Equation, and why is it useful?

• Even if life arises, will it inevitably evolve towards intelligence?

• What are the methods SETI uses to search for intelligence today?

Page 29: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 21: Search for Extraterrestrial Intelligence Ty Robinson

Quiz

3 - What is one thing you did not understand from today’s lecture?

2 - What term in the Drake Equation will NASA’s Kepler mission be the first to measure?

1 - Explain why methane on Mars is a biosignature but methane on Titan is not.