Astronomy190 - Topics in Astronomy

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

description

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? - PowerPoint PPT Presentation

Transcript of Astronomy190 - Topics in Astronomy

Page 1: Astronomy190 - Topics in Astronomy

Astronomy190 - Topics in Astronomy

Astronomy and Astrobiology

Lecture 21: Search for Extraterrestrial Intelligence

Ty Robinson

Page 2: Astronomy190 - Topics in Astronomy

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

Are We Alone?

Page 4: Astronomy190 - Topics in Astronomy
Page 5: Astronomy190 - Topics in Astronomy

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

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

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

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

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

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

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

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

Fermi Paradox

What if Nc is much larger than 1?

Where are they?

Page 14: Astronomy190 - Topics in Astronomy

Alone in the galaxy?

What if Nc is less than 1?

Is anybody out there?

Page 15: Astronomy190 - Topics in Astronomy

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

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

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

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

Measuring Intelligence

big brainsmall brain

EQ= encephalization quotient

Page 20: Astronomy190 - Topics in Astronomy

Evolution to Higher Intelligence?

Enc

epha

lizat

ion

Quo

tient

(E

Q)

Time (millions of years ago)

Page 21: Astronomy190 - Topics in Astronomy

Evolution to Higher Intelligence?

Page 22: Astronomy190 - Topics in Astronomy

Intelligence = Technology?

Page 23: Astronomy190 - Topics in Astronomy

The Search for Extraterrestrial Intelligence

Page 24: Astronomy190 - Topics in Astronomy

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

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

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

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

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

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.