physics 55: two classes about astrobiology professor henry greenside [email protected]

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Physics 55: Two Classes About Astrobiology Professor Henry Greenside [email protected] April 9, 2012

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Physics 55: Two Classes About Astrobiology Professor Henry Greenside [email protected]. April 9, 2012. Great Scientific Question: Does Life Exist Outside of Earth?. Why life is likely elsewhere in the universe How to search for life Where are the aliens? - PowerPoint PPT Presentation

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Page 1: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Physics 55: Two Classes About AstrobiologyProfessor Henry Greenside

[email protected]

April 9, 2012

Page 2: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Great Scientific Question:Does Life Exist Outside of Earth?

1. Why life is likely elsewhere in the universe2. How to search for life3. Where are the aliens?4. Travel to the stars? Not likely, not even by probes

Page 3: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

What is Life? Start with discussion:How is fire like or not like a living creature?

Duke-Maryland game, 2002

Page 4: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Brownian Motion? Belousov-Zhabotinsky Reaction?

Page 5: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Is a star living or not?

Page 6: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Characteristics of Life Requires nutrients (atoms, molecules) Requires energy (chemicals, sunlight) Requires water (???) Produces waste products Can reproduce Can respond to environmental changes Can evolve.

Biologists and computer scientists have especially madeprogress with artificial life: evolving reproducing mutating computer codes “living” in memory of computer, viruses and ecologies spontaneously appear.

Page 7: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Key Slide:Key Slide: Why life is likely elsewhere:

Same ingredients (atoms) everywhere Life started rapidly on Earth Laboratory experiments suggest spontaneous formation of biological molecule, comets support this. Earth life can survive extreme environments Earth does not seem special 1011 stars in a galaxy, 1011 galaxies Universe is ancient, lots of time for life to have started elsewhere

Page 8: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Relative Abundance of the Elements: Why H-C-N-O Based Life is Likely

Page 9: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Relative Abundance of the ElementsOn Earth's Surface

Page 10: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

What Can You Make With H, C, O, N, P?

Polysaccharides (sugars)

Nucleic acids, DNA, RNA

Amino acids and proteins

Page 11: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

“Inner Life of a Cell” Movie

Page 12: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Why is Life Likely: Life Appeared on Earth as Soon as Life Was Possible!

Earth “born” 4.5 billion years agoHeavy bombardment sterilized Earth 4 billion years ago, life appeared shortly after, 3.85 billion years ago!

Page 13: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Life Appeared on Earth as Soon as Life Was Possible

Australian stramatolitesSome are 3.5 billion years old!

Evidence of age:- Radiodating of fossils - Increased ratio of carbon-12 isotope to carbon-13 isotope in rocks indicates presence of life.

Page 14: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Two Possibilities About Rapid Appearance of Life

Life can arise easily and spontaneously.

Panspermia: life arrived on Earth from some other location, perhaps Mars or comets or from outside solar system, but that just shifts question of origin to another location (and Mars was also bombarded).

Page 15: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Possible Example of Panspermia:Rocks from Mars on Earth

Martian meteorite that crashed in Tissint, Morocco, July 2011

Page 16: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Why Is Life Likely: Suggestive Chemistry Experiments

Miller-Urey Experiment, 1953Amino acids, nucleic acids found

Page 17: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Why Life Might Be Likely:Extreme Forms of Life on Earth

Bacterial matsYellowstone

Extremophiles: acidophile, anaerobe, lithoautotroph, oligotroph, cryptoendolith, xerophile, piezophile, radioresistant, etc

black smokerPitch Lake, Trinidad

Page 18: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

But “Advanced” Life Forms Might be Rare:Complexity Transitions Are Difficult

Single cell creatures persisted in ocean for first billion years, then multi-cell creatures appeared.

Dinosaurs existed for about 130,000,000 years but, to our knowledge, never developed technological civilization.

Humans around 3-4 millions years, but technology arose only in last 100,000 years!

Page 19: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Looking For Life in the Solar System

Key assumption: liquid water is essential!

Page 20: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Stellar Habitable Zone: Where Liquid Water Might Occur

Page 21: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Habitable Zone = Goldilocks Zone

Page 22: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Only One Other Planetary Candidate : Mars

Mars

Traces of water foundNo signs of life

Page 23: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Water on Mars

Page 24: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Gravitational Tides Might Allow LifeOutside the Goldilock's Zone

This complicates search for life around other stars, remote moons hard to study!

Page 25: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Life in Europa's Icy Ocean?

4th largest moon, about same size as Earth's Moon

Gravitational tides warm ice, create salty ocean possibly ~60 miles deep, versus ~7 miles for Earth.

Page 26: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Life Around Other StarsGalactic Habitable (“Goldilocks”) Zone

Page 27: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Many Exoplanets Now Known: ~760 Planets In 600 Planetary Systems!

Page 28: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Not Know Yet if Earth-Like Planets Are Rare

Page 29: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Searching For ExolifeTerrestrial Planet Finder (TPF)

Block light from star, observe planets directly!

Page 30: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Look Spectroscopically for Biosignatures

Water vapor Excess oxygen Excess methane (found on Mars!) Complex molecules like chlorophyll

Page 31: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Infrared Spectroscopic Signature of Life Based onSolar Sysem

Page 32: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

SETI: The Search for Extraterrestrial Intelligence

Page 33: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Drake Equation: How To Estimate NumberOf Intelligent Civilizations in Galaxy

Page 34: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

How To Search For Intelligent Life

Arecibo Radio Telescope in Puerto Rico

Page 35: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

How to Communicate?

Page 36: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Interstellar Travel: Implications for SETI

Page 37: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

How to Communicate: Lincos?

?

Page 38: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

How to Communicate?

Page 39: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Where is Everybody?

Galaxy has radius of 50,000 light-years so time to colonize less than ten million years with v ~ 0.1c, ok grant 100,000,000 years, still much less than 1/10 age of universe!

Page 40: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Travel to the Stars by Fusion

Page 41: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Implications

We are the only technological civilization in the Milky Way.

Civilizations are common but it's hard to colonize space (interstellar travel is hard!

There is a galactic civilization but it is hiding from us.

Page 42: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Why is the search for life worthwhile?

Page 43: Physics 55: Two Classes About Astrobiology Professor Henry Greenside hsg@phy.duke

Class Discussion: are snowflakes alive?

Prof Kenneth Libbrecht. Caltechwww.its.caltech.edu/~atomic/snowcrystals/