Notes
Outline
The Search for Extrasolar Planets
Astrometry
Precision Radial Velocity Searches
Discovery of Extrasolar planets
A Big Surprise : Close-in Jupiters
Properties of the systems found
How did the close Jupiters get there?
Transits
The Kepler Project
“Microlensing” : Gravitational lenses
The Problem with Direct Imaging
Nulling Interferometry
Interferometric Missions
Search Methods : what they can find
Eventually, imaging terrestrial planets?
The Elements of Life
Organic Chemistry
By definition, involves H,C,N,O
Most common elements (produced by most stars)
Well dispersed and available
Occurs even in interstellar space
Many organic compounds found in ISM, comets, meteors (despite extremely harsh conditions)
Easily delivered to early Earth, or produced locally
Biochemistry
Requires liquid water?
Arises naturally when basic conditions met?
What is “life”?
System out of chemical equilibrium which extracts energy from its environment to maintain itself
Energy source could be heat, light, chemical, other?
Reliably reproduces, with opportunity for evolution
Able to store and decode information for this
Basic Chemistry of Life (here)
Emergence of Life on the Earth
0.0-0.5 Gyr Formation and intense bombardment
surface is uninhabitable
0.5-1.0 Gyr Surface stabilizes, simple life starts
RNA, DNA; thermophilic progenitor (chemical energy)
1.0-2.0 Gyr Anerobic prokaryotes, stromatolite beds
single-celled, no nuclei; oldest fossils formed
2.0-2.5 Gyr Photosynthesis invented, free oxygen
surface life; use of sunlight; oxygen crisis
2.5-3.0 Gyr Aerobic bacteria, eukaryotes
exploit available oxygen (more energy), cell nucleus
3.0-3.5 Gyr bacteria diversify
Keep changing the mix, experiment
3.5-4.0 Gyr Sexual reproduction invented
Evolve, baby!
4.0-4.5 Gyr complex organisms appear
Let’s get together!  Let’s get it together!
The “Tree of Life”
Climate on the Earth
Habitable Zones (liquid surface water)
Many other conditions may be “habitable”
Life on Earth could be Martian
SETI : the search for extraterrestrial intelligence
Our only real hope of detecting ET (unless they come to us) is by listening to the radio
Radio travels at the speed of light, over the whole Galaxy
Radio is a low energy way to send a message
We already have the ability
             to send and receive across the Galaxy
Where should we listen?
Not the currently known extrasolar systems!
Solar-type stars? Milky Way?
How should we listen?
Frequencies that are relatively quiet.
How narrow-band?The “water hole”?
What should we listen for?
A regular carrier pattern. Complexity.
What are the odds we will hear
something?
The Drake equation
The Drake Equation
Evaluating the Odds Optimistically
…and so, we are listening!
Evaluating the Odds Pessimistically