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Class 10: Water/Life on Other Planets
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Astrobiology
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Life’s Sequence on Earth
3.75 Billion years ago 1.7 Billion years ago 4.5 Billion years ago 600 Million years ago 500 Million years ago 225 Million years ago
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Life As We Know It
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Conditions for Life (I)
Liquid water
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Conditions for Life (II)
Carbon
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Conditions for Life (III)
Energy
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Conditions for Life (IV)
Stable Environment
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Life on Mercury? Moon?
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Life on Venus? Earth? Mars?
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Life on the Gas Giants?
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Life on Europa?
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Life on Titan?
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Life on Mars?
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The Habitable Zone
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Searching for Life: Biomarkers
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The Drake Equation Nc = N* x fp x nLZ x fL x fI x Fs
= # of communicative civilization in galaxy Pessimistic Estimate Optimistic Estimate N*= # stars in galaxy x x1011 fp = fraction of stars w/planets nLZ = number of planets in habitable zone fL = fraction of planets where life could begin fI = fraction of life forms that evolve to intelligence Fs = fraction of star’s life where life communicates Nc = 2x x106 • Pessimist: we are alone • Optimist: many civilizations
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Search for Extraterrestrial Intelligence
(SETI) Search for Extraterrestrial Intelligence SETI Institute Aricebo
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SETI Projects nonprofit, $20M astronomy data - 2.3 million users,
• Project Phoenix: primary search, nonprofit, $20M SETI Projects • SERENDIP: piggyback search of ordinary astronomy data Jill Tarter • - 2.3 million users, yrs computer time each day
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SETI Telescopes Effelsberg Big Ear Haystack Square Kilometer Array
Arecibo Square Kilometer Array
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The hmmmm….. Factor
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