Class 10: Water/Life on Other Planets
Astrobiology
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
Life As We Know It
Conditions for Life (I) Liquid water
Conditions for Life (II) Carbon
Conditions for Life (III) Energy
Conditions for Life (IV) Stable Environment
Life on Mercury? Moon?
Life on Venus? Earth? Mars?
Life on the Gas Giants?
Life on Europa?
Life on Titan?
Life on Mars?
The Habitable Zone
Searching for Life: Biomarkers
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 2x1011 2x1011 fp = fraction of stars w/planets 0.01 0.5 nLZ = number of planets in habitable zone 0.01 1 fL = fraction of planets where life could begin 0.01 1 fI = fraction of life forms that evolve to intelligence 0.01 1 Fs = fraction of star’s life where life communicates 10-8 10-4 Nc = 2x10-5 10x106 • Pessimist: we are alone • Optimist: many civilizations
Search for Extraterrestrial Intelligence (SETI) Search for Extraterrestrial Intelligence SETI Institute Aricebo
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 • seti@home: - 2.3 million users, - 1000 yrs computer time each day
SETI Telescopes Effelsberg Big Ear Haystack Square Kilometer Array Arecibo Square Kilometer Array
The hmmmm….. Factor