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Astrobiology in the Context of a Research University. Dimitar D. Sasselov. Center for Planetary Astrophysics & Department of Astronomy Harvard University. One of Humankind’s Biggest Questions:. What is the path from Stars to Life ?.
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Astrobiology in the Context of a Research University Dimitar D. Sasselov Center for Planetary Astrophysics & Department of Astronomy Harvard University
One of Humankind’s Biggest Questions: What is the path from Stars to Life ? • One of the last remaining unresolved questions • It has become tractable by modern science • Major emerging discipline - one could lead !
The “Essence” of Life • Resolving the “Chicken-&-Egg” problem • of nucleic acids vs. proteins - • too much complexity ? • Solution: • RNA-catalyzed • RNA replication !
The “Essence” of Life • Find how Darwinian • behavior can emerge • from chemistry • Develop synthetic • self-replicating • molecules • Membranes & • vesicles - cell division • before cells ! RNA (red) adsorbed into clay, inside a vesicle (green) - Szostak lab (2004).
The Ultimate Leap: Chemistry to Life • Prebiotic chemistry: find a plausible route to “self-replicators”; • Prebiotic chemistry: on mineral surfaces, inside atmospheric particles, and ice-eutectic reactions; • Prebiotic chemistry: on the young Earth, other planets and in space ?
Co-evolution of Planets and Life • Life as a planetary phenomenon: • constraining the chemical pathways that led to life. • Unearthing the evidence - • how did it all begun on Earth ? • The next big question - • was Mars alive ? A fossil cyanobacterium in circa 1.5 Gyr old sedimentary rocks - (A. Knoll).
Mars, Endurance Crater distinct layers of sedimentary rocks (A. Knoll, Sept. 2004)
The Universe is the “stage”… • Planets - cradles for life • in a hostile Universe • Search & exploration: • by end of decade - • know planets like Earth • Formation & stability • of planetary systems Artist concept of a hot Jupiter
The Planetary Perspective • The initial condition: • chemical makeup & isotopes; • Precise timeline of early events. A pre-solar SiC grain from the Murchison meteorite. 2 microns
The Planetary Perspective • Precise timeline of early events. Jacobsen (2003)
Planets Orbiting Other Stars Number of planets discovered around stars like our Sun: 154 planets 14 multiple planet systems
Evidence for Planet OGLE-TR-56b Doppler Shift Light Dimming Konacki, Torres, Jha, Sasselov, 2003, Nature
Mass-Radius diagram: All known transiting extra-solar planets Konacki, Torres, Sasselov, Jha (2005)
The Next Step:Find Planets like Earth Lynnette Cook
KEPLER: Search for Earth Twins NASA Mission - launch in 2007 Transit Search: ~100,000 stars Can detect planets like our Earth GOAL: discover ~12 Earths in habitable zones; also - thousands of giant planets like Jupiter.
Why in a University ? • A major emerging discipline. • Education: a bridge b/n life & physical sciences • Undergraduate: e.g. Harvard Melton/Gross committee • Graduate: specialized courses; workshops • Public outreach: immense potential (lecture series, etc)
Special thanks to team members: S. Jacobsen, J. Szostak, A. Knoll, S. Martin, M. Shair
The Other Known Transiting Extrasolar Planet HD 209458b: Dimming of light due to transit, observed with HST. Tells us DIRECTLY: Planet radius, INDIRECTLY: Planet density Planet composition Brown, Charbonneau, Gilliland, Noyes, Burrows (2001)
Model: Seager & Sasselov 2000 Detection: Charbonneau et al 2002
NASA’s Terrestrial Planet Finder • Find and characterize Earth-like planets • Reduce the glare of the parent star by one million to one billion • Launch date 2015 • Observe stars within 50 light years Alcatel Space Industries