time-line for global planetary events

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NASA’s search for life in the galaxy: NASA’s search for life in the galaxy: Information from exoplanets and the Information from exoplanets and the ancient Earth ancient Earth John W. Delano, Ph.D. John W. Delano, Ph.D. Associate Director, New Associate Director, New York Center for Astrobiology (NASA) Distinguished Teaching York Center for Astrobiology (NASA) Distinguished Teaching Professor Professor Dept. of Atmospheric and Environmental Sciences Dept. of Atmospheric and Environmental Sciences The The University at Albany (SUNY) University at Albany (SUNY) [email protected] [email protected] http://www.origins.rpi.edu http://www.origins.rpi.edu

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Page 1: Time-line for global planetary events

NASA’s search for life in the galaxy: NASA’s search for life in the galaxy: Information from exoplanets and the ancient EarthInformation from exoplanets and the ancient Earth

NASA’s search for life in the galaxy: NASA’s search for life in the galaxy: Information from exoplanets and the ancient EarthInformation from exoplanets and the ancient Earth

John W. Delano, Ph.D. John W. Delano, Ph.D. Associate Director, New York Center for Astrobiology (NASA) Associate Director, New York Center for Astrobiology (NASA)

Distinguished Teaching Professor Distinguished Teaching Professor Dept. of Atmospheric and Environmental Sciences Dept. of Atmospheric and Environmental Sciences

The University at Albany (SUNY) The University at Albany (SUNY) [email protected] [email protected]

http://www.origins.rpi.eduhttp://www.origins.rpi.edu

John W. Delano, Ph.D. John W. Delano, Ph.D. Associate Director, New York Center for Astrobiology (NASA) Associate Director, New York Center for Astrobiology (NASA)

Distinguished Teaching Professor Distinguished Teaching Professor Dept. of Atmospheric and Environmental Sciences Dept. of Atmospheric and Environmental Sciences

The University at Albany (SUNY) The University at Albany (SUNY) [email protected] [email protected]

http://www.origins.rpi.eduhttp://www.origins.rpi.edu

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Goal 4: Understand how past life on Earth developed and evolved by integrating evidence from both geologic and

biomolecular records

Goal 4: Understand how past life on Earth developed and evolved by integrating evidence from both geologic and

biomolecular records

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Time-line for global planetary eventsTime-line for global planetary events

00 45674567Myr (106 yr) in pastMyr (106 yr) in past

When did the major geochemical/geophysical reservoirs form on the Earth and Mars?

When did the major geochemical/geophysical reservoirs form on the Earth and Mars?

Atmosphere

Crust

Mantle

Core

Atmosphere

Crust

Mantle

Core

The major geochemical/geophysical reservoirs on Mars, Earth, and

probably differentiated asteroids were formed within this time-

interval (green; ~50 My).

The major geochemical/geophysical reservoirs on Mars, Earth, and

probably differentiated asteroids were formed within this time-

interval (green; ~50 My).

Chemically neutral volcanic gases released from Earth’s interior impacts?Chemically neutral volcanic gases released from Earth’s interior impacts?

Page 5: Time-line for global planetary events

Moonrise on the Hadean EarthMoonrise on the Hadean EarthMoonrise on the Hadean EarthMoonrise on the Hadean Earth

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S. Blair Hedges and Sudhir Kumar (2009) The Timetree of Life. Oxford University Press, 551 pp. New York.

S. Blair Hedges and Sudhir Kumar (2009) The Timetree of Life. Oxford University Press, 551 pp. New York.

“Life on Earth arose from a single source, ~4400-4200 million years ago (Ma), and quickly achieved a

prokaryotic complexity.”

“Life on Earth arose from a single source, ~4400-4200 million years ago (Ma), and quickly achieved a

prokaryotic complexity.”

http://www.timetree.orghttp://www.timetree.org

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Woese Woese et al.et al. (1990) Proc. National Acad. Sci. USA, 87, p. 4576-4579. (1990) Proc. National Acad. Sci. USA, 87, p. 4576-4579.Woese Woese et al.et al. (1990) Proc. National Acad. Sci. USA, 87, p. 4576-4579. (1990) Proc. National Acad. Sci. USA, 87, p. 4576-4579.

Bold lines at base of the tree Bold lines at base of the tree of life are … of life are …

hyperthermophilic hyperthermophilic chemolithoautotrophic chemolithoautotrophic

organismsorganisms

Bold lines at base of the tree Bold lines at base of the tree of life are … of life are …

hyperthermophilic hyperthermophilic chemolithoautotrophic chemolithoautotrophic

organismsorganisms

Why is Earth’s phylogenetic tree of

life rooted in hyperthermophilic

organisms?

Why is Earth’s phylogenetic tree of

life rooted in hyperthermophilic

organisms?

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Modified after … Miller S. L. and Lazcano A. (1995) Modified after … Miller S. L. and Lazcano A. (1995) The origin of life – The origin of life – did it occur at high temperatures?did it occur at high temperatures? J. Molecular Evol., 41, p. 689-692. J. Molecular Evol., 41, p. 689-692.

Modified after … Miller S. L. and Lazcano A. (1995) Modified after … Miller S. L. and Lazcano A. (1995) The origin of life – The origin of life – did it occur at high temperatures?did it occur at high temperatures? J. Molecular Evol., 41, p. 689-692. J. Molecular Evol., 41, p. 689-692.

~4400 ~3800Time in the past (Ma)Time in the past (Ma)

Late heavy bombardment

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Gomes et al. (2005) Nature, 435, p. 466-469.Gomes et al. (2005) Nature, 435, p. 466-469.

Ast

ron

omic

al u

nit

s (A

U)

Astronomical units (AU)

NeptuneNeptune

UranusUranus

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How diverse is life on Earth?How diverse is life on Earth?How diverse is life on Earth?How diverse is life on Earth? Green plants:Green plants: >10>1055 species species

Animals:Animals: >10>1066 species species Bacteria:Bacteria: >6 x 10>6 x 1033 species species

Fungus:Fungus: >10>1066 species species Viruses:Viruses: >3.6 x 10>3.6 x 1033

Green plants:Green plants: >10>1055 species species Animals:Animals: >10>1066 species species

Bacteria:Bacteria: >6 x 10>6 x 1033 species species Fungus:Fungus: >10>1066 species species Viruses:Viruses: >3.6 x 10>3.6 x 1033

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Goal 1: Understand the nature and distribution of habitable environments in the Universe.

Goal 1: Understand the nature and distribution of habitable environments in the Universe.