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Early Earth and the Origins of Life Why do we care? How old do you think Life is?

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Presentation on theme: "Early Earth and the Origins of Life Why do we care? How old do you think Life is?"— Presentation transcript:

1 Early Earth and the Origins of Life Why do we care? How old do you think Life is?

2 Early Earth and the Origins of Life August 26, 2011 Lecture overview: -formation of the solar system and Earth -conditions on early Earth -theories concerning the origin of life on Earth -geologic evidence for earliest life on Earth

3 The Geologic Timescale Life!?! LIFE

4 Planetary disk NASA/JPL with thanks to L. T. Elkins-Tanton, JPL

5 Ca-Al inclusions in carbonaceous chondrites: 4.5672±0.0006 Ga (billion years ago)

6 Linked solidification and cooling processes Elkins-Tanton magma oceans at first…

7 Formation of the Moon: 4.53Ga Moon forms from debris of a collision between a Mars-sized body and Earth Animation of moon formation, courtesy of Joe Tucciarone

8 The Archean Earth System Archean: 4.03 to 2.5 Ga (Ga=billion years ago) Late Heavy Bombardment (4.1 to 3.8 Ga) Atmosphere: hardly any molecular oxygen (O 2 ); appears at ~2Ga  earliest life probably anearobic! UV radiation (no ozone shield)  earliest life probably underwater! CO 2 and CH 4 -rich atmosphere Likely warm surface conditions (80 o to 45 o C) High rate of heat transfer from core to surface, possible thin crust, plate tectonics just being established Stanley M. Awramik w/ thanks to Stanley M. Awramik, UCSB

9 Steps towards Life 1.synthesize biomolecules (organic C, amino acids) 2.organize them into macromolecular systems 3.emergence of self-replicating codes of molecules (RNA) 4.emergence of molecular evolution via natural selection after Hazen, 2006

10 Stanley Miller and Harold Urey (1953) -ran experiment for one week -observed 10% of C in organic form -2% of C in amino acid form but: -too high-energy environment (lightning not continuous) -early Earth contained appreciable CO 2 (in addition to CH 4 ) on the other hand… -meteorites contain appreciable amino acids The Miller/Urey Experiment

11 A modern-day Miller/Urey experiment Johnson et al., Science, 2008 -redid the Miller/Urey experiment in 2007 -found 22 amino acids (more than M/U!) -also analyzed the original M/U vials using modern-day analytical techniques Jeff Bada, Scripps Inst. of Oceanography

12 What about combining the two? hydrothermal vents  “Hot volcanoe” and “cold soup” models regarding the origin of Life on Earth Hazen, 2006 -organic molecules and amino acids can be organized by mineral lattices as templates

13 Modified from Awramik and McNamara, in press A schematic of evolution of life on Earth

14 Stromatolites: biofilms of cyanobacteria capture and bind sediment Pre-Cambrian? Today, at Shark’s Bay, Australia

15 An Opinion “…true consensus for life’s existence seems to be reached only with the bacterial fossils of the 1.9-billion-year-old Gunflint Formation…” Moorbath, S., 2005. Nature, 434, p. 155):. Tyler & Barghoorn, Science, 1954

16 Candidates for Early Archean Fossils

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19 Nature, 1996 3.85Ga rock apatite (Ca-PO 4 ) grain in rock “carbonaceous” remnant material after apatite dissolved with acid And the controversy continues….

20 ion microprobe -instrument that focuses a beam of charged ions onto the surface of a sample -charged ions generate ions for mass spectrometric analysis (separation by mass) -in this case, used to look at different “isotopes” of carbon

21 Carbon isotopes -C has two stable isotopes (12 protons, different # neutrons): 12 C (99%) and 13 C (1%) -for the most part, they behave identically -however, there is a slight difference in their “reactivity” ( 12 C > 13 C) -photosynthesis: 12 C is preferentially incorporated into biological materials (low 13 C values) cross-section of a leaf Mojzsis, 1996

22 Raman spectroscopy -instrument detects extremely small changes in energy of light/laser/IR radiation -in Schopf 2002, a laser is used to excite the sample molecules into a higher energy state; they report “Raman shifts” that denote changes in laser wavelength -shifts denote presence of specific chemical bonds and their relative orientations

23 kerogen -concentrated, high-molecular-weight organic compounds occuring in sedimentary rocks -precursor to fossil fuels (formed upon heating of kerogen) an oil shale carbonate (containing CO 3 ) -most commonly CaCO 3, the mineral in limestone -many marine organisms form carbonate shells (corals, foraminifera) limestone cliffs

24 trichome -any small outgrowth or appendage on certain plants and algae trichomes on a cannabis plant chert -finely-grained, silica-rich, microcrystalline rock -is a product of high-T chemical alteration of rocks

25 greenschist -metamorphic rocks resulting from low-T, moderate pressure environments -typically somewhat green in color


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