UV Irradiation of Interstellar Medium : Production of Organic Materials Evidence of Life in Meteorites: Origin of Life on Earth? 8 th Dec 2006 Yuki Shiraji.

Slides:



Advertisements
Similar presentations
Chapter 4 Chemistry of Carbon
Advertisements

Early Origins Chapter 19.1 & 19.3.
Environmental Systems: Chapter 2-
Primordial Cell Membrane. Overview  Structure  Function  Ingredients  Self-assembly  Challenges  Future Work  Structure  Function  Ingredients.
Properties of Alcohols, Ethers, and Thiols Chapter 12 Organic Compounds with Oxygen and Sulfur Copyright © 2005 by Pearson Education, Inc. Publishing.
Chemistry Packet Presentation
1 Science (1999) Vol. 283 p Introduction A Brief Introduction - Max How we know polycyclic aromatic hydrocarbons are ubiquitous and abundant.
Topic 2.2 Water.
17-2 Earth’s Early History
Astrobiology The cosmic chemistry of life (the molecular basis)
Lipids
Lipid Review What are the four examples of lipids? 2.
Earth’s Atmosphere & The Origin of Life
Chapter 4 Notes Carbon and the Molecular Diversity of Life.
The Nature of Molecules Chapter 2. 2 Atomic Structure All matter is ____________ atoms. Understanding the structure of atoms is critical to understanding.
Chap 4 Carbon and the Molecular diversity of life.
Structure of Life. Elements of Life  90 Natural occurring elements, 25 essential  96% of the mass of a human is made up of C, O, H, N.
Helgi Rafn Hróðmarsson Friday seminar Utilization of spectroscopy in the determination of the origins of life.
The Nature of Molecules Chapter 2. 2 Atomic Structure All matter is composed of atoms. Understanding the structure of atoms is critical to understanding.
AP Biology Wed. 9/5/12 Agenda  Start Chp.4&5 with Chp.4 Notes  Macromolecules Synthesis/Degradation Video Clip  Start Biomolecules group poster.
AP Biology Origin of Life “…sparked by just the right combination of physical events & chemical processes…”
Chapter 17 Origins of Life. Astrobiology is study of the origin, evolution, distribution, & destiny of life in the universe. It attempts to answer 3 fundamental.
Amino Acids From Interstellar Space Craig Lieneck.
Functional Groups.
Chemical Evolution: The Atoms and Molecules of Ancient Earth.
Chapter 12 Section 1 How Did Life Begin? Grade 10 Biology Spring 2011.
Chapter 4 Functional Groups Chapter 5 Macromolecules
Life.
Chapter 26 Early Earth and the Origin of Life. Phylogeny Traces life backward to common ancestors. How did life get started?
Biochemistry Functional Groups. Carbon—The Backbone of Biological Molecules All living organisms Are made up of chemicals based mostly on carbon due to.
Chemistry of Life Matter… Energy… Life…. Objectives Objectives: A.Explain the nature of matter; B.Discuss the importance of water and solutions; C.Break.
Do Now 10/8 Complete SAQ 2.4 and 2.5 on pg 13 in INB if you did not complete for hw X and Y show the structures of two hexose sugars Which statement is.
Chapter 2: Atoms and Molecules of Ancient Earth Life requires about 25 elements carbon (C) oxygen (O) hydrogen (H) nitrogen (N)
 The solar system is estimated to be 6.6 billion years old.  Earth is estimated to be 4.1 billion years old.
Discovering the origins of life on Earth. Organic molecules Before life could begin the organic molecules necessary for life first had to ‘evolve’. These.
FUNCTIONAL GROUPS IN ORGANIC COMPOUNDS. Naturally occurring organic compounds are found in plants, animals, and fossil fuels All of these have a plant.
The Nature of Molecules Chapter 2. 2 Do Now Complete Vocab pre-quiz for Ch 2.
What has happened so far in chemical evolution? Biological monomers formed from interaction of atmospheric gases, water and energy The monomers (ex. nucleotides)
STAAR Reporting Category 1 Matter & Energy
The Nature of Molecules
Biology 140 Chapter 2 Notes.
Section 1: How Did Life Begin?
Chapter 14 Aldehydes, Ketones, and Chiral Molecules
Review of Basic Chemistry
Carbon and the Molecular Diversity of Life
The Basic Chemicals of Life
Topic 2.1 Molecules to metabolism
TAKS objective 3 Structure and Properties of Matter
Chemistry of Carbon and
Topic 2: Molecular Biology
The Star of The Show (Ch. 4)
Building Blocks of Life
Chapter 2: Water pgs
Carbon and the Molecular Diversity of Life
Biological Chemistry -- Organic: anything with carbon vs.
Chapter 4 Carbon and the Molecular Diversity of Life
2.1 UNSATURATED HYDROCARBONS
Carbon and the Molecular Diversity of Life
Functional Groups and Macromolecules
Chemistry of Life Matter… Energy… Life….
STAAR Reporting Category 1 Matter & Energy
Carbon and the Molecular Diversity of Life
Matter Volume is the amount of three dimensional space an object occupies. Mass is a measure of the amount of matter. Matter is anything that has mass.
Carbon and Molecular Diversity
Biological Chemistry -- Organic: anything with carbon vs.
STAAR Reporting Category 1 Matter & Energy
TAKS objective 3 Structure and Properties of Matter
Chapter 2 Chemistry of Life.
Chapter 14 Aldehydes, Ketones, and Chiral Molecules
Presentation transcript:

UV Irradiation of Interstellar Medium : Production of Organic Materials Evidence of Life in Meteorites: Origin of Life on Earth? 8 th Dec 2006 Yuki Shiraji

Current Common Theory: Chemical Evolution Creation of Amino Acids from Inorganic Material Miller-Urey Experiment: Electric Discharge Methods Using Alternative Energy Sources: -Heat -Gamma rays -Infrared rays -Ultraviolet rays

Scott A. Standford et al.: Creation of Organic Materials under Their Emulated Interstellar Environment. + Similar Organic Materials Have Been Discovered in Meteorites. ↓ Hypothesis: “ Organic Materials Created in the Space Were Brought to the Earth via Meteorites Which Was the Point of Origin of Life on Earth.”

UV Irradiation of Simulated Interstellar Medium Resulted in… 1)Creation of Alcohols, Quinones, and Ethers. 2) Creation of Membrane-like Droplets. Experiments Done by Scott A. Standford et al :

Experiment #1: PAH + H20 + UV Irradiation Results in the Production of Alcohols, Quinones, and Ethers PAH = Polycyclic Aromatic Hydrocarbons

Experiment#1: Materials and Methods Methodology 1) H2O + PAHs  compressed into Ice particle, (H2O/PAH= ) 2) Temperature = 10K 3) UV Irradiation at 2x10^15 Photons / sec (cm) 4) Irradiation Treatment for 200mins 5) Examine the Resulting RESIDUE Benzene Materials EX: Benzo[ghi]perylene

Experiment #1: Methodologies Cont. Result of UV radiation to PAH + H20 Result of UV radiation to PAH + H20

Experiment #1: Examining the Residue Method #1: Infrared spectroscopy Significance of Results: Starting Material: PAHs  Stable, Refractory, Unreactive Resulting Product: Functional groups  Gain of Reactive Nature; the Ability of the Molecule to React with Other Nucleophiles Result: Discovery of Addition of Functional Groups to the PAH 1. >C=O (Carbonyl) 2. –O-H (Hydroxy)

Experiment# 1: Examining the RESIDUE Method #2: Mass Spectroscopy Method: Compare Mass Spec. Results of UV Radiated Benzo[ghi]pyrene And Control. Results: - Residue from UV Radiated Sample Contain Additional Oxygen and Hydrogen Atoms

Experiment #1: Analysis of Results Species Found in the Residue Belong to a Class of Molecules that Are Necessary Organic Compounds for Primordial Life: Ex) Ketone + Quinones: Made from Ketone Precursors. Quinones Are Crucial for Electron Transport in Simple Organisms

Experiment #1: Analysis of Results Mass Spec. of Corene (another type of PAH) shows Increased Deuterium Enrichment: This Enrichment Profile Is Consistent with that of Organic Globules Found in Meteorites Ex). Organic Globules Found in Tagish Meteorites: Times Increase in D- enriched Method #2: Mass Spectroscopy

Experiment #2: Gas-Mixture (H2O, CH3OH, NH3, CO) + UV Irradiation Results in the Production of Membrane-like Organic Droplets

Experiment#2: Materials and Methods 1)Gas-mixture: H2O, CH3OH, NH3, CO (ratio of 100:50:1:1) was compressed into ice particle 2) Temperature = 15K 3) UV irradiation at 10^15 photons/sec 4) Isolate membrane-like materials  use HPLC (High Performance Liquid Chromatography) 5) Examine the RESIDUE (droplets) Methodology Materials Emulated Interstellar Gas-Mixture: H2O, CH3OH, NH3, CO

Experiment #2: Observations, Data Results and Anaylsis Observations -Starting Gas-Mixture (H2O, CH3OH, NH3, CO) Was Mostly Polar = Water Soluble. -But Droplets  Water Insoluble This INDICATES That, the Subunit Components Making Up the Lipids Found Are Amphiphilic -Have Both Polar and Non-Polar Characteristic -Have Both Hydrophilic and Hydrophobic. Conclusion: UV Irradiation Caused the Formation of Amphiphilic Molecules

Experiment #2: Analysis of Droplet Structures Method: Fluorescent Experiment Hollow Structure Inside of droplets??  YES! Explanation for This Finding: Nakamura : “Formation of Lipid Wall  Prevents Further UV to Reach Inside.” Depth of Lipid Wall in Tagish Lake Meteorites = Depth of UV penetration (about nm)

*Conclusion* 1)UV Irradiation on emulated Interstellar PAHs Creates Complex Organic Compounds Crucial for Primordial Life on Earth (Such As Alcohols, Quinones, Ethers, etc), 2) UV Irradiation on Emulated Interstellar Gas-Mixture (H2O, CH3OH, NH3, CO) Creates Membrane-like Vesicle Droplets Which Highly Resemble Membranes Found in All Cells Today.

So, Now It Is Proven That Organic Materials Found on Earth Can Be Created in an Artificial Interstellar Medium ↓ Justifies the Hypothesis: “Life on Earth Originated in Space, Reaching to Earth via Meteorites” + Also in Reality, Organic Materials Are Discovered in Meteorites,

Further Considerations Organic Droplets Could Potentially Be the Precursors to the Very First Cells that Existed.

E N D. Thank you! Works Cited 1. Max P. Bernstein, Scott A. Sandford, Louis J. Allamandola, J. Seb Gillette, Simon J. Clemett, Richard N. Zare, in Science 283, 5405, (1999), p Jason P. Dworkin, David W. Deamer, Scott A. Sandford, and Louis J. Allamandola, in PNAS 98, 3, (2001), p Keiko Nakamura-Messenger, Scott Messenger, Lindsay P. Keller, Simon J. Clemett, Michael E. Zolensky, in Science 314, 5804, (2006), p