Topics in Astrobiology 1.What is and can be done 2. The problem of chirality.

Slides:



Advertisements
Similar presentations
Topic D.1 Evolution Origin of Life on Earth.
Advertisements

IB Biology Option D Evolution.
Chapter 2 Biochemistry Atoms, Bonds, Periodic Table, Energy and Work, Properties, Solutions, Acids and Bases, Organic and Inorganic Compounds, Food Labels,
Chemistry 100 Chapter 25 Biochemistry. Chiral Molecules  Molecules that have non-superimposable mirror images – chiral molecules Enantiomers  Distinguish.
Biology Unit 2 Test – August 26th
Extra-Terrestrial Life and the Drake Equation Astronomy 311 Professor Lee Carkner Lecture 25.
Universe formed 15 billion years ago (Big Bang) Galaxies formed from stars, dust and gas Earth formed 4.6 billion years ago.
Chemistry Review. Why is carbon found in all living things?
Silicon Based Life Forms. Life on Earth Chemistry of life on Earth -organic -Carbon based -water used as solvent -from water come hydrogen bonds, which.
Lecture 15. Prebiotic Chemistry, Pyrite, Clays, RNA World, Transition from Abiotic to Biotic World reading: Chapter 5.
Homochirality through enantiomeric cross-inhibition Axel Brandenburg, Anja Andersen, Susanne Höfner, Martin Nilsson To appear in Orig. Life Evol. Biosph.,
How long can left and right handed life forms coexist? Axel Brandenburg, Anja Andersen, Susanne Höfner, Martin Nilsson, Tuomas Multamäki (Nordita) Orig.
Chapter 25 The History of Life on Earth. Question u How have events in the Earth’s history contributed to life as we know it?
Earth is estimated to be ~4.6 bill. yr old –Evidence: Radiometric dating of rocks & meteors Nebula Hypothesis: –Nebula: cloud of gas & dust in space.
Theories on the Origin of Life. When did life form? Age of the Earth: 4.6 billion years Oldest rocks: 3.8 – 4.0 billion years Oceans established > 3.8.
Astrobiology, homochirality, and origins of life Int. J. Astrobio. 3, 209 (2004), 4, 75 (2005), Orig. Life Evol. Biosph. 35, 225 (2005), 35, 507 (2005)
Modeling Chemical Evolution
Polymer Molecule made of many monomers bonded together
Prebiotic Chemstry Jeff G. Wardeska, PhD Jan. 24, 2008.
Objectives: 1.Be able to Summarize the Miller-Urey Experiment 2.Relate the structure of Clay beds to the polymerization of nucleotides 3.Understand the.
+ Chapter 14 Section 2. Activity - Earth’s timeline Materials: 1 ruler, 1 sheet of paper, colored pencils or markers Instructions: Draw a horizontal line.
THE ORIGIN OF LIFE HOW DID IT ALL BEGIN?. FORMATION OF THE EARTH 4.55 billion years ago Earth formed by accretion of matter. Constant bombardment heated.
Origin of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust in space.
Origin of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust in space.
Origin of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust in space.
EOCT Review Day 3 Protein Synthesis Photosynthesis Respiration.
KEY CONCEPT The origin of life on Earth remains a puzzle.
Origin of Life Today How did life originate? Working back from today The most basic components How DNA and RNA work Working forward from simple molecules.
12.3 Origin of Life 12.3: The Origin of Life How do scientists think Earth formed and life on Earth began?
Origins of Life Chapter 12 Section 3 pg. 368.
The Search for Life in the Universe. Criteria Defining Life 1.Made up of one or more cells 2.Organized 3.Grows & develops 4.Reproduces 5.Responds to stimuli.
THE HISTORY OF LIFE ON EARTH PART 1 UNIVERSE TO EUKARYOTES.
Astrobiology, homochirality, and origin of life
New Core Curriculum The Asymmetry on a Molecular Scale (Chirality)
Earth was very different billions of years ago 1. The most widely accepted hypothesis is the nebula hypothesis. The solar system formed by a condensing.
Chapter 2 Review. What is an atom? The smallest basic unit of matter.
Origin of homochirality in an early peptide world Axel Brandenburg, Harry Lehto and Kirsi Lehto (Nordita) Int. J. Astrobio. 3, 209 (2004), 4, 75 (2005),
General Chapter 6 Assessment answers. Section 1 1. What is chemistry? The study of matter 2. What is the definition of matter? Anything that has mass.
12.3 Origin of Life KEY CONCEPT The origin of life on Earth remains a puzzle.
12.3 Origin of Life KEY CONCEPT The origin of life on Earth remains a puzzle.
12.3 Origin of Life KEY CONCEPT The origin of life on Earth remains a puzzle.
Essential Questions How does the structure of water make it a good solvent? What are the similarities and differences between solutions and suspensions?
Homochirality: models and results Axel Brandenburg, Anja Andersen, Susanne Höfner, Martin Nilsson To appear in Orig. Life Evol. Biosph., q-bio.BM/
Meteorites Meteorites are solid objects originating in outer space that survives impact with the Earth's surface. One of famous: Allende Fell in Mexico.
Ch 2 The Chemistry of Life Students know most macromolecules (polysaccharides, nucleic acids, proteins, lipids) in cells and organisms are synthesized.
Basic Biological Chemistry
Spyros Kitsionas Grade 5 BISS 28/3/2017
Theories of where life came from
ORIGIN OF LIFE.
Review PowerPoint For each topic, there is a key image to understand, and the essential idea and question to be able to answer. Key terms in each of the.
ASTR/GEOL-2040: Search for life in the Universe: Lecture 6
KEY CONCEPT The origin of life on Earth remains a puzzle.
KEY CONCEPT The origin of life on Earth remains a puzzle.
KEY CONCEPT The origin of life on Earth remains a puzzle.
Macromolecule Review.
Biochemistry The Building Blocks of Life
Evolution Origin of Life on Earth.
KEY CONCEPT The origin of life on Earth remains a puzzle.
Diversity of Living Things
The Chemistry of Life Unit One Biology Notes.
ASTR/GEOL-2040: Search for life in the Universe, Lecture 7
The origin of Life.
Origin of Life Page 96 Just write the red lettering into your notebook.
Please take out Breeding Bunnies Lab to turn in
4/19/12 Objective: Understand and explain the field of astrobiology
KEY CONCEPT The origin of life on Earth remains a puzzle.
Origin of Life Just write the red lettering into your notebook.
Reading: 12.3 (finish); 3.1, 3.3; test monday Activator: enzymes
All organic molecules contain which element?
KEY CONCEPT The origin of life on Earth remains a puzzle.
Presentation transcript:

Topics in Astrobiology 1.What is and can be done 2. The problem of chirality

2 The range of problems From dust to planets –Exoplanets –Water delivery –Habitable worlds Archaen world –Volcanos, Carbon cycle –Impacts, panspermia Miller experiment –Amino acids, chemistry Artificial life Origin of life –RNA world, TNA, PNA –homochirality Early life –Extremophiles –cyanobacteria

3 Rough time line 10 4 yr 10 6 yr 10 8 yr 10 9 yr planetesimals Sun ignites All gas gone Remaining dust settles First life

4 Time line (later)

5 Carbon cycle Source of the atmosphere Venus, Earth: active volcanos: thick atmosph. Mars:Volcanosextinct

6 Water delivery via comets Comet LINEAR: same HDO ratio as on Earth’s oceans cf. Hale-Bopp (too much)

7 Evaporation of LINEAR during fly-by. Cloud of hydrogen Estimated water content 3x10 9 kg (outgassed during fly-by) Obsered in Ly 

8 Miller/Urey experiment 15 organic compounds 2% amino acids (11 different ones) Wait 1 week

9 The RNA world Central dogma of chemistry of life –DNA  RNA  protein enzyme all enzymes are themselves proteins? Walter Gilbert (1986)

10 RNA itself as enzyme

11 pre-RNA worlds Many problems: stability of sugars 2-amino ethyl glycin (AEG)

12 pre-RNA worlds PE Nielsen (1993) better alternative: Nelson, Levi, Miller (2000)

13 Photosynthesis Requires chlorophyll As catalyst What about chiralitry?

Homochirality: models and results Axel Brandenburg, Anja Andersen, Susanne Höfner, Martin Nilsson To appear in OLEB, q-bio.BM/

15 Aminoacids in protein: left-handed Sugars in DNA and RNA: right-handed Louis Pasteur ( ) animogroup carboxylgroup

16 Racemic mixture (from lecture of Antoine Weiss) Racemization  dating method

17 Chirality and origin of life Dead stuff not chiral, so is chirality –with racemic mixture: structure fragile Importance: –Prerequisite of life (provides curvature and twist) –Consequence of life (enzymatic reactions) Miller-Urey amino acids: both chiralities –in Murchison meteorite: mostly left-handed! –but contamination is debated… Reasons discussed: circularly polarized light, beta- decay (weak force), homochiral template

18 Relevant experiments: nucleotides template-directed oligomerization poly (C D )  oligo (G D )  Mononucleotides with wrong Chirality terminate chain growth cytosine guanine ok poisoned Joyce, et al. (incl. Orgel) (1984) (using HPLC)

19 Contergan: was sold as racemic mixture causes misformations Cures morning sickness during pregnancy (abundaned in December 1961)

20 Relevant experiments: crystals Crystal growth with stirring: primary nucleation suppressed Crystal growth, many different nucleation sites: racemic mixture Autocatalytic self-amplification? Frank (1953), Goldanskii & Kuzmin (1989), …

21 Model by Saito & Hyuga (Jan 2004) Bimodal behavior

22 Model by Sandars (Dec 2003, OLEB) Reaction for left-handed monomers Loss term for each constituent

23 Combined equations Loss term for each constituent

24 Including enantiomeric cross-inhibition Loss term for each constituent Racemic solution ~2 1-n

25 Coupling to substrate S Q L comes from substrate acts as a sink of S S sustained by source Q Catalytic properties of substrate (depending on how much L and R one has)  Q L = Q R (L n,R n ) Source of L 1 monomers Q L

26 Self-catalytic effect Form of Q L = Q R (L n,R n ) Possible proposals for C L (similarly for C R )

27 Birfurcation properties  Mononucleotides with wrong Chirality terminate chain growth

28 Stability Relative perturbation of racemic solution, 10 -4

29 Conservation law Dependence on fidelity where

30 Differences to Sandars Coupling to substrate: here proportional to E L –in Sandars: [L N ] Outer boundary condition: here open –in Sandars: prescribed damping term Future extensions: –Chain braking –add spatial 3D dynamics

31 Reduced equations Quantitatively close to full model

32 Initial bias Effect in reality very weak

33 Conclusions There are many astrobiology topics where astrophysicists can help out with their knowledge, as well as technical and computational tools Homochirality is a hot one with several papers this topic in each issue of OLEB