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Organic Chemistry Basics And Perspectives

Organic Chemistry Basics And Perspectives. Paradoxes in the Biochemistry of Living Systems. Darwinian evolution implies “best” chemical solutions for life Life did not necessarily choose the “best” Many alternative chemical possibilities

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Organic Chemistry Basics And Perspectives

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  1. Organic Chemistry Basics And Perspectives

  2. Paradoxes in the Biochemistry of Living Systems • Darwinian evolution implies “best” chemical solutions for life • Life did not necessarily choose the “best” • Many alternative chemical possibilities • WHY only 20 amino acids in living systems ? •  Other amino acids work in proteins • WHY only four base pairs in DNA, RNA ? •  Other base pairs equally effective • WHY ribose and deoxyribose in DNA, ATP ? •  Why not glycerol, a hexose or a tetrose? • Terrestrial Life evolved quickly not time to sample all chemical possibilities • Life must reflect what was present by chance SYNTHETIC CONTINGENCY

  3. DNA • Ribose: • Key sugar in DNA • ALTERNATIVES • TO RIBOSE ??

  4. Many alternatives • to ribose in DNA and RNA • Other sugars also form • Watson-Crick base pairs • Hexoses as well as pentoses • Many pentoses • Ribose unlikely candidate • Formation in Formose Reaction (H2CO(aq) in base) • - One of numerous sugars produced w/o SELECTIVITY • - Mechanism of 1 + 1 carbon addition still uncertain • Decomposes in water under neutral, acidic, basic conditions • Other sugars could do the job…

  5. Thymine- Adenine base pair: 2 hydrogen bonds • Thymine-Amino-adenine base pair: 3 hydrogen bonds • Three hydrogen bonds better than two ? What established the synthetic contingencies (i.e. STARTING MATERIALS that led to life on Earth ???)

  6. e • Earth originated with the formation of the solar system • Solar system formed in a molecular cloud

  7. Solar system formed • from a molecular cloud • 4.6 Gyr ago • Remnant cloud: Oort Cloud • Full of interstellar debris • Solar system left with • Molecular Cloud debris

  8. The Problems with Carbon • Starting materials were just “here” on Earth • Miller-Urey type synthesis • Electrical discharge of CH4, NH3, H2O, H2 • Produced racemic mixers of amino acids • But… problems with simple picture • Earth lost early atmosphere, including carbon-bearing species CO2, CH4, etc. • No evidence for carbon in early crust • Uncertain if any primordial carbon survived • Carbon brought back through exogenous delivery (FROM SPACE) • Bombardment by meteorites, comets, interplanetary dust particles • Probably in period of Late Heavy Bombardment (4.2 – 3.8 Gyr ago)

  9. And Even More Problems with Carbon… • What form did the carbon return to Earth ? • Meteorites, IDP’s, comets suggest in organic compounds, polymer material • Where did these organic compounds originate ? • In Galaxy, O > C (factor of ~ 1.5) • Carbon should be mainly contained in CO • CO: • VERY abundant interstellar molecule • Organic chemistry: should not occur • Objects in the Galaxy: C >O • Carbon-rich stars and their ejecta • Forming solar systems: need to be • near such stars for organic chemistry ??

  10. Our Galaxy in Molecules Columbia-CfA Project CO 1-0 All Sky Survey • Molecular Gas is Widespread in the Galaxy Our Galaxy at Optical Wavelengths • Molecular clouds largest well-defined objects in Galaxy (1 -106 Mass of sun) • 50% of matter in inner 10 kpc is MOLECULAR (~1010 Solar Masses) • Molecular clouds are rich in simple organic molecules

  11. 2 3 4 5 6 7 8 9 10 H2 CH+ H2O C3 NH3 SiH4 CH3OH CH3CHO CH3CO2H CH3CH2OH CH3COCH3 OH CN H2S HNC H3O+ CH4 NH2CHO CH3NH2 HCO2CH3 (CH3)2O CH3(CC)2CN SO CO SO2 HCN H2CO CHOOH CH3CN CH3CCH CH3C2CN CH3CH2CN (CH2OH)2 H(CC)3CN HCCCN SO+ CS NNH+ CH2 H2CS CH3NC CH2CHCN C7H H(CC)2CH3 H(CC)2CN SiO C2 HNO NH2 HNCO CH2NH CH3SH H2C6 SiS SiC CCS HOC+ HNCS NH2CN C5H C6H CH2OHCHO C8H NO CP NH2 NaCN CCCN H2CCO HC2CHO c-CH2OCH2 H(CC)4CN NS CO+ H3+ MgNC HCO2+ C4H CH2=CH2 H2CC(OH)H HCl HF NNO AlNC CCCH c-C3H2 H2C4 NaCl SH HCO SiCN c-C3H CH2CN HC3NH+ KCl HD HCO+ SiNC CCCO C5 C5N H(CC)5CN AlCl OCS H2D+ C3S SiC4 11 AlF CCH MgCN HCCH H2C3 PN HCS+ KCN HCNH+ HCCNC SiN c-SiCC HCCN HNCCC NH CCO H2CN H2COH+ CH c-SiC3 12 13 Known Interstellar Molecules C8H- CH3CONH2 C6H- PO ~100 Carbon Molecules 11 Silicon Species 9 Metal Containing Molecules 5 Phosphorus Species HCP CCP C4H- ~ 90% Identified by Radio Astronomy

  12. Purpose of Course • Life started from chemical reactions • Need to determine starting materials: astronomy, geology, planetary science • Need to determine physical conditions in which reactions occurred: • planetary science and geology • Life requires carbon • How did the carbon get back to Earth and in what form • How is an environment created where organic compounds can form and • flourish • With such a large amount of interstellar molecular material, did interstellar • and pre-solar nebula chemistry influence the ORIGIN of LIFE ?? • But still need some chemical basics….

  13. Biochemistry Basics • Chemical reactions: use heat; acid, base catalysts • Biochemical reactions: use enzymes as catalysts • Enzymes are Proteins • Typical mammal muscle: • 72 – 80% Water • 1% Carbohydrate • 17 – 21% Proteins • 5% Lipids (“Fats”) • 0.3 % Nucleic Acids • 1% Minerals (Metals)

  14. Carbohydrates • Sugars and starches • Polyhydroxy aldehydes and ketones with formula Cm(H2O)n • m > 1 or 2 (excludes H2CO) • May include glycolaldehyde • Carbohydrates can be classifieds as: • Monosaccharides • Disaccharides • Polysaccharides • Monosaccharides • Cannot be HYDROLIZED to smaller carbohydrates • Single carbon chain with two or more hydroxyl groups. • General formula (C•H2O)n • Example: D-Glucose D-glucose Fischer projection

  15. Classified according to three different characteristics: • placement of its CARBONYL group • number of CARBON atoms • -CHIRALITY (right of left-handedness: D or L) • Aldose from an aldehyde • Ketose from a ketone • Triose: 3 carbon atoms • Tetrose has 4 C atoms • Pentose has 5 C atoms • Hexose has 6 C atoms, etc • Glucose: aldohexose; Ribose an aldopentose • Each C atom with -OH group asymmetric, with exception of first & last C’s • Each asymmetric carbon a Stereo center; generates isomers • Glucose has 16 isomers, depending on orientation of OH groups D-Glucose

  16. Monosaccharides have straight-chain and ring form (Glucose) • Rings form: aldehyde or ketone group of straight-chain monosaccharide • reacts reversibly with hydroxyl group on different carbon atom • Forms a hemiacetal (aldehyde) or hemiketal (ketone) • Creates ring structure with oxygen bridge between two C atoms • Rings with 5 and 6 atoms are called furanose and pyranose hemiacetal hemiketal

  17. Pyranose Furanose

  18. Conversion from straight-chain to cyclic form • C atom with carbonyl oxygen (anomeric C) becomes stereogenic center • Generates two possible configurations: • O atom above or below plane of the ring • Have pair of stereoisomers: anomers • α anomer, the -OH group on anomeric carbon rests (TRANS) on opposite side of ring from the CH2OH side branch • β anomer: CH2OH substituent and the anomeric – OH on same side (CIS) of plane of ring

  19. Disaccharides and Polysaccharides • Mono groups joined together • 1-4, 1-6, 1-3 linkages; alpha and beta • Loss of H on –OH group: glycosidic bond • Sucrose: D-glucose and D-fructose • O-α-D-glucopyranosyl-(1→2)-D-fructofuranoside

  20. Proteins • High molecular weight substances • Upon hydrolysis yield amino acids • One or more polypeptides typically folded into globular or fibrous form • Polypeptide: single linear polymer chain of amino acids • Peptide Bond between the carboxyl and NH2groups of adjacent amino acids • Have non-peptide groups attached (co-factors, prosthetic groups, co-enzymes) L-Alanine Simple Amino Acids Glycine

  21. Example Protein: Myoglobin • Turquoise strands: eight alpha helices • Alpha Helix: right-handed coiled or spiral • Every backbone N-H group hydrogen bonds to backbone carbonyl group of amino acid four “residues” earlier • Among coils: HEME prosthetic group • Red: bound oxygen molecule • Myoglobin related to hemoglobin • Oxygen carrier in muscles of • mammals Heme

  22. Proteins have many functions in living systems • Enzymes that catalyze biochemical reactions • Vital to Metabolism • Also have structural or mechanical functions • Actin in muscle • Form scaffolding cytoskeleton that maintains cell shape • Important in cell signaling, immune responses • Protein: complete biological molecule in stable conformation • Peptide: short amino acid oligomer lacking stable 3-D structure • Polypeptide: single linear chain of amino acids, absence of • defined conformation • Consist of 20 standard amino acids • Certain organisms have selenocysteine • Certain archaea—pyrrolysine. Alpha-helix

  23. 20 different L-α-AMINO ACIDS • Possess common structural features • Alpha C to which NH2, C=O, and variable side chain are bonded • Proline differs • An unusual ring to the N-end amine group • Forces the CO–NH amide moiety into a fixed conformation • Side chains: great variety of chemical structures and properties • Combined effect of all amino acid side chains in a protein • Determines its three-dimensional structure and its chemical reactivity • An individual amino acid in a protein is residue • Linked series of carbon, nitrogen, and oxygen atoms: • main chain or protein backbone • End of protein with a free carboxyl group: C-terminus or carboxy terminus • End with a free amino group: N-treminus or amino terminus.

  24. Structure of Proteins • Four distinct levels of protein structure • PRIMARY • Amino acid linear sequence of the polypeptide chain (No branches) • Held together by peptide (covalent) bonds • Made during the process of translation from m-RNA • Sequence amino acids is unique and defines structure/function of protein

  25. SECONDARY • Highly regular local sub-structures caused by hydrogen bonding • Bonds form between main-chain peptide groups (N-H and C=O groups) • Two main types: alpha helix and beta strand and sheets • Other ordered but not regular patterns • Alpha Helix: every backbone N-H group • H-bonds to backbone C=O group • Bonds occur between every 4th residue • Beta strand: Polypeptide chain 3 to 10 amino acids long • with fully extended backbone • Beta sheets: beta strands connected laterally • by at least two or three backbone H-bonds • Form twisted, pleated sheets

  26. H-bonds N-H C=O Beta Sheet 2nd common structure Beta Strands Alpha Helix Most common structure

  27. TERTIARY • 3-D protein structure • Alpha-helices and beta-sheets folded into compact globule • Folding caused by non-specific hydrophobic interactions • Certain functional groups avoid water (solvent) • Folding locked into place by specific tertiary interactions • Include Ionic (“salt-bridges”) and Hydrogen bonds • Tight packing of side chains (strain/steric hindrance) • Disulfide bonds Tertiary structure t-RNA Di-sulfide Bond

  28. Typical tertiary structures Globular (Hemoglobin) Membrane Imbedded or Peripheral (Potassium channel KvAP) Fibrous (Collagen)

  29. QUATERNARY • Proteins may consist of several sub-units (polypeptides chains) • 3-D structure of a multi-subunit protein • Subunits stabilized by same non-covalent interactions and disulfide bonds as tertiary structure • Hemoglobin, DNA polymerase have such structure DNA polymerase

  30. Proteins: may shift between several structures • Change in tertiary or quaternary structures • Necessary to perform their specific functions • Such structures: “conformations” Insulin Hexamer, bound by Zinc

  31. Lipids and Fats • Lipids: diverse class of compounds • Small Hydrophobic (dislike water) molecules • Consist of non-polar aliphatic chains • Used in energy storage, membrane structure and cell signaling • Fats and Oils: Triglycerides of fatty acids (Glycerolipids) • Fatty Acids • Soaps and Detergents • Waxes • Phospholipids • Steroids

  32. Fatty Acids • Carboxylic Acid with a long aliphatic chain (saturated or unsaturated) • C-chain usually 4 to 24 carbons long (even # of carbons) • Chain may have functional groups with O, N, and S, also Cl • Branched chains rare in animals and higher plant life • Hydrophobic (non-polar: carbon chain) and hydrophilic (water-loving: acid • group) ends • Essential fatty acids for human body: • Linolenic acid (LA) and alpha-linolenic acid (ALA) • Used to create fats and oils by esterification

  33. Fats and Oils • Created by reaction of glycerol and fatty acid: ESTERS • Most common lipids • Primary energy storage in animals; provide insulating layers • Most common biochemical reaction: Hydrolysis • Waxes: Esters of fatty acid • with simple alcohol

  34. Phospholipids • Lipids that contain phosphorus • Prevalent in brain and nervous tissue • Common phospholipid: lecithin in egg yolks • Glycerol-based phospholipids: phosphoglycerides • Glycerol with 2 fatty acids and 1 phosphonic acid attached • Main components of biological membranes • Membranes: bilipid layers • Two non-polar carbon chain tails orient inward • Phosphorus (polar) head faces outward

  35. Nucleic Acids • “Nucleic” because originally found in cell nucleus • Like proteins, important biological macromolecules • Include DNA (deoxyribonucleic acid) and RNA (ribonucleic acid) • Other “artificial” nucleic acid analogs: “pepide” and “threose” nucleic acids • Basic unit: Nucleotide • Contains pentose sugar (Ribose; dioxyribose), phosphate group, nucleobase • Also called “polynucleotides” • 21 nucleotides (small interfering RNA) to 247 million nucleotides (Human • Chromosome 1) Pentose Sugar Nucleobases Phosphate

  36. Usually DNA double-stranded; RNA single-stranded • DNA contains 2‘-deoxyribose • RNA contains ribose • Difference is the presence of -OH group • Nucleobases in DNA and RNA different: • Adenine, cytosine, guanine in both • RNA and DNA, • Thymine in DNA and Uracil in RNA • Sugar + base = nucleoside ribose 2‘-deoxyribose

  37. cytosine uracil thymine Purines 2 rings Pyrimidines 3 rings Nucleoside H2O lost (OH off sugar, H off the nitrogen)

  38. More on the DNA and RNA Structure • Sugars and phosphates connect to each other in alternating chain • Creates “sugar-phosphate” backbone • Phosphodiester linkages with 3'-end and the 5'-end carbons of sugar • Gives nucleic acid Directionality • Nucleobases joined to sugars via • N-glycosidic linkage • Involves nucleobase ring nitrogen • N-1 for pyrimidines and N-9 for purines • 1' carbon of the pentose sugar ring • In DNA, two strands linked by • Hydrogen Bonding • Occurs between a base pair • (Watson-Crick base-pairing)

  39. Adenine (A) forms base pair with Thymine (T) with 2 H bonds • Guanine (G) forms base pair with Cytosine (C) with 3 H bonds • In RNA, Thymine is replaced by Uracil (U) • Alternate H bonding patterns in RNA: result in complex tertiary structures • Purines complementary only with pyrimidines • Pyrimidine-pyrimidine pairings unfavorable: molecules are too far apart • No H-bonding can occur • Purine-purinepairings are unfavorable: molecules too close (steric problem) • Other pairings (AC, GT, UA ) mismatches, except GU in RNA Uracil

  40. Most stabilization due to packing • Hydrogen bonds only • partially help • G-C most stable: 3 H bonds • More G-C pairs, more stable DNA • Can see Major and Minor grooves in Helix • Adjacent to a base pair • Provide binding site

  41. Strands are not directly opposite each other; grooves unequally sized • Major groove: 22 Å wide; the minor groove:12 Å wide • Edges of bases more accessible in major groove • Where transcription factors attach

  42. DNA Structures • Three known structures: only B and Z in living organisms • DNA twisted like rope: supercoiling (A and Z) • More twisted, more H-bonding • Inverse twisting: weakens H-bonding • Enzymes help in coiling • Twist to weaken H-bond • Start replication A B Z

  43. Alternate hydrogen bonding patterns • Such as wobble base pair • guanine-uracil, inosine-uracil, inosine-adenine, • inosine-cytosine • RNA: gives rise to complex tertiary structures • Functional RNA’s are not floppy strands • Folded, stable molecules with three-D shapes • Cations essential for thermodynamic stabilization • of RNA tertiary structures • K+, Mg2+,Mn2+,Na+, Ca2+ • Also get triple-stranded RNA (rarely observed)

  44. RNA Triplex Catalytic RNA

  45. Certain enzymes recognize specific base pairing patterns • Identify particular regulatory regions of genes • Size of an individual Gene or Genome measured in base pairs • Haploid human genome (23 chromosomes) about 3.2 billion base pairs long • Contains 20,000–25,000 distinct genes • DNA used to construct Proteins (amino acid polymers) • Codon: corresponds to single amino acid • DNA transcribed to mRNA in cell nucleus • mRNA travels to cytoplasm • Each possible combination of three • bases corresponds to specific amino acid • GCA: alaine • Proteins constructed

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