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Speciation I. Modes II. Mechanisms A. Progressive Genomic Incompatibility

Speciation I. Modes II. Mechanisms A. Progressive Genomic Incompatibility B. Hybrid Incompatibility C. Differential Selection D. Hybridization E. Polyploidy. E. Polyploidy. Autopolyploidy. Allopolyploidy. E. Polyploidy. Allopolyploidy. Spartina

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Speciation I. Modes II. Mechanisms A. Progressive Genomic Incompatibility

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  1. Speciation I. Modes II. Mechanisms A. Progressive Genomic Incompatibility B. Hybrid Incompatibility C. Differential Selection D. Hybridization E. Polyploidy

  2. E. Polyploidy Autopolyploidy Allopolyploidy

  3. E. Polyploidy Allopolyploidy Spartina Spartina alternifolia, native to US,was found in southern England in late1800's. There is a European species Spartina maritima. Early in the 20th century a sterile hybrid was found and was called Spartina townsendii This went through a process of diploidization (increased ploidy) and became a new sexually reproducing species known as Spartina anglica S. maritima sterile hybrid S. anglica S. alterniflora

  4. E. Polyploidy Allopolyploidy

  5. Speciation I. Modes II. Mechanisms III. Rates

  6. III. Rates Mark Pagel,* Chris Venditti, Andrew Meade .2006. Large Punctuational Contribution of Speciation to Evolutionary Divergence at the Molecular Level . Science 314:119. A long-standing debate in evolutionary biology concerns whether species diverge gradually through time or by punctuational episodes at the time of speciation. We found that approximately 22% of substitutional changes at the DNA level can be attributed to punctuational evolution, and the remainder accumulates from background gradual divergence. Punctuational effects occur at more than twice the rate in plants and fungi than in animals, but the proportion of total divergence attributable to punctuational change does not vary among these groups. Punctuational changes cause departures from a clock-like tempo of evolution, suggesting that they should be accounted for in deriving dates from phylogenies. Punctuational episodes of evolution may play a larger role in promoting evolutionary divergence than has previously been appreciated.

  7. Origin of Life Hypotheses

  8. I. Earth History 4.5 bya: Earth Forms

  9. I. Earth History - Earliest Atmosphere - probably of volcanic origin Gases produced were probably similar to those created by modern volcanoes (H2O, CO2, SO2, CO, S2, Cl2, N2, H2) and NH3 and CH4

  10. I. Earth History 4.0 bya: Oldest Rocks 4.5 bya: Earth Forms

  11. I. Earth History 4.0 bya: Oldest Rocks 3.5 bya: Oldest Fossils 4.5 bya: Earth Forms

  12. I. Earth History 4.0 bya: Oldest Rocks 3.5 bya: Oldest Fossils 4.5 bya: Earth Forms Stromatolites - communities of layered 'bacteria'

  13. I. Earth History 2.3-2.0 bya: Oxygen in Atmosphere 4.0 bya: Oldest Rocks 3.4 bya: Oldest Fossils 4.5 bya: Earth Forms

  14. I. Earth History 2.3-2.0 bya: Oxygen 1.8 bya: first eukaryote 4.0 bya: Oldest Rocks 3.4 bya: Oldest Fossils 4.5 bya: Earth Forms

  15. I. Earth History 2.3-2.0 bya: Oxygen 0.9 bya: first animals 1.8 bya: first eukaryote 4.0 bya: Oldest Rocks 3.4 bya: Oldest Fossils 4.5 bya: Earth Forms

  16. I. Earth History 2.3-2.0 bya: Oxygen 0.9 bya: first animals 1.8 bya: first eukaryote 0.5 bya: Cambrian 4.0 bya: Oldest Rocks 3.4 bya: Oldest Fossils 4.5 bya: Earth Forms

  17. I. Earth History 2.3-2.0 bya: Oxygen 0.9 bya: first animals 1.8 bya: first eukaryote 0.5 bya: Cambrian 0.24 bya:Mesozoic 4.0 bya: Oldest Rocks 3.4 bya: Oldest Fossils 4.5 bya: Earth Forms

  18. I. Earth History 2.3-2.0 bya: Oxygen 0.9 bya: first animals 1.8 bya: first eukaryote 0.5 bya: Cambrian 0.24 bya:Mesozoic 0.065 bya:Cenozoic 4.0 bya: Oldest Rocks 3.4 bya: Oldest Fossils 4.5 bya: Earth Forms

  19. I. Earth History 4.5 million to present (1/1000th of earth history) 2.3-2.0 bya: Oxygen 0.9 bya: first animals 1.8 bya: first eukaryote 0.5 bya: Cambrian 0.24 bya:Mesozoic 0.065 bya:Cenozoic 4.0 bya: Oldest Rocks 3.4 bya: Oldest Fossils 4.5 bya: Earth Forms

  20. II. Origin of Life Hypotheses - Oparin-Haldane Hypothesis (1924): - in a reducing atmosphere, biomonomers would form spontaneously Aleksandr Oparin (1894-1980) J.B.S. Haldane (1892-1964)

  21. II. Origin of Life Hypotheses - Oparin-Haldane Hypothesis (1924): - in a reducing atmosphere, biomonomers would form spontaneously - Miller-Urey (1953) all biologically important monomers have been produced by these experiments, even while changing gas composition and energy sources

  22. II. Origin of Life Hypotheses - Oparin-Haldane Hypothesis (1924): - in a reducing atmosphere, biomonomers would form spontaneously - Miller-Urey (1953) - Sydney Fox - 1970 - polymerized protein microspheres

  23. II. Origin of Life Hypotheses - Oparin-Haldane Hypothesis (1924): - in a reducing atmosphere, biomonomers would form spontaneously - Miller-Urey (1953) - Sydney Fox - 1970 - polymerized protein microspheres - Cairns-Smith (1960-70) - clays as templates for non-random polymerization - 1969 - Murcheson meteorite - amino acids present; some not found on Earth. To date, 74 meteoric AA's. - 2004 - Szostak - clays could catalyze formation of RNA's

  24. III. Acquiring the Characteristics of Life A. Three Primary Attributes: - Barrier (phospholipid membrane) - Metabolism (reaction pathways) - Genetic System

  25. III. Acquiring the Characteristics of Life B. Barrier (phospholipid membrane) - form spontaneously in aqueous solutions

  26. III. Acquiring the Characteristics of Life C. Metabolic Pathways - problem: how can pathways with useless intermediates evolve? These represent 'maladaptive valleys', don't they? A B C D E How do you get from A to E, if B, C, and D are non-functional?

  27. III. Acquiring the Characteristics of Life C. Metabolic Pathways - Solution - reverse evolution A B C D E

  28. III. Acquiring the Characteristics of Life C. Metabolic Pathways - Solution - reverse evolution suppose E is a useful molecule, initially available in the env. E

  29. III. Acquiring the Characteristics of Life C. Metabolic Pathways - Solution - reverse evolution suppose E is a useful molecule, initially available in the env. As protocells gobble it up, the concentration drops. E

  30. III. Acquiring the Characteristics of Life C. Metabolic Pathways - Solution - reverse evolution Anything that can absorb something else (D) and MAKE E is at a selective advantage... D E

  31. III. Acquiring the Characteristics of Life C. Metabolic Pathways - Solution - reverse evolution Anything that can absorb something else (D) and MAKE E is at a selective advantage... but over time, D may drop in concentration... D E

  32. III. Acquiring the Characteristics of Life C. Metabolic Pathways - Solution - reverse evolution So, anything that can absorb C and then make D and E will be selected for... C D E

  33. III. Acquiring the Characteristics of Life C. Metabolic Pathways - Solution - reverse evolution A B C D E and so on until a complete pathway evolves.

  34. III. Acquiring the Characteristics of Life D. Genetic Systems - conundrum... which came first, DNA or the proteins they encode? DNA RNA (m, r, t) protein

  35. III. Acquiring the Characteristics of Life D. Genetic Systems - conundrum... which came first, DNA or the proteins they encode? DNA DNA stores info, but proteins are the metabolic catalysts... RNA (m, r, t) protein

  36. III. Acquiring the Characteristics of Life D. Genetic Systems - conundrum... which came first, DNA or the proteins they encode? - Ribozymes info storage AND cataylic ability

  37. III. Acquiring the Characteristics of Life D. Genetic Systems - conundrum... which came first, DNA or the proteins they encode? - Ribozymes - Self replicating molecules - three stage hypothesis

  38. IV. Early Life - the first cells were probably heterotrophs that simply absorbed nutrients and ATP from the environment. - as these substances became rare, there was strong selection for cells that could manufacture their own energy storage molecules. - the most primitive cells are methanogens, but these are NOT the oldest fossils.

  39. IV. Early Life - the second type of cells were probably like green-sulphur bacteria, which used H2S as an electron donor, in the presence of sunlight, to photosynthesize.

  40. IV. Early Life - the evolution of oxygenic photosynthesis was MAJOR. It allowed life to exploit more habitats, and it produced a powerful oxidating agent! These stromatolites, which date to > 3 bya are microbial communities.

  41. IV. Early Life - about 2.3-1.8 bya, the concentration of oxygen began to increase in the ocean and oxidize eroded materials minerals... deposited as 'banded iron formations'.

  42. IV. Early Life - 2.0-1.7 bya - evolution of eukaryotes.... endosymbiosis.

  43. IV. Early Life Eukaryote Characteristics - membrane bound nucleus - organelles - sexual reproduction

  44. infolding of membrane IV. Early Life Origins

  45. IV. Early Life endosymbiosis - mitochondria and chloroplasts (Margulis - 1970's) B. Origins

  46. IV. Early Life Relationships among life forms - deep ancestry and the last "concestor"

  47. IV. Early Life Woese - r-RNA analyses reveal a deep divide within the bacteria

  48. IV. Early Life

  49. IV. Early Life

  50. IV. Early Life Curiously, the very root of life may be invisible to genetic analysis. Bacteria transfer genes by division (to 'offspring'), but they also transfer genes "laterally" to other living bacteria. This makes reconstructing bacterial phylogenies difficult.

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