topic 1: origins of life origin of the solar system earth is estimated to be ~4.6byo –radiometric...

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Topic 1: Origins of Life

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Page 1: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Topic 1: Origins of Life

Page 2: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Origin of the Solar System• Earth is estimated

to be ~4.6byo– Radiometric dating

of rocks & meteors• Nebula: cloud of

gas & dust in space• Nebula Hypothesis:

– Gravity pulled much material together (Sun formed)

– Planets: remaining materials

Page 3: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

• Hypothesis: Energy from lightning created organic materials from inorganic ingredients

• Experimental Set-Up:– Ammonia, H2O vapor,

Methane, CO2 gases added

– Electricity added (simulate lightning)

• Result: Amino Acids & later nucleotides

Page 4: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Geologic Change• Early belief:

– Earth ~6,000 years old– Life remained

unchanged• “New” Observations

– Rock layers contained differing fossils

– Deeper/older fossils less complex

– Environmental changes thought to affect life characteristics

Page 5: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Charles Darwin

• Observed:– Organisms have variations based upon environment– Some variations proved helpful in particular environment

• Natural Selection: Process where organisms with favorable traits survive and reproduce

• Major concept in biology published in The Origin of Species (1859)

Page 6: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Topic 2: The Theory ofNatural Selection

Page 7: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

• Four factors:1) Overpopulation: more offspring are born than can

survive2) Variation: individuals of a population have

differences3) Adaptation: Some variations allow better survival4) Descent w/ modification: Offspring w/ advantages

will make up more of a population

Page 8: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Which rabbit is best adapted?

Page 9: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Which rabbit is best adapted?

Page 10: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Struggle for Survival

• Populations do not grow unchecked– Limiting Factors: food, water, shelter, disease,

predators• Fitness: measure of the ability to survive &

produce more offspring

Page 11: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Changing Environments

• Earth’s environments gradually change– Mountains created– Ocean valleys dry up– Rivers create canyons

• Variations allow some to survive changing environments– With adaptation: more likely to survive & reproduce– Without adaptation: more likely to perish

Page 12: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Are new environments being created and destroyed?

Page 13: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Topic 3: The Evidence to

Support Evolution Theory

Page 14: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

• Defined: Collection of known fossils– Most found in sedimentary

rock

• Age determined by depth– Law of Superposition: new

rock forms on top of older rock

• Evidence Conclusions:– 1) Newer fossils are more

complex– 2) Common ancestors:

similarities between ancient & modern life

Page 15: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Radiometric Dating

• Isotopes: atoms of the same element with differing neutrons– Ex: 12Carbon and 14Carbon– 12C = 6 protons + 6 neutrons– 14C = 6 protons + 8 neutrons

• 14C decays at known rate• Fossil age determined by comparing ratio of 12C to 14C

– Wider ratio = older samples

Page 16: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust
Page 17: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

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Page 18: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

• Show transitions between groups of organisms– Archaeopteryx: shares both bird & reptile features– Basilosaurus: early whale with tiny hind legs– Tiktaalik: early fish with legs

• Evidence Conclusion : Indicates common ancestry

Page 19: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

• Defined: similar body structures with very different functions

• Different environments lead to adaptations– Ex: The forelimbs of animals

• Evidence Conclusion : Indicates common ancestry

Page 20: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

• Defined: Organs which have lost most or all their original function

• Vestigial Human Parts:– Gill slits = once used to breath oxygen in water– Yolk sac = once used to nourish developing embryo– Appendix = once used to digest plants

• Evidence Conclusion : Indicates common ancestry

Vestigial Structures

Page 21: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Human Embryo w/ Vestigial Structures

Page 22: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Snake femurs (leg bones) are vestigial

Page 23: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Pelvic bones of whales are vestigial

Page 24: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Nictitating membrane is vestigial in humans

Page 25: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

• DNA, proteins, & amino acids compared

• More related species have more similar chemistry

• Evidence Conclusion : Indicates common ancestry

Page 26: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

• Different species show similar development

• Different body plans become noticeable later in development

• Evidence Conclusion : Indicates common ancestry

Page 27: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

• Antibiotics: chemicals designed to kill bacteria

• Antibiotic Resistance: Bacteria are adapting to the use of antibiotics– Example of natural

selection– Importance: Bacteria

infections are becoming harder to treatFungus

Bacteria

No bacteria

Page 28: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust
Page 29: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Antibiotic Resistance

GoodBad

Page 30: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

• Pesticides: Chemicals designed to kill pests (rodents, insects)

• Pesticide Resistance: pests are adapting to the use of pesticides– Example of natural selection– Importance: Crops are being destroyed by pests

Page 31: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Topic 4: Speciation

Page 32: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Speciation• Defined: evolution of a new

species• Species: group of

organisms that can interbreed and produce fertile offspring

• Factors that lead to evolution– Natural Selection– Gene flow– Mutations– Sexual selection– Genetic drift

Page 33: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Gene Flow

• Defined: Movement of genes from 1 population to another

• Increases variations in a population (new genes introduced)

• If gene flow prevented– No variations exchanged– Populations isolated– Organisms adapt to their own environment

Page 34: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Genetic Drift

• Defined: Changes in gene pool due to chance (not natural selection)

• More likely in smaller populations• Ex: Natural disaster

– Pre-forest fire (left picture): Blue is more advantageous– Post-forest fire (right picture): Due to more red survivors, red has the

advantage to reproduce– Survival unrelated to adaptations; Random

Page 35: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Geographic Isolation

• Mountains, rivers, canyons, oceans may separate a population– Gene flow stopped

• Each population adapts to its isolated environment

• Over time, genetic differences accumulate between the groups

Page 36: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust
Page 37: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Behavioral Isolation

• Gene flow prevented due to different mating rituals

• Populations unable to reproduce• Differences accumulate between both groups

Page 38: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Temporal Isolation• Gene flow prevented

due to time interference–1) Mate at different

seasons–2) Some active at

night (nocturnal)• Differences

accumulate between both groups

Page 39: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Topic 5: Patterns in Evolution

Page 40: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Divergent Evolution

• Defined: closely related species become increasingly different

• Cause: Different environments• Ex: Red fox (forest) vs. Kit fox (desert)

Page 41: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Convergent Evolution

• Defined: different species evolve similar traits due to similar habitats

• Survival advantage to a particular environment • Ex: Tuna (fish) and dolphins (mammals)

– Unrelated species with a similar environment (ocean)– Faced similar evolutionary pressures

Page 42: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

Coevolution

• Defined: 2 or more species evolve in response to changes in each other

• Ex: Plants and Insects– Plants: provide insects with nectar– Insect: transfers pollen from one plant to another

Page 43: Topic 1: Origins of Life Origin of the Solar System Earth is estimated to be ~4.6byo –Radiometric dating of rocks & meteors Nebula: cloud of gas & dust

How Fast Does Evolution Occur?

• No exact time frame• Gradualism: slow & steady change of 1 species into another

– Small changes continually build• Punctuated Equilibrium: Rapid periods of evolution

– Due to sudden environment change– Ex: Mammal diversity exploded after dinosaur extinction

• Examples of both models exist