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Raven biology 13th edition, CH25
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Deep Time, Geologic time is divided into four eons
Eons are subdivided into eras, which are further subdivided into periods
Deep Time, Geological evidence suggests a meteor hit the earth 4.6 billion years ago
No rocks exist from Hadean eon (first 500 to 700 million years of Earth's history
Deep Time, Hadean Earth was pummeled by asteroids
Could potentially vaporize entire oceans
Deep Time, When meteor hit, debris formed the moon and the rocky mantle melted
Temperatures exceeded 2000° C
Changes in Earth in geological time, CO levels shifted and affected temperature
Early atmosphere high CO levels
Changes in Earth in geological time, Water slowly vaporized
From the molten rock
Changes in Earth in geological time, Increased weathering converted
Silicate rock to soil
Changes in Earth in geological time, CO formed carbonic acid
Carbonic acid released bicarbonate ions (HCO₃⁻) and Ca²⁺ from rock
Changes in Earth in geological time, Decreases in CO
Lowered Earth's temperature
Weathering rocks pull CO₂ from the atmosphere, Weathering rocks pull CO₂ from the atmosphere
Process that removes CO₂ from the atmosphere
Continents moved over geological time, Earth's crust formed rigid slabs of rock called plates
Under continents and oceans
Continents moved over geological time, Two ( important) supercontinents formed
Rodinia (all continents) and Pangea ( separating continents)
Continents moved over geological time, Pangea formed
From Gondwana
Life emerged in the Archean eon, Proterozoic ("early life") eon occurred
Two billion years into Earth's history
Life emerged in the Archean eon, Proterozoic eon was characterized by
Formation of Rodinia
Life emerged in the Archean eon, Rodinia broke up before Phanerozoic eon
Cambrian period showed diversification of multicellular organisms
Life emerged in the Archean eon, Birds and mammals have existed for
4% of earth's existence
Life emerged in the Archean eon, Humans present for
0.2% of earth's history, or 1 second of earths time
Early organic molecules, How first organic molecules formed is not known
Hundreds of thousands of meteorites and comets slammed into early earth; some may have carried organic materials
Early organic molecules, Alternatively
Organic molecules may have originated on early earth
Early Earth's atmosphere, Few geochemists agree on
exact composition of early atmosphere, popular view of early atmosphere
Early Earth's atmosphere, Popular view includes
Carbon dioxide, Nitrogen gas, Water vapor , Hydrogen gas , and other sulfur, nitrogen, and carbon compounds
CO₂, N₂, H₂O, H₂, an S, N , C compounds
Early Earth's atmosphere, Atmosphere was reducing
Because of availability of hydrogen atoms and their electrons
Miller-Urey experiment, In 1953, Miller and Urey did an experiment that reproduced early atmosphere
Assembled reducing atmosphere rich in hydrogen with no oxygen gas
Miller-Urey experiment, Atmosphere placed over
Liquid water
Miller-Urey experiment, Temperature below
100°C
Miller-Urey experiment, Simulated lightning with
Sparks
Miller-Urey experiment, Found within a week that methane gas (CH₄) converted into
Other simple carbon compounds
Miller-Urey experiment, Compounds combined to form
Simple molecules and then more complex molecules
Miller-Urey experiment, Later experiments produced
More than 30 carbon compounds including amino acids
Miller-Urey experiment, Adenine is
also produced
Miller-Urey experiment, Concluded that key molecules of earth could have formed
On early Earth
Evolution of metabolism, Primitive organisms may have been
Autotrophic or heterotrophic
Evolution of metabolism, Landmarks in the evolution of metabolism include
Oxygenic photosynthesis, Carbon fixation, and Nitrogen fixation
Evolution of metabolism, RNA may have been first
Genetic material
Evolution of metabolism, Lipid bubbles could increase the probability of
Metabolic reactions
Evolution of metabolism, Leads to
Cell membranes
Evolution of metabolism, Single-celled organism the first
Life-form
Conditions on early Earth, Seems likely that Earth's first organisms emerged and lived at
Very high temperatures
Conditions on early Earth, Around 3.8 BYA ocean temperatures dropped to
49° to 88° C
Conditions on early Earth, First organisms
emerged around this time
Fossil evidence of life, Evidence of life during the Archean in the form of microfossils is
Difficult to find and interpret
Fossil evidence of life, Two main formations of 3.5- to 3.8- billion-year-old rocks have been found
Kaapvaal craton (South Africa) and Pilbara craton (Australia)
Fossil evidence of life, Structures in each interpreted to be
Biological in origin
Microfossils, Microfossils are fossilized forms of
Microscopic life
Microfossils, Oldest are 3.5 billion years old
Seem to resemble present-day prokaryotes
Microfossils, Fossils from 3.2 BYA could be
Eukaryotic cells but probably cyanobacteria
Stromatolites, Stromatolites are mats of cyanobacterial cells that
Trap mineral deposits
Stromatolites, Indirect evidence for
Ancient life
Stromatolites, Oldest are
2.7 billion years old
Stromatolites, Modern forms are also
Known
Isotopic data, Living organisms incorporate ¹²C into their cells
Before other carbon isotopes
Isotopic data, Work has been done dating and analyzing carbon compounds in the oldest rocks
Looking for evidence of life
Isotopic data, Carbon fixation active as long as
3.8 BYA
Isotopic data, Ancient carbon fixation via
Calvin cycle or a reductive version of the citric acid cycle
Isotopic data, Ability to fix carbon has evolved
More than once
Biomarkers, Look for evidence of
Ancient organic molecules of biological origin
Biomarkers, Simple in theory but
Difficult to find
Biomarkers, Hydrocarbons derived from fatty acid tails of lipids were found in
Ancient rocks
Biomarkers, Analyzed for carbon isotope ratios to indicate
Biological origin
Biomarkers, Indicates that cyanobacteria are at least
2.7 billion years old
Earth's Changing System, Climate (temperature and water availability) and atmosphere among many factors that
Affect organisms' survival
Earth's Changing System, Dramatic shifts in all these factors led to
Mass extinctions influencing the course of evolution
Earth's Changing System, Earth has been cooling since its
Formation
Earth's Changing System, Extreme drops in temperature resulted in
Glacial ice covering Earth, "Snowball Earth"
Shifts in atmosphere, Geological changes explain many changes in
Atmosphere
Shifts in atmosphere, Hot wet climate of tropics accelerated
Weathering
Shifts in atmosphere, Snowball Earth decreased temperature and slowed
Weathering
Shifts in atmosphere, Plate tectonics can also affect
Weathering and atmospheric levels of CO₂
Continental motion affected evolution, Continents sit on submerged plates that are
In motion
Continental motion affected evolution, Shifting plates affect evolution by
Reproductively isolating populations or allowing previously separate populations to interbreed
Continental motion affected evolution, Cenozoic era began
66 mya
Continental motion affected evolution, Australia and Antarctica separated, as did
Greenland and North America
Continental motion affected evolution, The Atlantic Ocean continued to grow as
Plates in the mid-Atlantic spread
Continental motion affected evolution, Greenhouse conditions during Cretaceous period led to
A rise in sea level and continental areas were submerged
Life changes Earth 1, Oxygenic photosynthesis produced atmospheric O₂
200-million-year lag between the origins of photosynthesis and substantial levels of O₂
Life changes Earth 1, Iron oxide in the
Oceans
Life changes Earth 1, O₂ in the atmosphere interacted with ultraviolet (UV) radiation from the Sun and formed
O₃ (ozone)
Life changes Earth 2, Did plants contribute to glaciations?
Growing evidence that plants contributed to two glaciations
Life changes Earth 2, Colonization of land by plants followed by
Gradual cooling and abrupt glaciation 488 to 444 mya
Life changes Earth 2, Vascular plants diversification concurrent with second glaciation
400 to 360 mya
Ever-Changing Life on Earth, Life evolved into three monophyletic domains
Eubacteria, Archaea, and Eukaryotes
Ever-Changing Life on Earth, Eukaryotes divided into 5 supergroups
Excavata, SAR (Stramenopila, Alveolata, and Rhizaria), Archaeplastida, Amoebozoa, Opisthokonta
Compartmentalization of cells, Compartmentalization of cells enabled the advent of
Eukaryotes
Compartmentalization of cells, Bacteria and archaea ruled the Earth for
1 billion years
Compartmentalization of cells, Bacteria and archaea are distinct from eukaryotes in that they have much less
Compartmentalization
Compartmentalization of cells, Eukaryotes developed an extensive
Endomembrane system
Evolution of endomembrane system, Infolding of the
Cellular membrane
Evolution of endomembrane system, Nuclear membrane, not found in bacteria and archaea, accounts for
Increased complexity in eukaryotes
Evolution of endomembrane system, Physical separation of transcription and translation adds additional levels of
Gene expression
Evolution of endomembrane system, Golgi apparatus and endoplasmic reticulum facilitate
Intracellular transport
Evolution of endomembrane system, Not all cellular compartments are derived from
Endomembrane system
Endosymbiosis and the origin of eukaryotes, Mitochondria and chloroplasts entered early eukaryotic cells by
Endosymbiosis
Endosymbiosis and the origin of eukaryotes, Mitochondria are the descendants of the parasite Rickettsia, incorporated into cells
Early in the evolution of eukaryotes
Endosymbiosis and the origin of eukaryotes, Chloroplasts are derived from
Cyanobacteria
Multicellularity leads to cell specialization, Unicellular body plan
Tremendously successful
Multicellularity leads to cell specialization, Unicellular prokaryotes and eukaryotes constitute about half of the
Biomass on Earth
Multicellularity leads to cell specialization, But a single cell has limits with
Cell specialization
Multicellularity leads to cell specialization, Multicellularity allowed organisms to deal with environment in novel ways through
Differentiation
Multicellularity leads to cell specialization 2, Multicellularity has arisen independently in
Different eukaryotic supergroups