This document discusses the evolution of microbial life on Earth from its origins to the development of eukaryotic organisms. It describes how early Earth conditions allowed for the emergence of self-replicating molecules like RNA. Cellular life likely first arose in hydrothermal vents where conditions were stable. Early cells diversified metabolically, with some producing oxygen through photosynthesis. Accumulation of oxygen allowed for aerobic respiration and eukaryotic life, likely arising through endosymbiotic relationships between cells and oxygen-consuming or producing prokaryotes.
nitrate and sulfate reduction ; methanogenesis and acetogenesisjyoti arora
this powerpoint includes the following topics in brief:
1. Nitrate assimilatory reduction
2. Sulfate assimilatory reduction
3. Methanogenesis
4. Acetogenesis
Unit 6: Diversity of Microbial Mats
LECTURE LEARNING GOALS
1. Definemicrobialmats.Describethe functional guilds of microbes in the different layers, and how they interact.
2. Foreachofthethreephylaof photosynthetic bacteria, contrast how each fixes C and gains energy and reducing equivalents from light.
3. Forthetwothermophilicbacterialphyla, describe their adaptations to life at high
temperature. Explain how they are primitive and deeply-branching.
nitrate and sulfate reduction ; methanogenesis and acetogenesisjyoti arora
this powerpoint includes the following topics in brief:
1. Nitrate assimilatory reduction
2. Sulfate assimilatory reduction
3. Methanogenesis
4. Acetogenesis
Unit 6: Diversity of Microbial Mats
LECTURE LEARNING GOALS
1. Definemicrobialmats.Describethe functional guilds of microbes in the different layers, and how they interact.
2. Foreachofthethreephylaof photosynthetic bacteria, contrast how each fixes C and gains energy and reducing equivalents from light.
3. Forthetwothermophilicbacterialphyla, describe their adaptations to life at high
temperature. Explain how they are primitive and deeply-branching.
“Bioleaching" or "bio-oxidation" employs the use of naturally occurring bacteria, harmless to both humans and the environment, to extract of metals from their ores.
Conversion of insoluble metal sulfides into water-soluble metal sulfates.
It is mainly used to recover certain metals from sulfide ores. This is much cleaner than the traditional leaching.
Methanogenesis or biomethanation is the formation of methane by microbes known as methanogens. Organisms capable of producing methane have been identified only from the domain Archaea, a group phylogenetically distinct from both eukaryotes and bacteria, although many live in close association with anaerobic bacteria.
“Bioleaching" or "bio-oxidation" employs the use of naturally occurring bacteria, harmless to both humans and the environment, to extract of metals from their ores.
Conversion of insoluble metal sulfides into water-soluble metal sulfates.
It is mainly used to recover certain metals from sulfide ores. This is much cleaner than the traditional leaching.
Methanogenesis or biomethanation is the formation of methane by microbes known as methanogens. Organisms capable of producing methane have been identified only from the domain Archaea, a group phylogenetically distinct from both eukaryotes and bacteria, although many live in close association with anaerobic bacteria.
Presentation is about the "Origin of Life". Many theories being proposed to clearly explains how does Life actually came into existence on our planet Earth.
Origin of life-where did life come fromArosek Padhi
this chapter prompts you to wonder where did life as we know it came from. this is a presentation from Dr.Tithi Parija (asst professor) from KIIT school of biotechnology including different theories from different thinkers and scientists
Life, living matter are those that shows certain attributes that include responsiveness, growth, metabolism, energy transformation and reproduction.
In biology origin of life or abiogenesis is the natural process by which life has arisen from non-living matter, such as simple organic compounds.
It means the emergence of heritable and evolvable self-reproduction.
It is a complex subject and oftentimes controversial.
Several attempts have been made from time to time to explain the origin of life on earth.
There are several theories which offer their own explanation on the possible mechanism of origin of life.
Unit 3: Microbiology of Early Earth
LECTURE LEARNING GOALS
• Describe the early Earth environment, and prevailing theories for the origins of life.
• Describe the major events in the evolution of cellular life, and when they happened.
• Explain the lines of evidence that lead us to know when early life arose, and the scientific basis behind each line.
COMPLETE DETAILED DESCRIPTION ON EVOLUTION OF LIFE ON EARTH. MILLER UREY EXPERIMENT. SELF REPLICATING DNA. EARLY CELL LIKE STRUCTURE. PANSPERMIA . PHOTOSYNTHESIS. EMERGENCE OF HUMAN.
The full Crash Course Ecology Series- now in Note-Form! I've added my own little 'twists' on the notes, and have added some pictures to make studying easier.
Dr. Bruce Damer @ QAU Pakistan-The Origin of Life & Life in the UniverseBruce Damer
Dr. Bruce Damer presents a talk linking the new "Hot Spring Hypothesis" for the origin of life to the search for life in our Solar System and beyond on exoplanets. His host, the renowned physicist and activist Dr. Pervez Hoodbhoy, hosted this talk at the Physics department auditorium at Quaid-i-Azam University in Islamabad , Pakistan. Dr. Bruce “inflamed the minds” of Pakistani students and professors alike as he took them on a rapid romp through life’s possible origins on Earth to the search for evidence for life on Mars in 2020, icy Enceladus in the next decade and onward to the likelihood of life on exoplanets. Dr. Bruce Damer and Prof. Pervez Hoodbhoy (presenters), Elixir Technologies Pakistan (recording and support). [presented 17 November 2017]. Find a podcast with audio, video and additional information about this presentation at: http://www.levityzone.org/lz-episode-059-origins-science-comes-pakistan/
Similar to Microbes, Man and Environment (Microbial Evolution & Phylogeny ).pptx (20)
This pdf is about the Schizophrenia.
For more details visit on YouTube; @SELF-EXPLANATORY;
https://www.youtube.com/channel/UCAiarMZDNhe1A3Rnpr_WkzA/videos
Thanks...!
Professional air quality monitoring systems provide immediate, on-site data for analysis, compliance, and decision-making.
Monitor common gases, weather parameters, particulates.
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.Sérgio Sacani
The return of a sample of near-surface atmosphere from Mars would facilitate answers to several first-order science questions surrounding the formation and evolution of the planet. One of the important aspects of terrestrial planet formation in general is the role that primary atmospheres played in influencing the chemistry and structure of the planets and their antecedents. Studies of the martian atmosphere can be used to investigate the role of a primary atmosphere in its history. Atmosphere samples would also inform our understanding of the near-surface chemistry of the planet, and ultimately the prospects for life. High-precision isotopic analyses of constituent gases are needed to address these questions, requiring that the analyses are made on returned samples rather than in situ.
A brief information about the SCOP protein database used in bioinformatics.
The Structural Classification of Proteins (SCOP) database is a comprehensive and authoritative resource for the structural and evolutionary relationships of proteins. It provides a detailed and curated classification of protein structures, grouping them into families, superfamilies, and folds based on their structural and sequence similarities.
Nutraceutical market, scope and growth: Herbal drug technologyLokesh Patil
As consumer awareness of health and wellness rises, the nutraceutical market—which includes goods like functional meals, drinks, and dietary supplements that provide health advantages beyond basic nutrition—is growing significantly. As healthcare expenses rise, the population ages, and people want natural and preventative health solutions more and more, this industry is increasing quickly. Further driving market expansion are product formulation innovations and the use of cutting-edge technology for customized nutrition. With its worldwide reach, the nutraceutical industry is expected to keep growing and provide significant chances for research and investment in a number of categories, including vitamins, minerals, probiotics, and herbal supplements.
Multi-source connectivity as the driver of solar wind variability in the heli...Sérgio Sacani
The ambient solar wind that flls the heliosphere originates from multiple
sources in the solar corona and is highly structured. It is often described
as high-speed, relatively homogeneous, plasma streams from coronal
holes and slow-speed, highly variable, streams whose source regions are
under debate. A key goal of ESA/NASA’s Solar Orbiter mission is to identify
solar wind sources and understand what drives the complexity seen in the
heliosphere. By combining magnetic feld modelling and spectroscopic
techniques with high-resolution observations and measurements, we show
that the solar wind variability detected in situ by Solar Orbiter in March
2022 is driven by spatio-temporal changes in the magnetic connectivity to
multiple sources in the solar atmosphere. The magnetic feld footpoints
connected to the spacecraft moved from the boundaries of a coronal hole
to one active region (12961) and then across to another region (12957). This
is refected in the in situ measurements, which show the transition from fast
to highly Alfvénic then to slow solar wind that is disrupted by the arrival of
a coronal mass ejection. Our results describe solar wind variability at 0.5 au
but are applicable to near-Earth observatories.
Seminar of U.V. Spectroscopy by SAMIR PANDASAMIR PANDA
Spectroscopy is a branch of science dealing the study of interaction of electromagnetic radiation with matter.
Ultraviolet-visible spectroscopy refers to absorption spectroscopy or reflect spectroscopy in the UV-VIS spectral region.
Ultraviolet-visible spectroscopy is an analytical method that can measure the amount of light received by the analyte.
Introduction:
RNA interference (RNAi) or Post-Transcriptional Gene Silencing (PTGS) is an important biological process for modulating eukaryotic gene expression.
It is highly conserved process of posttranscriptional gene silencing by which double stranded RNA (dsRNA) causes sequence-specific degradation of mRNA sequences.
dsRNA-induced gene silencing (RNAi) is reported in a wide range of eukaryotes ranging from worms, insects, mammals and plants.
This process mediates resistance to both endogenous parasitic and exogenous pathogenic nucleic acids, and regulates the expression of protein-coding genes.
What are small ncRNAs?
micro RNA (miRNA)
short interfering RNA (siRNA)
Properties of small non-coding RNA:
Involved in silencing mRNA transcripts.
Called “small” because they are usually only about 21-24 nucleotides long.
Synthesized by first cutting up longer precursor sequences (like the 61nt one that Lee discovered).
Silence an mRNA by base pairing with some sequence on the mRNA.
Discovery of siRNA?
The first small RNA:
In 1993 Rosalind Lee (Victor Ambros lab) was studying a non- coding gene in C. elegans, lin-4, that was involved in silencing of another gene, lin-14, at the appropriate time in the
development of the worm C. elegans.
Two small transcripts of lin-4 (22nt and 61nt) were found to be complementary to a sequence in the 3' UTR of lin-14.
Because lin-4 encoded no protein, she deduced that it must be these transcripts that are causing the silencing by RNA-RNA interactions.
Types of RNAi ( non coding RNA)
MiRNA
Length (23-25 nt)
Trans acting
Binds with target MRNA in mismatch
Translation inhibition
Si RNA
Length 21 nt.
Cis acting
Bind with target Mrna in perfect complementary sequence
Piwi-RNA
Length ; 25 to 36 nt.
Expressed in Germ Cells
Regulates trnasposomes activity
MECHANISM OF RNAI:
First the double-stranded RNA teams up with a protein complex named Dicer, which cuts the long RNA into short pieces.
Then another protein complex called RISC (RNA-induced silencing complex) discards one of the two RNA strands.
The RISC-docked, single-stranded RNA then pairs with the homologous mRNA and destroys it.
THE RISC COMPLEX:
RISC is large(>500kD) RNA multi- protein Binding complex which triggers MRNA degradation in response to MRNA
Unwinding of double stranded Si RNA by ATP independent Helicase
Active component of RISC is Ago proteins( ENDONUCLEASE) which cleave target MRNA.
DICER: endonuclease (RNase Family III)
Argonaute: Central Component of the RNA-Induced Silencing Complex (RISC)
One strand of the dsRNA produced by Dicer is retained in the RISC complex in association with Argonaute
ARGONAUTE PROTEIN :
1.PAZ(PIWI/Argonaute/ Zwille)- Recognition of target MRNA
2.PIWI (p-element induced wimpy Testis)- breaks Phosphodiester bond of mRNA.)RNAse H activity.
MiRNA:
The Double-stranded RNAs are naturally produced in eukaryotic cells during development, and they have a key role in regulating gene expression .
Observation of Io’s Resurfacing via Plume Deposition Using Ground-based Adapt...Sérgio Sacani
Since volcanic activity was first discovered on Io from Voyager images in 1979, changes
on Io’s surface have been monitored from both spacecraft and ground-based telescopes.
Here, we present the highest spatial resolution images of Io ever obtained from a groundbased telescope. These images, acquired by the SHARK-VIS instrument on the Large
Binocular Telescope, show evidence of a major resurfacing event on Io’s trailing hemisphere. When compared to the most recent spacecraft images, the SHARK-VIS images
show that a plume deposit from a powerful eruption at Pillan Patera has covered part
of the long-lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth-based telescopes. The SHARK-VIS instrument ushers in a new era of high resolution imaging of Io’s surface using adaptive
optics at visible wavelengths.
The increased availability of biomedical data, particularly in the public domain, offers the opportunity to better understand human health and to develop effective therapeutics for a wide range of unmet medical needs. However, data scientists remain stymied by the fact that data remain hard to find and to productively reuse because data and their metadata i) are wholly inaccessible, ii) are in non-standard or incompatible representations, iii) do not conform to community standards, and iv) have unclear or highly restricted terms and conditions that preclude legitimate reuse. These limitations require a rethink on data can be made machine and AI-ready - the key motivation behind the FAIR Guiding Principles. Concurrently, while recent efforts have explored the use of deep learning to fuse disparate data into predictive models for a wide range of biomedical applications, these models often fail even when the correct answer is already known, and fail to explain individual predictions in terms that data scientists can appreciate. These limitations suggest that new methods to produce practical artificial intelligence are still needed.
In this talk, I will discuss our work in (1) building an integrative knowledge infrastructure to prepare FAIR and "AI-ready" data and services along with (2) neurosymbolic AI methods to improve the quality of predictions and to generate plausible explanations. Attention is given to standards, platforms, and methods to wrangle knowledge into simple, but effective semantic and latent representations, and to make these available into standards-compliant and discoverable interfaces that can be used in model building, validation, and explanation. Our work, and those of others in the field, creates a baseline for building trustworthy and easy to deploy AI models in biomedicine.
Bio
Dr. Michel Dumontier is the Distinguished Professor of Data Science at Maastricht University, founder and executive director of the Institute of Data Science, and co-founder of the FAIR (Findable, Accessible, Interoperable and Reusable) data principles. His research explores socio-technological approaches for responsible discovery science, which includes collaborative multi-modal knowledge graphs, privacy-preserving distributed data mining, and AI methods for drug discovery and personalized medicine. His work is supported through the Dutch National Research Agenda, the Netherlands Organisation for Scientific Research, Horizon Europe, the European Open Science Cloud, the US National Institutes of Health, and a Marie-Curie Innovative Training Network. He is the editor-in-chief for the journal Data Science and is internationally recognized for his contributions in bioinformatics, biomedical informatics, and semantic technologies including ontologies and linked data.
3. Microbial Evolution
Early Earth and the Origin and Diversification of
Life
● The processes that might have given rise to the first
cellular life, its divergence into two evolutionary
lineages, Bacteria and Archaea, and the later
formation, through endosymbiosis, of a third lineage,
the Eukarya.
● Although much about these events and processes
remains speculative, geological and molecular
evidence has combined to build a plausible scenario
for how life might have arisen and diversified.
4. Formation and Early History of Earth
● Before considering how life arose, we need to go back even farther,
and ask how Earth itself formed.
Origin of Earth
● Earth is thought to have formed about 4.5 billion years ago, based
on analyses of slowly decaying radioactive isotopes.
● Our planet and the other planets of our solar system arose from
materials making up a disc-shaped nebular cloud of dust and gases
released by the supernova of a massive old star.
● As a new star—our sun—formed within this cloud, it began to
compact, undergo nuclear fusion, and release large amounts of
energy in the form of heat and light.
● Materials left in the nebular cloud began to clump and fuse due to
collisions and gravitational attractions, forming tiny accretions that
gradually grew larger to form clumps that eventually coalesced into
planets.
● Energy released in this process heated the emerging Earth as it
formed, as did energy released by radioactive decay within the
condensing materials, forming a planet Earth of fiery hot magma.
5. ● As Earth cooled over time, a metallic core, rocky mantle, and a
thin lower-density surface crust formed.
● The inhospitable conditions of early Earth, characterized by
abmolten surface under intense bombardment from space by
asteroids and other objects, are thought to have persisted for over
500 million years.
● Water on Earth originated from innumerable collisions with icy
comets and asteroids and from volcanic outgassing of the planet’s
interior.
● At this time, due to the heat, water would have been present only
as water vapor.
● The sedimentary composition of these rocks indicates by that time
Earth had at least cooled sufficiently (<100°C) for the water vapor
to have condensed and formed the early oceans.
● Even more ancient materials, crystals of the mineral zircon
(ZrSiO4), however, have been discovered, and these materials
give us a glimpse of even earlier conditions on Earth.
6. Evidence for Microbial Life on Early Earth
● The fossilized remains of cells and the isotopically “light” carbon
abundant in these rocks provide evidence for early microbial life
● Some ancient rocks contain what appear to be bacteria-like
microfossils, typically simple rods or cocci.
● In rocks 3.5 billion years old or younger, microbial formations called
stromatolites are common. Stromatolites are microbial mats
consisting of layers of filamentous prokaryotes and trapped mineral
materials; they may become fossilized.
What kind of organisms were these ancient stromatolitic bacteria?
● By comparing ancient stromatolites with modern
stromatolites growing in shallow marine basins or in hot
springs we can see it is likely that ancient stromatolites
formed from filamentous phototrophic bacteria, such as
ancestors of the green nonsulfur bacterium Chloroflex
7. ● The age of these microfossils, about 1 billion years, is well within
the time frame that such organisms were thought to be present
on Earth.
● In summary, microfossil evidence strongly suggests that
microbial life was present within at least 1 billion years of the
formation of Earth and probably somewhat earlier, and that by
that time, microorganisms had already attained an impressive
diversity of morphological forms.
9. Origin of Cellular Life
● Here we consider the issue of how living organisms
might have originated, focusing on two questions:
■ How might the first cells have arisen?
■ What might those early cells have been like?
● But along the way, we will consider the likely
possibility that self replicating RNAs preceded cellular
life and how these molecules may have paved the
way for cellular life.
10. Surface Origin Hypothesis
● One hypothesis for the origin of life holds that the first membrane-
enclosed, self-replicating cells arose out of a primordial soup rich in
organic and inorganic compounds in a “warm little pond,” as Charles
Darwin suggested in On the Origin of Species—in other words, life
arose on Earth’s surface.
● Although there is experimental evidence that organic precursors to
living cells can form spontaneously under certain conditions, surface
conditions on early Earth are thought to have been hostile to both
life and its inorganic and organic precursors. The dramatic
temperature fluctuations and mixing resulting from meteor impacts,
dust clouds, and storms, along with intense ultraviolet radiation,
make a surface origin for life unlikely
11. Subsurface Origin Hypothesis
● A more likely hypothesis is that life originated at hydrothermal
springs on the ocean floor, well below Earth’s surface, where
conditions would have been much less hostile and much more
stable.
● A steady and abundant supply of energy in the form of reduced
inorganic compounds, for example, hydrogen (H2) and hydrogen
sulfide (H2S), would have been available at these spring sites.
● When the very warm (90–100°C) hydrothermal water flowed up
through the crust and mixed with cooler, iron-containing and more
oxidized oceanic waters, precipitates of colloidal pyrite (FeS),
silicates, carbonates, and magnesium containing montmorillonite
clays formed.
● These precipitates built up into structured mounds with gel-like
adsorptive surfaces, semipermeable enclosures, and pores.
● Serpentinization, the abiotic process by which Fe/Mg silicates
(serpentines) react with other minerals and H2, was a likely source
of the first organic compounds, such as hydrocarbons and fatty
acids.
12. ● These could then have reacted with iron and nickel sulfide
minerals to eventually form amino acids, simple peptides,
sugars, and nitrogenous bases.
● With phosphate from seawater, nucleotides such as AMP and
ATP could have been formed and polymerized into RNA by
montmorillonite clay, a material known to catalyze such
reactions.
● An important point to keep in mind here is that before life
appeared on Earth, organic precursors of life would not have
been consumed by organisms, as they would be today.
● So the possibility that millions of years ago organic matter
accumulated to levels where self-replicating entities emerged, is
not an unreasonable hypothesis.
13.
14. An RNA World and Protein Synthesis
● The synthesis and concentration of organic compounds by prebiotic
chemistry set the stage for self-replicating systems, the precursors to
cellular life. How might self-replicating systems have arisen?
● One possibility is that there was an early RNA world, in which the first
self replicating systems were molecules of RNA.
● Because RNA can bind small molecules, such as ATP and other
nucleotides, and has catalytic activity, RNA might have catalyzed its
own synthesis from the available sugars, bases, and phosphate
● RNA also can bind other molecules, such as amino acids, catalyzing the
synthesis of primitive proteins.
● Later, as different types of proteins emerged, some with catalytic
abilities, proteins began to take over the catalytic role of RNAs.
● Eventually, DNA, a molecule more stable than RNA and therefore a
better repository of genetic (coding) information, arose and assumed
the template role for RNA synthesis. This three-part system—DNA,
RNA, and protein—became fixed early on as the fittest solution to
biological information processing.
15. Lipid Membranes and Cellular Life
● Anther important step in the emergence of cellular life was the
synthesis of phospholipid membrane vesicles that could enclose
the evolving biochemical and replication machinery.
● Proteins embedded in the lipids would have made the vesicles
semipermeable and thus able to shuttle nutrients and wastes
across the membrane, setting the stage for the evolution of
energy-conserving processes and ATP synthesis. By entrapping
RNA and DNA, these lipoprotein vesicles, may have enclosed the
first self-replicating entities, partitioning the biochemical machinery
in a unit not unlike the cells we know today.
● From this population of structurally very simple early cells, referred
to as the last universal common ancestor (LUCA), cellular life
began to evolve in two distinct directions, possibly in response to
physiochemical differences in their most successful niches.
● As natural selection continued, these two prokaryotic lineages, the
Bacteria and the Archaea, became ever more distinct, displaying
the characteristic properties we associate with each lineage today.
16. Early Metabolism
● From the time of formation, the early ocean and all of Earth was
anoxic.Molecular oxygen (O2) did not appear in any significant quantities
until oxygenic photosynthesis by cyanobacteria evolved.
● Thus, the energy generating metabolism of primitive cells would have been
exclusively anaerobic and would likely have had to be heat-stable because
of the temperature of early Earth. It is widely thought that H2 was a major
fuel for energy metabolism of early cells. This hypothesis is also supported
by the tree of life, in that virtually all of the earliest branching organisms in
the Bacteria and Archaea lineages use H2 as an electron donor in energy
metabolism
● Moreover, because of the abundance of H2 and sulfur compounds on Early,
this scheme would have provided cells with a nearly limitless supply of
energy.
● These early forms of chemolithotrophic metabolism driven by H2 would
likely have supported the production of large amounts of organic
compounds from autotrophic CO2 fixation. Over time, these organic
materials would have accumulated and could have provided the
environment needed for the appearance of new chemoorganotrophic
bacteria with diverse metabolic strategies to conserve energy from organic
compounds; metabolic diversity would have been off and running.
17.
18. Microbial Diversification:
Consequences for Earth’s Biosphere
● Following the origin of cells and the development of early forms of
energy and carbon metabolism, microbial life underwent a long
process of metabolic diversification, taking advantage of the
various and abundant resources available on Earth. As particular
resources were consumed and became limiting, evolution
selected for more efficient and novel metabolisms.
● Also, microbial life, through its metabolic activity, altered the
biosphere, depleting some resources and creating others through
the production of waste products and cellular material.
● Here we examine the scope of metabolic diversification and focus
on one key metabolic waste product in particular, molecular
oxygen (O2), a molecule that had a profound impact on the
further evolution of life on Earth.
19. Metabolic Diversification
● LUCA, the last universal common ancestor, may have existed as
early as 4.3 billion years ago. Molecular evidence suggests that
ancestors of modern-day Bacteria and Archaea had already
diverged by 3.8–3.7 billion years ago. As these lineages diverged,
they developed distinct metabolisms.
● Early Bacteria may have used H2 and CO2 to produce acetate, or
ferrous iron (Fe2+) compounds, for energy generation.
● At the same time, early Archaea developed the ability to use H2 and
CO2, or possibly acetate as it accumulated, as substrates for
methanogenesis (the production of methane, CH4), according to the
following formulas:
20. ● Phototrophy arose somewhat later, about 3.3 billion years
ago, and apparently only in Bacteria. The ability to use solar
radiation as an energy source allowed phototrophs to diversify
extensively. With the exception of the early-branching
hyperthermophilic Bacteria (genera such as Aquifex and
Thermotoga), the common ancestor of all other Bacteria
appears to be an anaerobic phototroph, possibly similar to
Chloroflexus.
● About 2.7–3 billion years ago, the cyanobacteria lineage
developed a photosystem that could use H2O in place of H2S
for photosynthetic reduction of CO2, releasing O2 instead of
elemental sulfur (S0) as a waste product; the evolution of this
process opened up many new metabolic possibilities, in
particular aerobic respiration.
21. The Rise of Oxygen: Banded Iron Formations
● Molecular and chemical evidence indicates that oxygenic
photosynthesis first appeared on Earth about 300 million years before
significant levels of O2 appeared in the atmosphere.
● By 2.5 billion years ago, O2 levels had risen to one part per million, a
tiny amount by present-day standards, but enough to initiate what has
come to be called the Great Oxidation Event.
What delayed the buildup of O2 for so long?
● The O2 that cyanobacteria produced did not begin to accumulate in the
atmosphere until it first reacted and consumed the bulk of reduced
materials, especially reduced iron minerals such as FeS and FeS2, in
the oceans; these materials oxidize slowly but spontaneously with O2.
● The Fe3+ produced from the oxidation of these minerals became a
prominent marker in the geological record. Much of the iron in rocks of
Precambrian origin (0.5 billion years ago) exists in banded Iron
formations, laminated sedimentary rocks formed in deposits of iron and
silica-rich materials.
● Once the abundant Fe2+ on Earth was consumed, the stage was set for
O2 to accumulate in the atmosphere, but not until 800–900 million years
ago did atmospheric O2 accumulate to present-day levels (+21%)
22. New Metabolisms and the Ozone Shield
● As O2 accumulated on Earth, the atmosphere gradually changed
from anoxic to oxic. Species of Bacteria and Archaea unable to
adapt to this change were increasingly restricted to anoxic habitats
because of the toxicity of O2 and because it oxidized the reduced
substances upon which their metabolisms were dependent.
● However, the oxic atmosphere also created conditions for the
evolution of various new metabolic pathways, such as sulfate
reduction, nitrification, and the various other chemolithotrophic
processes.
● Prokaryotes that evolved the ability to respire O2 gained a
tremendous energetic advantage because of the high reduction
potential of the O2/H2O couple and so are capable of producing
larger cell populations from a given amount of resources than were
anaerobic organisms.
23. ● As Earth became more oxic, organelle-containing eukaryotic
microorganisms arose, and the rise in O2 spurred their rapid
evolution. The oldest microfossils known to be eukaryotic because
they have recognizable nuclei are about 2 billion years old.
Multicellular and increasingly complex microfossils of algae are
evident from 1.9 to 1.4 billion years ago.
● By 0.6 billion years ago, with O2 near present-day levels, large
multicellular organisms, the Ediacaran fauna, were present in the
sea.
● In a relatively short time, multicellular eukaryotes diversified into the
ancestors of modern-day algae, plants, fungi, and animals.
● An important consequence of O2 for the evolution of life was the
formation of ozone (O3), a gas that provides a barrier preventing
much of the intense ultraviolet (UV) radiation of the sun from
reaching the Earth.
● Until an ozone shield developed in Earth’s upper atmosphere,
evolution could have continued only beneath the ocean surface and
in protected terrestrial environments where organisms were not
exposed to the lethal DNA damage from the sun’s intense UV
radiations.
25. Endosymbiotic Origin of Eukaryotes
● Up to about 2 billion years ago, all cells apparently lacked a
membrane-enclosed nucleus and organelles, the key
characteristics of eukaryotic cells (domain Eukarya). Here we
consider the origin of the Eukarya and show how eukaryotes are
genetic chimerascontaining genes from at least two different
phylogenetic domains.
Endosymbiosis
● The origin of eukaryotes came after the rise in atmospheric O2,
the development of respiratory metabolism and photosynthesis in
Bacteria, and the evolution of enzymes such as superoxide
dismutase that could detoxify the oxygen radicals generated as a
by-product of aerobic respiration.How might Eukarya have
arisen and in what ways did the availability of oxygen
influence evolution?
● A well-supported explanation for the origin of the eukaryotic cell is
the endosymbiotic hypothesis
26. Endosymbiotic Hypothesis
● The hypothesis posits that the mitochondria of modern-day
eukaryotes arose from the stable incorporation of a respiring
bacterium into other cells, and that chloroplasts similarly arose
from the incorporation of a cyanobacterium-like organism that
carried out oxygenic photosynthesis.
● Oxygen was almost certainly a driving force in endosymbiosis
through its consumption in energy metabolism by the ancestor of the
mitochondrion and its production in photosynthesis by the ancestor
of the chloroplast.
● The overall physiology and metabolism of mitochondria and
chloroplasts and the sequence and structures of their genomes
support the endosymbiosis hypothesis. For example, both
mitochondria and chloroplasts contain ribosomes of prokaryotic size
(70S) and have 16S ribosomal RNA gene sequences characteristic
of certain Bacteria.
27. Formation of the Eukaryotic Cell
● Two hypotheses have been put forward to explain the
formation of the eukaryotic cell.
■ In one, eukaryotes began as a nucleus-bearing cell
that later acquired mitochondria and chloroplasts by
endosymbiosis. In this hypothesis, the nucleus-bearing
cell line arose in a lineage of cells that split from the
Archaea; the nucleus is thought to have arisen in this cell
line during evolutionary experimentation with increasing
cell and genome size, probably in response to oxic
events that were transforming the geochemistry of Earth.
However, a major problem with this hypothesis is that it
does not easily account for the fact that Bacteria and
Eukarya have similar membrane lipids, in contrast to
those of Archaea.
28.
29. ● The second hypothesis, called the hydrogen hypothesis,
proposes that the eukaryotic cell arose from an association
between a H2-producing species of Bacteria, the
symbiont, which eventually gave rise to the
mitochondrion, and a species of H2-consuming
Archaea, the host. In this hypothesis, the nucleus arose
after genes for lipid synthesis were transferred from the
symbiont to the host. This led to the synthesis of lipids
containing fatty acids by the host, lipids that may have been
more conducive to the formation of internal membranes,
such as the nuclear membrane system. The simultaneous
increase in size of the host genome led tosequestering DNA
within a membrane, which organized it and made replication
and gene expression more efficient. Later, this
mitochondrion-containing, nucleated cell line acquired
chloroplasts by endosymbiosis, leading to the first
phototrophic eukaryotes.
32. Microbial Phylogeny
● Biologists previously grouped living organisms into five
kingdoms:
plants, animals, fungi, protists, and bacteria.
● DNA sequence-based phylogenetic analysis, on the other
hand, has revealed that the five kingdoms do not
represent five primary evolutionary lines. Instead cellular
life on Earth has evolved along three primary lineages, called
domains.
■ Two of these domains, the Bacteria and the
Archaea, are exclusively composed of prokaryotic
cells.
■ The Eukarya contains the eukaryotes including the
plants, animals, fungi, and protists.
33.
34. Bacteria
Among Bacteria, at least 80 lineages (called phyla, singular
phylum, or divisions) have been discovered thus far; only some
key ones are shown in the universal tree. Many lineages of
Bacteria are known only from environmental sequences
(phylotypes). Although some lineages are characterized by
unique phenotypic traits, such as the morphology of the
spirochetes or the physiology of the cyanobacteria,
Most major groups of Bacteria consist of species that,
although specifically related from a phylogenetic standpoint, lack
strong phenotypic cohesiveness. The largest group, the
Proteobacteria, is a good example of this, as collectively this
group shows all known forms
of microbial physiology. The major eukaryotic organelles
clearly originated from within the domain Bacteria, the
mitochondrion from within the Proteobacteria and the
chloroplast from within the cyanobacteria.
35. Archaea
The domain Archaea consists of two major phyla,
● Crenarchaeota and
● Euryarchaeota.
Branching close to the root of the universal tree are hyperthermophilic
species of Crenarchaeota, such as Pyrolobus. These are followed by
the phylum Euryarchaeota, which includes the methane-producing
(methanogenic).
Archaea and the extreme halophiles and extreme acidophiles, such as
Thermoplasma.There are some lineages of Archaea known only from
the sampling of rRNA genes from the environment. This list keeps
expanding as more habitats are specifically sampled for Archaea
diversity. It has become clear that cultured species of Archaea, primarily
obtained from extreme environments such as hot springs, saline lakes,
acidic soils, and the like, have many relatives in more moderate habitats
such as freshwater lakes, streams, agricultural soils, and the oceans; at
this point we have only limited knowledge of the activities and metabolic
strategies of the Archaea that inhabit nonextreme environments.
36. Eukarya
Phylogenetic trees of species in the domain Eukarya have been constructed
from comparative sequence analysis of the 18S rRNA gene, the functional
equivalent of the 16S rRNA gene. The eukaryotic evolution was triggered by
the onset of oxic conditions on Earth and subsequent development of the
ozone shield. The latter would have greatly expanded the number of
surface habitats available for colonization. Nevertheless, although 18S
rRNA sequencing appears to give a skewed view of eukaryotic microbial
evolution, it still clearly sorts the eukaryotes out as a distinct domain of life
with evolutionary roots more closely tied to the Archaea than to the Bacteria