COMPLETE DETAILED DESCRIPTION ON EVOLUTION OF LIFE ON EARTH. MILLER UREY EXPERIMENT. SELF REPLICATING DNA. EARLY CELL LIKE STRUCTURE. PANSPERMIA . PHOTOSYNTHESIS. EMERGENCE OF HUMAN.
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.
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/
Dr. Bruce Damer: Hot Spring Hypothesis of the Origin of Life & Future of Life...Bruce Damer
Dr. Bruce Damer covers the new science of the origin of life (the Hot Spring Hypothesis) and its relationship to our future in space (the expansion of the biosphere into the Solar System). The was presented at the 2018 Bay Area Society for Information Display at the Stanford Golf Course/Club on September 8, 2018.
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.
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/
Dr. Bruce Damer: Hot Spring Hypothesis of the Origin of Life & Future of Life...Bruce Damer
Dr. Bruce Damer covers the new science of the origin of life (the Hot Spring Hypothesis) and its relationship to our future in space (the expansion of the biosphere into the Solar System). The was presented at the 2018 Bay Area Society for Information Display at the Stanford Golf Course/Club on September 8, 2018.
New articles were published at the end of the 2017 about "chicken-the-egg" question: which organic molecules were the first: nucleotides or amino acids. RNA world is still the predominant theory, but new studies on proteins could change that.
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
IB Biology markscheme, past exam papers, notes and 2012 IB Biology syllabus. IB Biology option D evolution markscheme. IB Biology option D evolution notes, IB Biology option D Evolution exam papers, IB Biology option E markscheme, IB Biology option E notes, IB Biology option E Neurobiology papers, IB Biology Option A Human Nutrition and Health syllabus 2012, Stimulus and response, Homologous structures, Pavlov experiments.
An Origin of Life in Salt Water or Fresh Water?Bruce Damer
Returning to Darwin's "Warm Little Pond" with the Terrestrial Origin of Life Hypothesis. Presented at the Australasian Astrobiology Meeting, Perth, July 2016. Presented by Dr. Bruce Damer, U.C. Santa Cruz.
New articles were published at the end of the 2017 about "chicken-the-egg" question: which organic molecules were the first: nucleotides or amino acids. RNA world is still the predominant theory, but new studies on proteins could change that.
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
IB Biology markscheme, past exam papers, notes and 2012 IB Biology syllabus. IB Biology option D evolution markscheme. IB Biology option D evolution notes, IB Biology option D Evolution exam papers, IB Biology option E markscheme, IB Biology option E notes, IB Biology option E Neurobiology papers, IB Biology Option A Human Nutrition and Health syllabus 2012, Stimulus and response, Homologous structures, Pavlov experiments.
An Origin of Life in Salt Water or Fresh Water?Bruce Damer
Returning to Darwin's "Warm Little Pond" with the Terrestrial Origin of Life Hypothesis. Presented at the Australasian Astrobiology Meeting, Perth, July 2016. Presented by Dr. Bruce Damer, U.C. Santa Cruz.
Earth and Life Sciences for Senior High School by Duyanen and Andaya pages 176-179
My fun and colorful grade 11 report on Life Sciences 2nd semester of A.Y. 2016-2017 under Ms. Lagmay
Biodiversity, Microbial Biodiversity, Bacterial Biodiveristy, Archae Biodiversity, Protozoa Biodiversity, Fungal Biodiversity, Origin of Life, Origin of Life on Earth, Chemical Evolution, Physical Evolution, Biological Evolution
EMERGENCE OF THE FIRST LIVING CELL [Autosaved].pptxRASHMI M G
The origin of life on Earth is a mystery of science, with no widely accepted theory but many hypotheses supported by evidence. The earliest known fossils are 3.5 billion years old, but there is evidence that bacteria-like organisms lived on Earth 3.5 billion years ago, and may have existed even earlier, when the first solid crust formed, almost 4 billion years ago. Scientists think that early life may have formed from lighting strikes or arisen in deep sea vents.
A PowerPoint Presentation about the introduction to Life Science as part of the 2nd quarter curriculum of Earth and Life Science subject in Senior High School.
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.
Comparing Evolved Extractive Text Summary Scores of Bidirectional Encoder Rep...University of Maribor
Slides from:
11th International Conference on Electrical, Electronics and Computer Engineering (IcETRAN), Niš, 3-6 June 2024
Track: Artificial Intelligence
https://www.etran.rs/2024/en/home-english/
Toxic effects of heavy metals : Lead and Arsenicsanjana502982
Heavy metals are naturally occuring metallic chemical elements that have relatively high density, and are toxic at even low concentrations. All toxic metals are termed as heavy metals irrespective of their atomic mass and density, eg. arsenic, lead, mercury, cadmium, thallium, chromium, etc.
ISI 2024: Application Form (Extended), Exam Date (Out), EligibilitySciAstra
The Indian Statistical Institute (ISI) has extended its application deadline for 2024 admissions to April 2. Known for its excellence in statistics and related fields, ISI offers a range of programs from Bachelor's to Junior Research Fellowships. The admission test is scheduled for May 12, 2024. Eligibility varies by program, generally requiring a background in Mathematics and English for undergraduate courses and specific degrees for postgraduate and research positions. Application fees are ₹1500 for male general category applicants and ₹1000 for females. Applications are open to Indian and OCI candidates.
Salas, V. (2024) "John of St. Thomas (Poinsot) on the Science of Sacred Theol...Studia Poinsotiana
I Introduction
II Subalternation and Theology
III Theology and Dogmatic Declarations
IV The Mixed Principles of Theology
V Virtual Revelation: The Unity of Theology
VI Theology as a Natural Science
VII Theology’s Certitude
VIII Conclusion
Notes
Bibliography
All the contents are fully attributable to the author, Doctor Victor Salas. Should you wish to get this text republished, get in touch with the author or the editorial committee of the Studia Poinsotiana. Insofar as possible, we will be happy to broker your contact.
hematic appreciation test is a psychological assessment tool used to measure an individual's appreciation and understanding of specific themes or topics. This test helps to evaluate an individual's ability to connect different ideas and concepts within a given theme, as well as their overall comprehension and interpretation skills. The results of the test can provide valuable insights into an individual's cognitive abilities, creativity, and critical thinking skills
Deep Behavioral Phenotyping in Systems Neuroscience for Functional Atlasing a...Ana Luísa Pinho
Functional Magnetic Resonance Imaging (fMRI) provides means to characterize brain activations in response to behavior. However, cognitive neuroscience has been limited to group-level effects referring to the performance of specific tasks. To obtain the functional profile of elementary cognitive mechanisms, the combination of brain responses to many tasks is required. Yet, to date, both structural atlases and parcellation-based activations do not fully account for cognitive function and still present several limitations. Further, they do not adapt overall to individual characteristics. In this talk, I will give an account of deep-behavioral phenotyping strategies, namely data-driven methods in large task-fMRI datasets, to optimize functional brain-data collection and improve inference of effects-of-interest related to mental processes. Key to this approach is the employment of fast multi-functional paradigms rich on features that can be well parametrized and, consequently, facilitate the creation of psycho-physiological constructs to be modelled with imaging data. Particular emphasis will be given to music stimuli when studying high-order cognitive mechanisms, due to their ecological nature and quality to enable complex behavior compounded by discrete entities. I will also discuss how deep-behavioral phenotyping and individualized models applied to neuroimaging data can better account for the subject-specific organization of domain-general cognitive systems in the human brain. Finally, the accumulation of functional brain signatures brings the possibility to clarify relationships among tasks and create a univocal link between brain systems and mental functions through: (1) the development of ontologies proposing an organization of cognitive processes; and (2) brain-network taxonomies describing functional specialization. To this end, tools to improve commensurability in cognitive science are necessary, such as public repositories, ontology-based platforms and automated meta-analysis tools. I will thus discuss some brain-atlasing resources currently under development, and their applicability in cognitive as well as clinical neuroscience.
Professional air quality monitoring systems provide immediate, on-site data for analysis, compliance, and decision-making.
Monitor common gases, weather parameters, particulates.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
This presentation explores a brief idea about the structural and functional attributes of nucleotides, the structure and function of genetic materials along with the impact of UV rays and pH upon them.
The use of Nauplii and metanauplii artemia in aquaculture (brine shrimp).pptxMAGOTI ERNEST
Although Artemia has been known to man for centuries, its use as a food for the culture of larval organisms apparently began only in the 1930s, when several investigators found that it made an excellent food for newly hatched fish larvae (Litvinenko et al., 2023). As aquaculture developed in the 1960s and ‘70s, the use of Artemia also became more widespread, due both to its convenience and to its nutritional value for larval organisms (Arenas-Pardo et al., 2024). The fact that Artemia dormant cysts can be stored for long periods in cans, and then used as an off-the-shelf food requiring only 24 h of incubation makes them the most convenient, least labor-intensive, live food available for aquaculture (Sorgeloos & Roubach, 2021). The nutritional value of Artemia, especially for marine organisms, is not constant, but varies both geographically and temporally. During the last decade, however, both the causes of Artemia nutritional variability and methods to improve poorquality Artemia have been identified (Loufi et al., 2024).
Brine shrimp (Artemia spp.) are used in marine aquaculture worldwide. Annually, more than 2,000 metric tons of dry cysts are used for cultivation of fish, crustacean, and shellfish larva. Brine shrimp are important to aquaculture because newly hatched brine shrimp nauplii (larvae) provide a food source for many fish fry (Mozanzadeh et al., 2021). Culture and harvesting of brine shrimp eggs represents another aspect of the aquaculture industry. Nauplii and metanauplii of Artemia, commonly known as brine shrimp, play a crucial role in aquaculture due to their nutritional value and suitability as live feed for many aquatic species, particularly in larval stages (Sorgeloos & Roubach, 2021).
1. THE ORIGIN AND EVOLUTION
OF LIFE ON EARTH
PRESENTED BY: -
M P SANDHYA
2. WHEN DID LIFE BEGIN?
Quite early in Earth’s history
Cannot pinpoint time, but can narrow down a time
period with 3 lines of evidence
3. WHEN DID LIFE BEGIN?
Stromatolites (3.5 bill. Yr)
Rocks with distinctive layer
structure
Look identical to living
mats of microbes
Layers of microbes and
sediment
Top layer uses
photosynthesis
Lower layers use top layer’s
byproducts
4. WHEN DID LIFE BEGIN?
Microfossils dating to
3.5 billion years ago
Difficult to distinguish
from mineral
structures
Analysis shows that
some structures
contain organic
carbon
-found in at least 3 sites
5. WHEN DID LIFE BEGIN?
Evidence in metamorphic
rocks that life existed 3.85
billions years ago
Low C12/C13 fraction in rock
layers suggests life
Biological processes prefer
C12 to C13
Find lower fraction of C13
Non-biological processes
have no preference, so find
equal amounts
6. WHEN DID LIFE BEGIN?
Rocks before ~4 billion years old are rare and
hard to find
Time of heavy bombardment ended about 3.8-
4.0 billion years ago
Last devastating impact between 4.2-3.9 bill. Yr ago
Evidence suggests life as long as 3.85 billion
years ago and definitely at 3.5 billion years ago
Life rose and dominated the planet between 100-
500 million years
7. LIVING FOSSILS
DNA used as living fossil
The more alike the DNA sequence between species, the more recent
their divergence and extinction of their common ancestor
8. LIVING FOSSILS
Bacteria and Archaea: genetic material NOT separated
from rest of cell
Eukarya: DNA separated from rest of cell by membrane
Extremophiles (live near deep-sea vents or in hot springs)
closest to root of tree of life
9.
10. WHERE DID LIFE BEGIN?
Land is unlikely
No O2, no ozone: UV destroys molecular bonds
Shallow ponds
Once favored, full of organic material
When evaporated, organic chemical concentration
increases making it easier to combine complex molecules
leading to life
Current experiments indicate lack of chemical energy
sufficient to support life
Deep-sea vents/hot springs
DNA evidence suggests that early organisms survived in
conditions similar to deep-sea vents
Plenty of chemical energy available
11. HOW DID LIFE BEGIN?
Simplest organisms today and those dated 3.5 billion years ago are
remarkable advanced
What are the natural chemical processes that could have led to life?
Assumptions
Life began under chemical conditions of early Earth
Life did not migrate to Earth
12. ORGANIC CHEMISTRY ON EARLY
EARTH
In 1920’s, scientists hypothesized that the chemicals in the early
atmosphere, fueled by sunlight, would spontaneously create organic
molecules
Tested by Miller-Urey experiment 1950’s
13. MILLER-UREY EXPERIMENT
First flask partially filled with water and heated to
produce water vapor (sea)
Water vapor was moved to a second flask where
methane and ammonia vapor was added
(atmosphere)
Electric sparks (lightening) in second flask was
energy source for chemical reactions
Below second flask, water vapor cooled (rain) and
recycled to first flask (sea)
Result: turned brown with amino acids and other
complex organic molecules
14.
15. TIME TO THINK……
We have discussed the formation of the solar system
and the formation of the terrestrial planets. Now,
what is wrong with the Miller-Urey experiment?
16. VARIATIONS OF MILLER-UREY
EXPERIMENT
Different mixes of gases to represent atmosphere
Different energy sources, like UV (sunlight)
Results: ALL PRODUCE AMINO ACIDS AND COMPLEX ORGANIC
MOLECULES
Not as much as original experiment
MUST be more sources of organic material
17. SOURCES OF ORGANIC MOLECULES
Chemical reactions in atmosphere
Lab experiments show this is likely
Organic material brought by impacts
Chemical analysis of comets and carbonaceous chondrites show that
they have organic molecules
Chemical reactions near deep-sea vents
Heat from undersea volcano can fuel chemical reactions between water
and minerals
18. TRANSITION FROM CHEMISTRY TO
BIOLOGY
Organic molecules are building blocks of life.
Low probability of forming life even if repeated several times.
Intermediate steps of high probability are necessary
19. SEARCH FOR SELF-REPLICATING
MOLECULE
Work backward from organisms that live today
DNA is double-stranded = complicated
RNA obvious candidate, more simple than DNA
Hereditary information
Can serve as template for replication
Fewer steps to produce backbone structure
20. SEARCH FOR SELF-REPLICATING
MOLECULE
Problem: RNA and DNA require enzymes to replicate
In 1980’s determined that RNA might catalyze their own replication
instead of other enzymes
Early Earth was an RNA-world
21. SEARCH FOR REPLICATING MOLECULE
On Early Earth, short strands of RNA-like molecules
were produced spontaneously partially or completely
RNA-like molecules that could replicate faster with
less errors soon dominated population
Copying errors introduced mutations, ensuring the
production of many variations of successful
molecules
Allowed molecular evolution to continue
RNA-world gave way to DNA-world
DNA less prone to copying errors
DNA more flexible hereditary material
RNA kept some of its original functions
22. ASSEMBLING COMPLEX ORGANIC
MOLECULES
Organic soup was too dilute to favor the creation
of complex organic molecules
Lab experiment with possible solution: When hot
sand, clay or rock is placed in dilute organic
solution, complex molecules self-assemble
Organic molecules stick to surface of clay
Increases density and likelihood of reactions
Strands of RNA up to 100 bases have been produced
this way
23. ASSEMBLING COMPLEX ORGANIC
MOLECULES
Other inorganic minerals may have also had a similar role
Iron pyrite (fool’s gold)
Positive charges on surface which allows organic molecules to adhere
Formation of pyrite releases energy which could be used as fuel for
chemical reactions
24. EARLY CELL-LIKE STRUCTURES
Advantages to
enclosing enzymes
with RNA molecules
Close proximity
increases rate of
reactions between
them
Isolate contents from
outside world
25. EARLY CELL-LIKE STRUCTURES
Lab experiments suggest that membrane structures
existed on early Earth
Form spontaneously
Cool down warm-water solution of amino acids
Mix lipids (fats) with water
26. NONLIVING PRE-CELLS HAVE
LIFELIKE BEHAVIOR
Grow in size until
unstable then split to
form a ‘daughter’ cell
Selectively allow other
types of molecules to
pass in/out of
membrane
Store energy in the form
of electric voltage
27. HANDEDNESS
Organic molecules come in left- and right-handed
forms
Non-biological processes have not preference
Biological processes DO have a preference
If both left- and right-handed RNA developed, why
did one die out?
29. PANSPERMIA?
Panspermia = life originated elsewhere and migrated
to Earth
Life began in rock, then kicked off the planet by an
impact
Support: organic material is everywhere, and some
bacteria can withstand large amounts of radiation and
go dormant under low atmospheric conditions
30. PANSPERMIA
2 schools of thought
School 1: life did not evolve as easily as imagined on early Earth in
timescales we’ve determined
Problem: entire solar system was under heavy bombardment at the
same time
Other possibility: interstellar migration
Problem: rock to be ejected out of its own system, then fall into ours
and hit the tiny planet of Earth
31. PANSPERMIA
School 2: life evolved easily and was everywhere with suitable
conditions
Earth was not first planet with suitable conditions
Migration of life from another planet (say Mars) dominated before
early life on Earth could
We’re Martians!!!!
34. TIME TO THINK……
Work out Exercise I. When, Where and How? in the
class activity ‘Origins of Life on Earth’.
35. EARLY EVOLUTION AND RISE OF O2
First organisms had simple metabolism
Atmosphere was O2 free, must have been anaerobic
Probably chemoheterotrophs
Obtained nutrients from organic material
Obtained nutrients from inorganic material
Modern archaea appear to be close to the root of the tree of life
Obtaining energy from chemical reactions involving hydrogen, sulfur and
iron compounds (all abundant on early Earth)
36. EARLY EVOLUTION
Natural selection probably resulted in rapid diversification
Modern DNA has enzymes that reduce the rate of mutations
RNA is not so lucky, more likely to have copying errors
Higher mutation rate in early evolution than now
37. PHOTOSYNTHESIS
Most important new metabolic process evolved
gradually
Organisms that lived close to ocean surface
probably developed means of absorbing sunlight
(UV in particular)
Once absorbed, developed method of turning it
into energy
Modern organisms of purple sulfur bacteria and green
sulfur bacteria much like early photosynthetic
microbes, use H2S instead of H2O for photosynthesis
38. PHOTOSYNTHESIS
Using water for photosynthesis developed later, perhaps 3.5
billion years ago
First appearing in cyanobacteria (blue-green algae)
By product of O2, released into atmosphere
Changed the world!
39. RISE OF O2
O2 is highly reactive
All initial O2 would react with rock and minerals in
water
O2 could not accumulate in atmosphere until surface
rock was saturated
Rocks 2-3 billion Years old called banded iron
formations, show atmosphere had <1% of current
amount of O2
Rock evidence suggests that O2 amounts in
atmosphere began to rise about 2.0 bill. Years ago
Clear evidence of O2 near current levels appears only
200 million years ago
Find charcoal (fossil fuel)
Indicates enough O2 in atmosphere for fires to burn
40. Rise of O2 would have created a crisis for life
O2 reacts with bonds of organic materials
Surviving species avoided effects of O2 because they lived or
migrated to underground locations
Many anaerobic microbes found in such locales today
41. EARLY EUKARYOTES
Fossil evidence dates to 2.1 billions Years ago
Dates to when O2 rising in atmosphere
DNA evidence suggests that prokaryotes and
eukaryotes separated from common ancestor much
earlier
O2 played a key role in eukaryote evolution
Cells can produce energy more efficiently using aerobic
metabolism than anaerobic metabolism
Adaptations of aerobic organisms could develop
adaptations that required more energy that would be
available for anaerobic organisms
42. THE CAMBRIAN EXPLOSION
Animal branch of the tree of life
Different classifications based on body plan
All known body plans made appearance in fossil record in a time
span of 40 million years
<1% of Earth’s age
Animal diversity began 545 mill. Years ago
43. COLONIZATION OF LAND
Life flourished where liquid water exist
Life on land was more complicated
Had to develop means of collecting solar energy above
ground and nutrients below
Life in shallow ponds or edges of lakes
Water evaporates
Natural selection favored that which could withstand
periods of drought
44. COLONIZATION OF LAND
DNA evidence suggests that plants evolved from
an algae
It took only 75 mill. Yrs for animals to follow
plants out of water
46. MASS EXTINCTIONS
Possible Causes
Impacts
Impact sites found for K-T boundary
Suspected for Permian extinction 245 mill years ago
Active volcanism
Climate change
External influence for copying errors
Increase in solar particles or radiation hitting surface
Local supernova
47. PRIMATE EVOLUTION
Monkeys, apes, lemurs and humans have common ancestor that lived
in trees
Tree life
Limber arms for swinging between branches
Eyes in front of head for depth perception
Offspring would be born more helpless than other animals
48. EMERGENCE OF HUMANS
Did NOT evolve from gorillas or monkeys
Share a common ancestor that lived just a few million years ago
98% of human genome is identical to genome of the chimpanzee
2% difference in genome separates the success of humans verses
chimps
Also indicates evolution of intelligence is complex
50. EMERGENCE OF HUMANS
After hominids diverged from chimps and gorillas,
evolution has followed a complex path
Numerous hominids species existed, some during
the same time period
All humans are the same species
First skull fossils that are identical to modern human
skulls dates to 100,000 years old
Our ancestors shared the Earth with Neanderthals
Went extinct 35,000 years ago
52. CULTURAL AND TECHNOLOGICAL
EVOLUTION
Have not undergone biological evolution in 40,000
years
Mutation rates are slow
Dramatic cultural changes
Transmission of knowledge between generations
Spoken to written word, thousands of years
agriculture
Technological evolution
Result of coupling between science and technology
About 100 years between industrial revolution to landing
on the Moon and generating weapons of mass destruction
53. TIME TO THINK……
Work out Exercise II. From Microbes to Complex
Organisms in class activity ‘Origins of Life on Earth’.