In the beginning
…??
Dr. Craig Benjamin
Bright Horizons 19
Big History Lecture 2
Part A: The Origins of the
Universe
Part B: The Emergence
(and Importance!) of
Stars and Galaxies
Part C: The Making of our
Solar System and
Planet
Part D: Origins and
EvoluJon of Life
Today we cross the first Five
Thresholds of complexity!
1.
The Universe [Cosmology]:
13.8 BYA
2.
The first Stars [Astronomy]:
13.6 BYA
3.
Chemical elements [Chemistry]: from 13.5 BYA
4.
Planets and our earth [Geology]:
4.5 BYA
5.
Life [Biology]:
3.8 BYA
6.
Human beings [Anthropology]: c. 200 KYA
7.
Agriculture [Archaeology]: c. 10 KYA
8.
Modern Society [History]: c. 200 Years ago!
9.
Where’s the next threshold? [Futurology] ...
‘ How did it all begin ’ ?
• All societies have asked this question, and devised different ways of answering it with their Creation Stories
The universe and everything in it was made by Gods
The universe and everything in it was born from Nothing
The universe is Eternal
But all CreaJon stories have to face the paradox of beginnings:
• Can SOMETHING come from NOTHING?
– If not, where do gods come from?
• Can SOMETHING be ETERNAL?
– If so, how is eternity created?
• Can any CreaJon Story solve these conundrums?
Modern Quantum Physics thinks it can – with
The Big Bang Theory!
Everything in the universe was created by a subatomic particle which popped into existence 13.82 billion years ago!
The Big Bang
Theory emerged from aQempts to map the cosmos
• 19 th century astronomers tried to measure:
– The Distance to Stars
• Using parallax (to esJmate distances to nearby stars)
• And variable stars or ‘ Cepheids ’ (to esJmate distances to distant stars-‐-‐HenrieQa LeaviQ)
– And how Stars Move
• Using spectrometers and the ‘ red shiT ’ phenomenon to determine if galaxies were moving towards or away from us
Using the ‘ Red ShiT ’ to understand the Universe in the 1920s,
Edwin Hubble Found …
– Most distant stars and galaxies are ‘ red-‐shiTed ’ (i.e. they are moving away from us)
– The further away they are, the faster they are moving away from us
– Which means the universe is expanding
– Which means it was once infinitesimally small
• This is the FUNDAMENTAL PIECE OF EVIDENCE FOR …
‘ BIG BANG COSMOLOGY
’
…
• Before 13.82 billion years ago, there is nothing we can really say
– We have no evidence, and calcula?ons go crazy
– Perhaps Time and Space did not even exist
• Then, for reasons we cannot explain
– Something appeared!
§ Around 13.82 billion years ago a ‘ speck ’ appeared
– Billions of billions degrees Celsius hot
– Not sure
• What there was before the speck
• Why it appeared
• Physicists cannot answer these quesJons yet (though there are many theories), but it has a coherent account from the moment the speck/singularity/first parJcle appeared!
• 10
-‐35
: Cosmic inflaJon created a large patch of space filled with a lumpy quark soup
• Mater and anJmaQer both existed in a state of tension
• Four fundamental forces also appeared at 10 -‐35 second aTer the Big Bang:
» Gravity (pen drop)
» ElectromagneJc (magnets)
» Strong force (glues neutrons
and protons together)
» Weak force (radioac?ve decay)
• 10
-11
: Matter tried to gain the upper
hand over antimatter
• 10
-5
: Protons and neutrons formed
from quarks
• Then a period of matter/
anti-matter annihilation …
BANG !!!!!!
Where there had been nothing, now there was everything.
A whole universe -- tiny, and fantastically hot .
For an instant, it expanded faster than the speed of light.
Then it slowed down and began to cool, but it kept expanding (and it still is today).
• The temperature within dropped enough for the first stable atoms to form
• Prior to that, the universe was like a
‘foggy soup’
• When atoms formed, the fog cleared and energy and light began to flow freely, releasing cosmic microwave radiation
• Gravity then continued to amplify differences in the gasses that filled space
Crucial Evidence:
Cosmic Background
RadiaJon
• If the universe began in a hot, dense state, there would have been lots of radia?on (Gamow, Alpher and
Hermann, 1948 )
• There should be some trace of this radiaJon today (5K or -‐268C)
• Sure enough, CBR was detected in 1965, and confirmed by satellites in the 80s and 90s
• Early universe was billions and billions of degrees hot, too hot for atoms
• ParJcle physicists have tried to replicate these condiJons, smashing apart atoms
• Predicted that the universe would be made of 25% helium and approx. 75% hydrogen, which matches exactly what has been found hepwww.rl.ac.uk
Particle smashing in the UK!
So is the ‘ Big Bang Theory ’ true?
• Absolute certainty is unaQainable
• In the future, parts of this story may begin to look as strange as earlier stories look to us now
• BUT:
– Big Bang Cosmology fits a huge amount of data
– Big Bang Cosmology, unlike all earlier creaJon stories, is accepted globally, by scienJsts of all cultures
– Big Bang Cosmology is by far the best ‘CreaJon
Myth’ available if you happen to live in the 21 st century!
B. The Emergence (and
Importance ) of Stars and Galaxies
• From SIMPLICITY to COMPLEXITY
– The early universe was SIMPLE
– Gradually, COMPLEX en??es
appeared
– Beginning with stars and
galaxies
• INCREASING COMPLEXITY
is a central theme of big history
• How did the universe make stars?
• Energy: e.g.
– Cosmic background radia?on
– Gravity
• MaQer:
– Huge clouds of
• Hydrogen atoms (75%) and
• Helium atoms (25%)
• But that was enough to
make everything else!
Hydrogen Clouds
Take Gravity, Hydrogen and Helium, and …
• Gravity magnified tiny differences in temperature and density
• Making dense regions denser
• Pulling atoms of Hydrogen and Helium into huge clouds
• Which got more compressed
• And heated up (like air when pumping up a tire)
A region of star formation today:
The ‘ Cone
Nebula ’
(observed by the
Hubble Space
Telescope)
When they got
HOT enough (c. 10 million degrees C) hydrogen atoms fused together with the power of millions of hydrogen bombs, releasing huge amounts of energy.
Billions of stars were formed, starting a mere 200 million years after the big bang.
They clustered together in galaxies, each containing hundreds of billions of new stars .
A Supernova in the Large Magellanic Cloud
A star starts out as a huge cloud of gas and matter, like this cloud in the Orion Nebula
The cloud collapses and heats up until a star is formed. It may shine for billions of years
Then it dies. If it ’ s big enough it will die in a huge explosion called a supernova
• When stars run out of hydrogen
– Their centers cool and collapse
– Which raises pressure and density
– Which generates very high temperatures again
• If temperatures reach 100 million degrees C
– Helium atoms starts to fuse into new elements
– When stars run out of helium, they collapse even more violently, which creates even higher temperatures …
– In large stars, a series of collapses forge elements such as oxygen, carbon and nitrogen, up to iron (No.
26 on the Periodical Table)
• How are the other elements created?
• In ‘ SUPERNOVAE ’
– Huge stars that explode so violently that, for a few days, a supernova can outshine a galaxy
– Supernovae , seen from earth, look like new stars (like the star of Bethlehem)
– In just a few seconds a supernova can cook all the other elements of the periodic table
– Then it scaQers them through that region of the Universe
– There was a supernovae close to the region in which our Solar System formed!
THE PERIODIC TABLE
STAGE 1: big bang
Hydrogen (1 proton) Helium (2 protons)
STAGE 2: fusion
Iron (26 protons)
Uranium
(92 protons)
STAGE 3: supernovae create all the rest!
Gold (79 protons)
So stars made the materials of our world & spread them through the galaxy
Gold
Iron +
Oxygen
= Rust
And the materials for carbon-based life-forms such as gerbils and … US
Carbon
(diamonds)
Gold leaf covers this statue of the goddess Serket, found in the tomb of King Tutankhamun of Egypt, and the wall behind her. Gold leaf is made by hammering solid gold metal until it is very thin.
Microsoft ® Encarta ® Reference Library 2003. ©
1993-2002 Microsoft Corporation. All rights reserved.
• Solar systems most probably form from a huge cloud of material called a solar nebula
• The sun absorbed about 99.9% of the cloud; the other 0.1% of the Solar Nebula – orbited the new sun in a series of rings
• The remnant cloud contained gases, dust, ice (much the same material we find in comets today)
• These remnants formed the Solar
System
Solar Nebula Formation. The Star ‘ Vega ’ surrounded by a ring of dust & gas
[Reconstruction]
• Within each orbit: EXTREME VIOLENCE
– Dust, ice and gas par?cles collided
– And stuck together to form ‘ planetessimals ’
• Planetessimals (10-‐100 km in diameter)
– Grew like snowballs
– Their gravita?onal pull increased
– They aWracted other ‘ planetessimals ’ and formed …
• Protoplanets (100-‐1000 km in diameter)
• Eventually, in each orbit, one large protoplanet absorbed all the others
• To form Planets! One to each orbit
The Planets (Earth is third from the Sun-‐-‐ not to scale )
The formation of one planet was particularly important for the future of all of us!
(First color photo of Earth from space, appeared on the cover of Time in 1970)
Extremely hot, because of:
1.
Violent collisions with other objects
2.
Internal radioactivity
3.
Increasing internal pressure
As a result, the earth melted and liquefied through a process called differentiation
Heavier metals melted and sank to the center
Lighter metals rose to the surface to form a crust
Gases bubbled up to make the earth ’ s first atmosphere
So the earth acquired a structure
A structure that looked like this
Surface Core
Above
Surface
!
• Things stabilized:
– Earth cooled, so
• Water vapor stored in the atmosphere rained
down in thunderstorms for millions of years
• Seas were formed
– Meteorites arrived less frequently
– Undersea thermal acJvity pushed conJnental crust around so that the surface of the earth constantly changed. The theory of plate tectonics explains:
– How mountains are created
– Why volcanoes and earthquakes occur
– How the conJnents acquired their posiJons
– The shape of the modern world
Face of the Earth 180 MYS Ago:
Pangaea: the super-‐conJnent
Jurassic (Dinosaurs, 1 st birds)
North
America
Face of the Earth 120 MYS Ago
Pangaea starts to break up
Cretaceous (1 st flowering plants, marsupials)
LAURASIA
North
America
GONDWANALAND
Cretaceous asteroid impact
(dinosaurs vanish, mammals flourish)
North
America
Asteroid impact
Watch India
Humans flourish
India has collided, creating the Himalaya!
North
America
Standing at 5,500 meters on the summit of Gokyo Ri in the Nepalese
Himalayas, close to the highest point on Planet Earth (above my left hand)!
• The core ideas of modern Astronomy:
– Explaining the Universe
• The core ideas of modern Earth Sciences
(Geology):
– Explaining our Earth
• NOW: The core ideas of
modern Life Sciences (Biology):
– Explaining Life!
All living organisms share 3 key features
1.
AdaptaJon
– Species of living things slowly change & find new ways of extrac?ng energy from their surroundings
2.
ReproducJon
– Living things preserve adapta?ons by replica?ng them
3.
Metabolism
– Living things find the energy needed to support complex adapta?ons
Adapta?on
, preserved by
Reproduc?on
, powered by
Metabolism , explains why flies are more complex than stars
Life introduces a new level of complexity
Remember our eight major thresholds of complexity?
1.
The Universe [Cosmology]:
13.8 BYA
2.
The first Stars [Astronomy]:
13.6 BYA
3.
Chemical elements [Chemistry]: from 13.5 BYA
4.
Planets and our earth [Geology]:
4.5 BYA
5.
Life [Biology]:
3.8 BYA
6.
Human beings [Anthropology]: c. 200 KYA
7.
Agriculture [Archaeology]: c. 10 KYA
8.
Modern Society [History]: c. 200 Years ago!
9.
Where’s the next threshold? [Futurology] ...
Biology’s biggest challenge has been explaining how life adapts
How do living organisms ‘ adapt ’ to their environment ?
The human eye is exquisitely ‘ adapted ’ for seeing
How did it get that way ?
• Linnaeus: Founder of
‘ taxonomy ’
– Life is fixed : God made creatures already ‘ adapted ’ , and they haven ’ t changed since
• This is the traditional answer:
– animals are ‘ well adapted ’ because they are designed by a benign Creator
• But, there were problems with this theory …
Linnaeus
(1707-78)
ay
Fossilized leaves
Trilobites: 200 Mill. Ys. old .
Breeders know that living organisms can change through arJficial selecJon e.g. modern breeds of dogs are all descended from wolves
Charles Darwin (1809-‐1882):
Modern Theory of EvoluJon
Twenty years a^er a voyage round the world he reluctantly published his extraordinary theory in …
The Origin of Species by Natural Selection, published in 1859
Darwin was inspired by what he saw on the Galapagos Islands
14 nearly identical species of finches, but their beaks and heads were all slightly different
Why were the beaks and heads so different?
Was it a form of adaptation
• Trees on the Galapagos islands varied slightly
• On each island finches ’ beaks were perfectly adapted to the local trees and nuts
•
• So each species had made Jny
‘ adaptaJons ’ to the local environment
HOW? Galapagos Cactus
Finch
‘
’
• Darwin concluded that he was seeing the first stages in the creaJon of new species
– Tiny variaJons between individuals get magnified when geographical barriers (such as canyons or seas) stop individuals of the same species from maJng
– Over Jme, groups separated geographically diverge more and more from each other
• Eventually, when the groups can no longer interbreed, they form new species
• This is the CORE IDEA of modern biology – evoluJon by ‘ Natural
SelecJon ’
• The environment constantly changes
– So the definiJon of ‘ fitness ’ constantly changes
– So ‘ natural selecJon ’ is an endless process
• This explains the huge
variety of organisms
that have inhabited
our earth
• Natural SelecJon is the
source of the rich biodiversity on earth!
ImplicaJons of ‘ Natural SelecJon ’
1.
Blind processes can create things as complex as living organisms
2. All living creatures are related
– This means that all living creatures share the same ancient ancestors
3. Humans are closely
related to apes
– So humans and apes share common ancestors quite recently (in biological terms)
’
• Fossils
• SimilariJes between species (embryos)
• Geographical distribuJon of species www.micromacro.co.uk/
• We can see evoluJon at work (fruit fly, HIV, other viruses)
• We know how heredity works ( DNA )
• We can show geneJcally that all living organisms are related
• Mitochondrial DNA shows that all human females are descended from a common ‘mother’
• Darwin ’ s theory of evoluJon is now the core idea of modern Biology
– As fundamental as ‘ Big Bang
Cosmology ’ is in Astronomy
– Or ‘ Plate Tectonics ’ in Earth
Sciences
But one big question remained for biologists to address …
How did life appear in the first place?
pharyngula.org/ index/weblog/2004/02/
1.
The Earth made simple organic molecules
(amino acids, nucleoJdes, phospholipids in fats, etc.)
2.
These turned into organic chemicals that evolved and behaved a bit like living organisms (chemical evoluJon)
3.
DNA emerged to control replicaJon
(the geneJc code)
Making Simple Organic Molecules:
The Urey-‐Miller Experiment
• Create a model of the early atmosphere in a flask
• Energize it with heat and electric sparks, and wait:
• Within 7 days:
– a dark red sludge appears, containing many elements from which life is made:
• Amino acids (from which proteins are made)
• NucleoJdes (from which DNA is made)
• Phospholipids (from which cell membranes are made)
• So: making the raw materials of life is easy!
Making More Complex Organic
Chemicals: ‘ Chemical EvoluJon ’
• Under the right condiJons
– Organic chemicals link into huge chains of millions of atoms to form proteins and nucleoJdes
Amino acids are simple
Proteins are made from chains of amino acids
Proteins fold up into complicated balls of matter
Where were condiJons right for this to have first taken place?
Near deep-‐sea volcanoes
Chains of deep-sea volcanoes
• CondiJons were ideal:
– No ultraviolet rays
– No meteorite collisions
– Heat from the earth ’ s core
– Plenty of water
– Plenty of chemicals
• Here is where the first life probably formed!
• Now we have complex organic chemicals
– Made from the same stuff as living organisms
– With metabolism (taking in energy)
– Capable of ‘ adapJng ’ (chemical evoluJon)
– They can even reproduce in a fashion
• But
– They reproduce inaccurately , so they cannot preserve complexity over many generaJons
– The key to life is more accurate reproducJon
• How do you precisely reproduce something with billions of carefully arranged molecules?
The GeneJc
Code!
• DNA: the molecule of life
• How does it work?
– If organisms reproduce too perfectly , adapta?on and change are impossible
– If they reproduce too imperfectly , they cannot retain the informa?on needed to construct viable organisms
• DNA achieves a perfect balance:
– Accurate copying
– With just a dash of variaJon
– This is the key to biodiversity
Finally, a brief history of life on
Earth: Tale of increasing complexity
8 stages in the history of life on earth
1. First organisms
2. Photosynthesis
3. Prokaryotes à Eukaryotes
4. Sexual reproduction
5. Multi-celled organisms
6. Living on the land
7. Vertebrates
8. Mammals
1. The earliest living organisms on earth were ...
• Prokaryotes
– Too small to be seen with the naked eye
– No nucleus: genes float freely inside
DNA but no nucleus
• Some organisms rose to the surface of the seas
• And learnt to extract the energy of
sunlight through
PHOTOSYNTHESIS
(like plants today)
Why plants are green
Chlorophyll is green, and is present in all plants
Chlorophyll molecules are where photosynthesis occurs
‘
’
‘
’
• The oxygen produced by photosynthesizers was poisonous for most species
• But eventually, some bacteria learnt to exploit the excepJonal chemical energy of oxygen
• Those that could use oxygen flourished and became more complex:
• The first ‘ eukaryotes ’
– They used the energy from oxygen and/or sunlight
– Their genes were protected inside the nucleus
– They were much larger and more complex than prokaryotes
Eukaryotes (10 – 100 times as large as prokaryotes )
The nucleus protects the cell ’ s DNA
Mitochondria generate energy from oxygen
What was bacterial sex like?
• For most prokaryotes it was boring: they just cloned
• But some eukaryotes began to swap genes before reproducing. Result?
– Their offspring were more varied
– Greater variety accelerated the pace of evolu?onary change
Tube sponges may be similar to the earliest multi-cellular organisms
• For c. 3 billion years, all life on earth consisted of single-‐celled organisms
• From c. 600 million years ago:
– Some cells gathered together in
‘ socieJes ’ (like sponges)
– Some cells specialized , and became more dependent on their neighbors
– Some became so dependent on other cells they turned into large, single organisms
The first vertebrates probably looked like
‘ lancelets ’ .
They are extremely simple fish, with no heart and no brain!
7. 1st large organisms to survive on land: from c. 370 million years ago
• Surviving away from water was tough
– Supplies of water had to be found
– Skins needed to prevent excessive dryness
– Eggs and offspring needed to be protected
• Which large species got there first?
– Plants were probably first, more than 400 million years ago
– Followed by insects
– Then the first land animals,
early forms of amphibians,
c. 370 million years ago Ichthyostega lived about 370 million years ago
• Mammals were
– Warm-‐blooded
– Fed their young with milk
– Had fur
• The first mammals were small,
shrew-‐like creatures living in a
world dominated by dinosaurs
Morganucodon lived c. 250 million years ago.
It was the size of a small mouse or shrew
st
65 million years ago, a giant meteor came crashing down to earth, and the dinosaurs were no more.
This allowed mammals to prosper and evolve!!
Primates lived in trees.
To survive in trees they needed:
• 3D vision and
• large brains to process visual informaJon
• And hands that could grip with precision
Imagine living in a tree without these abiliJes: you ’ d fall out!
According to all the available scienJfic evidence we are descended from primates!
Bonobo chimps – our very close relatives (98.4% of our DNA is identical to that of chimps)
All chimps, apes and hominines
(including humans) are descended from a common ancestor who lived 8 MYA
• In this lecture we have covered almost 13.8 billion years of history, and now the bizarre species of homo sapiens is poised to join the modern creaJon myth!
•
actually be very difficult because of the incredible complexity of human socieJes!
• Next Jme we bring our story closer to the present
• Before taking it hundreds, thousands, and even billions of years into the future in our