astr-3040:astrobiology day 12 the origin & evolution of life on earth chapter 6
TRANSCRIPT
ASTR-3040:Astrobiology
Day 12
The Origin & Evolution of Life on Earth
Chapter 6
Homework
Due Tue. March 1
Chapter 6: 1, 4, 8, 13, 23, 28, 34, 35, 42, 46, 49, 52, 53, 56
Exam 1 – Tuesday March 1 Chapters 1 - 6
Searching for Life's Origins Geologic record details much of life history.
Evolution theory tells us how life has changed.
But, how did life arise?
Three lines of fossil evidence.
Stromatolites – date to 3.5 Gyr. Photosynthesis
Microfossils – date to 3.5 Gyr.
Isotopic evidence
Stromatolites
Photosynthetic at least in top microbes.
Modern ones resemble old fossils.
Date to 3.5 Gyr
Microfossils
Biological?
photosynthetic?
Australia – 3.5 Gyr
Africa – 3.2-3.5 Gyr
2.7-3.0 Gyr - conclusive
Isotopic Evidence Carbon-13 evidence of 3.85 Gyr life
But, no microfossils in the rocks
Sedimentary – so fossils might be destroyed.
Implications?
The carbon dating – if it stands – puts life at 3.85 Gyr ago – at least. Rocks this old are scarce.
Life itself must be older than this.
Arose and colonized Earth in ~100 Myr?
Probably after the LHB period (4.2-3.9 Gyr)
Suggests life will arise and spread quickly.
What did early life look like?
Evolutionary relationships. Track changes through DNA sequence.
Large difference in genome between two life forms indicates a longer time since they shared common ancestor.
Extremophiles (hyperthermophiles) are probably the closest to first life. Chemoheterotrophes?
Where? Deep-sea hot water vents – most likely
Origin of Life
Experiments try to re-create chemical conditions on Earth indicate life may have started through natural, chemical processes.
Panspermia – could life have originated elsewhere and been transported to Earth?
How Did Life Begin?
Miller-Urey Experiment 1950s
H2O and CH
4, NH
3
Add electric spark
Pass condensates back to water flask.
Amino acids and many organics.
But, what was 1st atmo?
Other sources of organics
Chemical reactions near deep-sea vents
Material from space – meteorites, comets Organics can form in space?
Protoplanet & solar nebula
When was chemical ==> biological transition? DNA is a complex molecule.
RNA
Single strand rather than double
Easier to manufacture
Recent (early 1980s) work show RNA can self-catalyze using rybozymes
Experiments show “clay” can facilitate self-assembly of complex, organic molecules.
Abundant on Earth and in oceans
Laboratory experiments
Then what?
Assuming self-replicating RNA is formed Rapid modification –
natural selection
Mutations
Then what?
Pre-cells Keep molecules
concentrated – increase reaction rates
Protect from the outside world
Primitive structures form naturally and easily.
Pre-cells
Amino acids will form spherical structures when cooled. Grow by adding chains
Split to form daughters
Lipids in water form membrane-like structures
Put it together 1. Some combination of atmo. chemistry, deep-
sea chemistry, molecules from space.
2. More complex molecules -RNA- grew form the building blocks. Some become self-replicating.
3. Membranes form spontaneously.
4. Natural selection among RNA molecules . Eventually these become true living organisms.
5. Natural selection – diversity. DNA becomes favored hereditary molecule.
Migration of Life to Earth
We've seen some organisms survive in space.
Could life arise on Venus or Mars first?
Possibility of migration 20,000 meteorites cataloged
~36 come from Mars.
1. Large impacts.
2. Survival during transit.
3. Atmo. entry.
ALH8400
Transit
Endoliths could survive both blast and entry.
Transit survival depends on time in space. Most rocks millions or billions of years
A few ten years or less.
Probably no interstellar meteorites (none known).
Why migration? Does life form easily on early Earth?
Does life form too easily on any planet?
Implications of Transit
Of the early solar system planets Mercury and Moon are probably not favorable.
Early Venus and Mars might have been hospitable.
Migration from Earth?
Why migration?
Evolution of Life
Major events. Early microbes – anaerobic (primitive atmosphere).
Chemoautotrophes – underwater probably
Photosynthesis – multiple steps to arise ~3.5 Gyr ago (stromatolites)
Oxygen crisis ~2.4 Gyr ago?
Evolution of Eukarya – cell complexity Symbiosis?
Mitochondria & Chloroplasts
Cambrian Explosion
Life started slowly (?)
Multi-cell organisms ~1.2 Gyr ago Microbes had 2+ Gyr by themselves
Animals – little change from 1.2 – 0.7 Gyr ago
Then a huge diversification 30 body plans 40 Myr for all this to occur.
Why Cambrian Explosion
Oxygen level reached a critical value Survival of large, energy-intensive life forms
Genetic diversity of eukaryotes
Climate change – coming out of snowball
No efficient predators May explain why no similar explosion since.
Colonization of Land
Oxygen level reached a critical value Ozone could form UV protective layer.
Need to evolve a method to obtain oxygen and nutrients.
Plants first ~475 Myr ago Probably evolved from alga.
Specialization in larger plants (leaves, roots)
Amphibians and insects within 75 Myr
Carboniferous Period By 360 Myr ago – vast forests, insects
Flooded land masses – so little decay These deposits formed coal.
Rise of Oxygen Critical to animal life
Molecular Oxygen – reactive gas. Disappears quickly if not replenished
Early – oxidation reactions (rust, iron-oxides...)
Now – use by animals
Cyanobacteria
Timing Fossil and rock studies
2-3 Gyrs – banded iron formations
< 1% of present level
Sulfur isotope studies ~2.35 Gyrs for oxygen.
Cyanobacteria started ~2.7 Gyrs (350 Myr gap) Removal by non-biologicals – oxidation
Slow build-up – no “explosion”
200 Myr ago – first charcoal
Implications If Earth is typical – probably few planets with
complex, oxygen using life (rqr ~4 Gyr to form)
If Earth was delayed – complex life might be flourishing elsewhere.