32
Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

  • View
    221

  • Download
    0

Embed Size (px)

Citation preview

Page 1: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Astronomy190 - Topics in Astronomy

Astronomy and Astrobiology

Lecture 13 : Life’s History

Ty Robinson

Page 2: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Questions of the Day

• What was early life like?

• How has life evolved with the Earth’s environment?

• How did life change Earth’s environment?

Page 3: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Geologic Time

Origin of life (prokarya, archaea)

Rise of atmospheric O2 (Ice age)

First ‘shelly’ fossils (Cambrian explosion)‘Snowball Earth’ ice ages

Ice age (?)

First fossil evidence for eukarya

Page 4: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

PhanerozoicTime

First shelly fossils

Age of fish

First vascular plants on landIce age

Ice age

First dinosaurs

Dinosaurs goextinct

Ice age (Pleistocene)

Page 5: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Earth’s Prebiotic Atmosphere

• dominantly N2 and CO2

0.3 bars CO2 + ? to offset the faint young Sun

• abiotic net source of O2: photolysis of H2O followed by escape of H to space

• possible high-altitude O2 source: photolysis of CO2 followed by

O + O + M O2 + MJ. F. Kasting, Science (1993)

Page 6: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Questions?Why is it difficult to find evidence for the existence of O2 in Earth’s pre-biotic atmosphere?

Humans destroyed this O2 through respiration

reactions with CO2 destroyed any atmospheric O2

the O2 was in the upper atmosphere, never reacting with the surface

the evidence has been destroyed

Page 7: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Earth’s Earliest Life

Evidence for the earliest life on the Earth comes from three different sources.

• Stromatolites (3.5 Gya)

• Microfossils (3.5 Gya)

• 12C/13C Isotopic Evidence (3.85 Gya)

Page 8: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

3.5-GaStromatolites(Warrawoona)

Prokaryotic organisms in colonies

From: Earth’s EarliestBiosphere, J. W. Schopf,ed. (1993)

Page 9: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Old and New

Archean

Modern

Page 10: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Modern StromatolitesShark Bay, Western Australia

Page 11: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

• earliest organisms were probably chemoautotrophs, i.e., they derived their energy from chemical reactions and took their carbon from the environment

Examples• Sulfur reducers: S + H2 H2S (stinky!)

sulfur hydrogen hydrogen sulfide

• Methanogens: CO2 + 4 H2 CH4 + 2 H2O

What effect would life have had on the earlyatmosphere?

Page 12: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

• photosynthesis may well have been invented early, but since there was no surface oxygen, it originally used H2 (or H2S) rather than H2O

Oxygenic photosynthesis (prevalent today)

CO2 + H2O (+ h) CH2O + O2

Anoxygenic photosynthesis (early Archean)

CO2 + 2 H2 (+ h) CH2O + H2O

CO2 + 2 H2S (+ h) CH2O + H2O + 2 S

no O2 production!

Page 13: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Questions?Why is it difficult to determine the time when forms of non-oxygenic photosynthesis evolved?

the microbes were too small

the products of these reactions are also created abiotically

the products of these reactions are not as reactive as O2

the evidence has been destroyed

CO2 + 2 H2 (+ h) CH2O + H2O

CO2 + 2 H2S (+ h) CH2O + H2O + 2 S

Page 14: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson
Page 15: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

How do we learn about ancient organisms?

1. from the fossil record (but this isn’t very good prior to the Cambrian)2. from molecular phylogeny, that is, the sequencing of DNA and RNA

Page 16: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

The “Universal” Tree of Life

• rRNA—ribosomal RNA

• ribosomes: organelles within cells that are responsible for making proteins

• ribosomal RNA mutates slowly trees constructed from this molecule show deep divergences in evolution

Page 17: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

methanogenicarchaea

Courtesy ofNorm Pace

“Universal”(rRNA) Tree

Of life

hyperthermophiles root?

Page 18: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Cyanobacteria and The Rise of Oxygen

• atmospheric O2 rose 2.3 Gya

• land plants weren’t around until about 425 Mya

• Cyanobacteria (prokaryotes) were responsible

Page 19: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

cyanobacteria

Page 20: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Implications• oxygenic photosynthesis was only invented once!• cyanobacteria invented it, and then some eukaryote

‘imported’ a cyanobacterium (endosymbiosis)• higher plants and algae descended from this primitive

eukaryote

Page 21: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Geological O2 Indicators

H. D. Holland, in Early Life on Earth, S. Bengtsson, ed. (1994)

Page 22: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Banded Iron Formations• (>1.8 Ga)

• can only form when large amounts of iron are dissolved in the oceans

• this is only possible if oxygen is not present

• to form the layering, periods of no oxygen have to be alternated with a condition that oxidizes iron• cyanobacterial bloom?• iron oxidizing bacteria?

Page 23: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson
Page 24: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Timing the rise of oxygen• ratios of different sulfur isotopes in rocks suggest

that O2 started to rise 2.35 Gya

Page 25: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

The Story So Far

• bacteria, archaea and eukaryotes are all well established by 2.1 Gya (although they were all probably around much earlier than that)

• oxygen rises at 2.3-2.4 Gya • …then nothing much happens until….• oxygen rises again near 545Mya to nearer

present-day levels (~60% of present day) • at 545 Mya we get the ‘Cambrian Explosion’

Page 26: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Phyla

• biologists classify animals according to “body plan”

• mammals and reptiles are “phylum Chordata”• insects, crabs, spiders are “phylum Arthropoda”

• there are about 30 different phyla today

• Almost all these phyla first appeared between 545-505 Mya!

Page 27: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

The Cambrian Explosion

• Why did this occur so suddenly? Why hasn’t it happened since?

Page 28: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

The Timing of the Cambrian Explosion

• oxygen rose to the present-day level just prior to the Cambrian explosion– respiration needed for complex organisms?

• organisms may have developed a critical amount of complexity so that large diversity could evolve rapidly

• Earth was just coming out of a Snowball Earth phase

• efficient predators hadn’t evolved yet– maybe why it hasn’t happened since?

Page 29: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Crawling from the Primeval Slime…

• early microbial life protected itself from UV in water

• for land-based organisms, it is tougher– need UV shield

• plants arrived on land 475 Mya– probably evolved from algae– no land animals yet to eat them!

• by about 400 Mya amphibians and insects were eating plants

• dinosaurs and mammals arrived 245 Mya

Page 30: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Not a Bed of Roses!

Page 31: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Questions of the Day

• What was early life like?

• How has life evolved with the Earth’s environment?

• How did life change altered Earth’s environment?

Page 32: Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 13 : Life’s History Ty Robinson

Quiz

3 - What is one thing you did not understand from today’s lecture?

2 - What are two possible explanations for the “Cambrian Explosion”?

1 - Describe one possible location for the origin of life. What are the pros/cons for this location?