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Life in the Universe
Course Evaluations Open
FINAL EXAM:
8:00 AM FRI Dec. 16
Review Session
6-8 PM Today
PHYS 1410
Homework #6 Due Now
1
Baryons
4%
Dark Matter
23%
Dark Energy
73%
Contents of the Universe
“ΛCDM”
Hot Big Bang
+
Dark Energy
+
Dark Matter
is now called
THE ANSWER:
Here there
be
dragons!
2
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Chapter 18
Life in the Universe
3
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Evolution
• The unifying concept of biology
• Simple and general enough to work
everywhere, so we’ll discuss it
4
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
5
3
The Fact of Evolution
• Forms of life change over time, via descent
with modification
• Thatʼs it!
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
6
4
The Theory of Evolution
• Characteristics of population are most
strongly influenced by individuals who
leave the most viable offspring
Seems uncontroversial, even tautological!
• Variation: mutation, sex, horizontal gene
transfer, neutral drife, incorporation of cells
• Selection: natural/sexual
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
7 14
Misconception: Evolution is
Incompatible with Religion
• Question 1a: if I accept evolution, must I be
an atheist?
• Question 1b: if we agree we are descended
from animals, do we have no ethical guides?
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
8 15
Incompatible With Religion?
• No!
• Clergy letter project:
>11,000 ministers
signed in US alone
• Affirms evidence for
evolution; not at all in
conflict with personal
religious beliefs
http://openparachute.files.wordpress.com/2008/02/charles-darwin.jpg
http://www.clergyletterproject.net/clp140_100.gif
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
9
16
Must We Act Like Animals?
• No, how silly!
• Does gravity mean
that you have to push
people down stairs???
• Evolution is a
description of what
happened, not a guide
• Ethics comes from
other sources http://www.looptvandfilm.com/blog/homerevolution.jpg
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Earliest Life Forms
• Life probably arose on Earth around 3.8
billion years ago, after the end of heavy
bombardment.
• Evidence comes from fossils and carbon
isotopes.
10
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Fossils in Sedimentary Rock
• relative ages: deeper layers formed earlier
• absolute ages: radiometric dating
11
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Chalk (a form of limestone) consist mainly of coccolith biomicrites formed from the skeletal elements
of minute planktonic green algae, associated with varing proportions of larger microscopic fragments
of bivalves, foraminifera and ostracods.
White Cliffs of Dover
12
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Fossils in Sedimentary Rock
• Rock layers of the Grand Canyon record 2
billion years of Earth’s history.
13
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Earliest Fossils
• The oldest fossils
show that bacteria-
like organisms were
present over 3.5
billion years ago.
• Carbon isotope
evidence pushes the
origin of life to
more than 3.85
billion years ago.
Thrombolites in Lake Clifton, Western
Australia. Also a less evolved organism
at upper right 14
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
The Geological Time Scale
15
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Brief History of Life
• 4.5 billion years — Earth forms
• 4.4 billion years — early oceans form
• 3.5 billion years — cyanobacteria start releasing
oxygen
• 2.0 billion years — oxygen begins building up in
atmosphere
• 540–500 million years — Cambrian Explosion
• 225–65 million years — dinosaurs and small
mammals (dinosaurs ruled)
• Few million years — earliest hominids
• < 10,000 years — Our civilization
16
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Necessities for Life
• Nutrient source
• Energy (sunlight, chemical reactions,
internal heat)
• Liquid water (or possibly some other liquid)
Hardest to find on
other planets
17
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Necessities for Life
• Nutrient source
• Energy (sunlight, chemical reactions,
internal heat)
• Liquid water (or possibly some other liquid)
There is life everywhere on Earth where
there is liquid water at least part of the time
18
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
19
36
Life Deep in Rock
• Probably most of the biomass on Earth!
• So far, record is almost three miles below
the surface
• Also found miles below seafloor
• Live in rock cracks; can remain in stasis for
many years (thousands? more?) until there
is some water
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
20
37
Wild Speculation
• Depth limited by heat
Need liquid water
• Mars is smaller, has
cooled off faster
• Probably much thicker
part of crust that can
harbor life
• Might there now be
more living biomass on
Mars than on Earth?
http://www.windows.ucar.edu/mars/images/mars1.gif
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
21
38
Undersea Thermal Vents
• Near volcanic vents
• Rich with minerals
• Bacteria/archea use
the nutrients
• Other things eat them
• Whole ecosystem!
http://ocean-ridge.ldeo.columbia.edu/courses/subgeol/hot_springs/smokers.gif
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Searches for Life on Mars
• Mars had liquid water in the distant past.
• Mars still has subsurface ice—possibly
subsurface water near sources of volcanic heat.
22
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Could there be life on Europa or
other jovian moons?
23
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Titan
• Surface too cold for liquid water (but deep underground?)
• Liquid ethane/methane on surface
24
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Habitable zone
25
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Habitable Planets
Definition:
A habitable world contains the basic
necessities for life as we know it, including
liquid water.
• It does not necessarily have life.
26
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Constraints on star systems:
1. Old enough to allow time for evolution (rules
out high-mass stars — 1%)
2. Need to have stable orbits (might rule out
binary/multiple star systems — 50%)
3. Size of “habitable zone”: region in which a
planet of the right size could have liquid water
on its surface
Even so… billions of stars in the Milky Way seem
at least to offer the possibility of habitable worlds.
27
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
The Bottom Line
We don’t yet know how important or
negligible these concerns are.
28
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Interstellar travel (?)
29
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Current Spacecraft
• Pioneers & Voyagers beyond Pluto now
• These spacecraft travel at <1/10,000 c;
100,000 years to the nearest stars
Pioneer plaque Voyager record
30
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Difficulties of Interstellar Travel
• Far more efficient engines are needed.
• Energy requirements are enormous.
• Ordinary interstellar particles become like cosmic rays.
31
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Even at half light-speed...
• Takes 9 years to reach the nearest star
– more with acceleration & deceleration
• Takes just as long to get back
• There are 32 stars within 12 light-years
• That’s about all that can be explored in a
human lifetime
– 24 years to grow & train
– 24 to get there, 24 to get back
– you’re 72 upon return
32
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
SO...
• The universe is BIG
• and really, really OLD
What are the chances that aliens are visiting us just now?
(Consider what you’d find if you had visited Earth at any
random moment in its history.)
33
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
34
14
The Burden of Proof
• Suppose I claim to have seen an alien
• Is it up to you to disprove me?
• No!
• Carl Sagan: “Extraordinary claims require
extraordinary proof”
• What does this mean in practice?
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
35 15
First Claim
• Suppose I told you
that yesterday I saw a
friend walking down
the street
• Would you believe
me? If not, what level
of proof would you
require?
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
36
16
Second Claim
• Now suppose I told
you that the other day
I saw a 100-foot tall
cyclops walking down
the street
• Would you believe
me? If not, what level
of proof would you
require? http://bearah718.tripod.com/sitebuildercontent/sitebuilderpictures/cyclops.jpg
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
37
17
Importance of Discovery
• Suppose visits by aliens were established
beyond any question
• This would be the most important discovery
in history
• As a result, we need to apply the highest
standards of evidence to any alien claim
Must be absolutely indisputable
• ...and at this stage, no alien claim is even
remotely indisputable
© 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley
Alien life is likely
• LOTS of stars
• No reason to presume Earth is 100% unique
Visits from aliens very unlikely
• Distance between the stars is vast
• Nothing special about right now
• If aliens did make it to earth, they only
have a one in a million chance of arriving
while we’ve been around
38

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life in the Universe.pdf

  • 1. Today Life in the Universe Course Evaluations Open FINAL EXAM: 8:00 AM FRI Dec. 16 Review Session 6-8 PM Today PHYS 1410 Homework #6 Due Now 1
  • 2. Baryons 4% Dark Matter 23% Dark Energy 73% Contents of the Universe “ΛCDM” Hot Big Bang + Dark Energy + Dark Matter is now called THE ANSWER: Here there be dragons! 2
  • 3. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Chapter 18 Life in the Universe 3
  • 4. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Evolution • The unifying concept of biology • Simple and general enough to work everywhere, so we’ll discuss it 4
  • 5. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley 5 3 The Fact of Evolution • Forms of life change over time, via descent with modification • Thatʼs it!
  • 6. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley 6 4 The Theory of Evolution • Characteristics of population are most strongly influenced by individuals who leave the most viable offspring Seems uncontroversial, even tautological! • Variation: mutation, sex, horizontal gene transfer, neutral drife, incorporation of cells • Selection: natural/sexual
  • 7. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley 7 14 Misconception: Evolution is Incompatible with Religion • Question 1a: if I accept evolution, must I be an atheist? • Question 1b: if we agree we are descended from animals, do we have no ethical guides?
  • 8. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley 8 15 Incompatible With Religion? • No! • Clergy letter project: >11,000 ministers signed in US alone • Affirms evidence for evolution; not at all in conflict with personal religious beliefs http://openparachute.files.wordpress.com/2008/02/charles-darwin.jpg http://www.clergyletterproject.net/clp140_100.gif
  • 9. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley 9 16 Must We Act Like Animals? • No, how silly! • Does gravity mean that you have to push people down stairs??? • Evolution is a description of what happened, not a guide • Ethics comes from other sources http://www.looptvandfilm.com/blog/homerevolution.jpg
  • 10. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Earliest Life Forms • Life probably arose on Earth around 3.8 billion years ago, after the end of heavy bombardment. • Evidence comes from fossils and carbon isotopes. 10
  • 11. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Fossils in Sedimentary Rock • relative ages: deeper layers formed earlier • absolute ages: radiometric dating 11
  • 12. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Chalk (a form of limestone) consist mainly of coccolith biomicrites formed from the skeletal elements of minute planktonic green algae, associated with varing proportions of larger microscopic fragments of bivalves, foraminifera and ostracods. White Cliffs of Dover 12
  • 13. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Fossils in Sedimentary Rock • Rock layers of the Grand Canyon record 2 billion years of Earth’s history. 13
  • 14. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Earliest Fossils • The oldest fossils show that bacteria- like organisms were present over 3.5 billion years ago. • Carbon isotope evidence pushes the origin of life to more than 3.85 billion years ago. Thrombolites in Lake Clifton, Western Australia. Also a less evolved organism at upper right 14
  • 15. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley The Geological Time Scale 15
  • 16. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Brief History of Life • 4.5 billion years — Earth forms • 4.4 billion years — early oceans form • 3.5 billion years — cyanobacteria start releasing oxygen • 2.0 billion years — oxygen begins building up in atmosphere • 540–500 million years — Cambrian Explosion • 225–65 million years — dinosaurs and small mammals (dinosaurs ruled) • Few million years — earliest hominids • < 10,000 years — Our civilization 16
  • 17. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Necessities for Life • Nutrient source • Energy (sunlight, chemical reactions, internal heat) • Liquid water (or possibly some other liquid) Hardest to find on other planets 17
  • 18. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Necessities for Life • Nutrient source • Energy (sunlight, chemical reactions, internal heat) • Liquid water (or possibly some other liquid) There is life everywhere on Earth where there is liquid water at least part of the time 18
  • 19. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley 19 36 Life Deep in Rock • Probably most of the biomass on Earth! • So far, record is almost three miles below the surface • Also found miles below seafloor • Live in rock cracks; can remain in stasis for many years (thousands? more?) until there is some water
  • 20. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley 20 37 Wild Speculation • Depth limited by heat Need liquid water • Mars is smaller, has cooled off faster • Probably much thicker part of crust that can harbor life • Might there now be more living biomass on Mars than on Earth? http://www.windows.ucar.edu/mars/images/mars1.gif
  • 21. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley 21 38 Undersea Thermal Vents • Near volcanic vents • Rich with minerals • Bacteria/archea use the nutrients • Other things eat them • Whole ecosystem! http://ocean-ridge.ldeo.columbia.edu/courses/subgeol/hot_springs/smokers.gif
  • 22. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Searches for Life on Mars • Mars had liquid water in the distant past. • Mars still has subsurface ice—possibly subsurface water near sources of volcanic heat. 22
  • 23. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Could there be life on Europa or other jovian moons? 23
  • 24. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Titan • Surface too cold for liquid water (but deep underground?) • Liquid ethane/methane on surface 24
  • 25. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Habitable zone 25
  • 26. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Habitable Planets Definition: A habitable world contains the basic necessities for life as we know it, including liquid water. • It does not necessarily have life. 26
  • 27. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Constraints on star systems: 1. Old enough to allow time for evolution (rules out high-mass stars — 1%) 2. Need to have stable orbits (might rule out binary/multiple star systems — 50%) 3. Size of “habitable zone”: region in which a planet of the right size could have liquid water on its surface Even so… billions of stars in the Milky Way seem at least to offer the possibility of habitable worlds. 27
  • 28. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley The Bottom Line We don’t yet know how important or negligible these concerns are. 28
  • 29. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Interstellar travel (?) 29
  • 30. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Current Spacecraft • Pioneers & Voyagers beyond Pluto now • These spacecraft travel at <1/10,000 c; 100,000 years to the nearest stars Pioneer plaque Voyager record 30
  • 31. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Difficulties of Interstellar Travel • Far more efficient engines are needed. • Energy requirements are enormous. • Ordinary interstellar particles become like cosmic rays. 31
  • 32. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Even at half light-speed... • Takes 9 years to reach the nearest star – more with acceleration & deceleration • Takes just as long to get back • There are 32 stars within 12 light-years • That’s about all that can be explored in a human lifetime – 24 years to grow & train – 24 to get there, 24 to get back – you’re 72 upon return 32
  • 33. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley SO... • The universe is BIG • and really, really OLD What are the chances that aliens are visiting us just now? (Consider what you’d find if you had visited Earth at any random moment in its history.) 33
  • 34. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley 34 14 The Burden of Proof • Suppose I claim to have seen an alien • Is it up to you to disprove me? • No! • Carl Sagan: “Extraordinary claims require extraordinary proof” • What does this mean in practice?
  • 35. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley 35 15 First Claim • Suppose I told you that yesterday I saw a friend walking down the street • Would you believe me? If not, what level of proof would you require?
  • 36. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley 36 16 Second Claim • Now suppose I told you that the other day I saw a 100-foot tall cyclops walking down the street • Would you believe me? If not, what level of proof would you require? http://bearah718.tripod.com/sitebuildercontent/sitebuilderpictures/cyclops.jpg
  • 37. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley 37 17 Importance of Discovery • Suppose visits by aliens were established beyond any question • This would be the most important discovery in history • As a result, we need to apply the highest standards of evidence to any alien claim Must be absolutely indisputable • ...and at this stage, no alien claim is even remotely indisputable
  • 38. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Alien life is likely • LOTS of stars • No reason to presume Earth is 100% unique Visits from aliens very unlikely • Distance between the stars is vast • Nothing special about right now • If aliens did make it to earth, they only have a one in a million chance of arriving while we’ve been around 38