1. Life in the Universe… and how to find it!

2. Life on Earth What is “Life?” Life on Earth When did life arise?
How did life arise?
Life in our Solar System?
Is there Intelligent life in Space – that we can find?

3. What is Life? Atoms, Molecules – no
Random linear chains of Molecules – no
Random non-linear chains – no!
Applies to “life as we know it.”

4. What is Life?
Non-linear chains of silicon & oxygen => inert gels or liquids OR => inert rigid rocks
Applies to “life as we know it.”

5. What is Life?
Complex non-linear chains of carbon – no, but getting closer!
Complex non-linear chains of carbon, hydrogen, nitrogen, & oxygen – no, but getting closer still!
Applies to “life as we know it.”
Lysine – an amino acid

6. Common to all life on Earth?
Chemically interacts with environment
Takes in nutrients selectively
Expels waste products chemically
Applies to “life as we know it.”

7. Common to all life on Earth?
Transforms food into energy for metabolic processes
Add cream of wheat to a rock?
Applies to “life as we know it.”

8. Applies to “life as we know it.”

9. Common to all life on Earth?
Transforms food into energy for metabolic processes
Add cream of wheat to a rock?
=> No transformation!
Applies to “life as we know it.”

10. Common to all life on Earth?
Transforms food into energy for metabolic processes
Add cream of wheat to a person?
Transformation!
Applies to “life as we know it.”

11. Common to all life on Earth?
Reproduction!
Applies to “life as we know it.”

12. Common to all life on Earth?
DNA!
Applies to “life as we know it.”

13. What is Life?
Sequence of nucleo base-pairs tied together with sugar & phosphates? YES!!
Applies to “life as we know it.”

14. Necessities for Life Nutrient source
Energy (sunlight, chemical reactions, internal heat)
Liquid water (or possibly some other liquid)
Hardest to find on other planets
Applies to “life as we know it.”

15. Earliest Life Forms
Life probably arose on Earth more than 3.85 billion years ago, shortly after the end of heavy bombardment.
Grand Canyon layers record 2 billion years of Earth’s history.

16. Earliest Life Forms
Life probably arose on Earth more than 3.85 billion years ago, shortly after the end of heavy bombardment.
Evidence comes from fossils and carbon isotopes.
Grand Canyon layers record 2 billion years of Earth’s history.

17. Fossils in Sedimentary Rock
Discuss formation of sedimentary layers so students can see how fossils are related through time.
Rock layers of the Grand Canyon record more than 500 million years of Earth’s history.

18. 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.

19. How did life arise on Earth?

20. When did life arise on Earth?

21. Origin of Life on Earth Life evolves through time.
All life on Earth shares a common ancestry.
We may never know exactly how the first organism arose, but laboratory experiments suggest plausible scenarios.
DNA = Deoxyribonucleic acid. Most instructors won’t insist their students learn this term.

22. The Theory of Evolution
Fossil record shows evolution occurred through time.
Darwin’s theory tells HOW evolution occurs: through natural selection.
Theory supported by discovery of DNA: evolution proceeds through mutations.

23. Tree of Life
Mapping genetic relationships has led biologists to discover this new “tree of life”.
Plants and animals are a small part of the tree.
Suggests likely characteristics of common ancestor.

24. Genetic studies suggest earliest life on Earth may have resembled bacteria
Today found near deep ocean volcanic vents (black smokers)
Geothermal hot springs.

25. Laboratory Experiments
Miller–Urey experiment show building blocks of life form easily and spontaneously under conditions of early Earth.

26. Microscopic, enclosed membranes or “pre-cells” have been created in the lab.

27. Origin of Oxygen
Cyanobacteria paved the way for more complicated life-forms
Release oxygen into atmosphere via photosynthesis.

28. Could life have migrated to Earth?
Venus, Earth, and Mars have “exchanged” tons of rock (blasted into orbit by impacts).
Meteorites & Comets are known to carry organic materials.
Some microbes can survive years in space.
A picture of the famous Murchison meteorite (many amino acids) can be found at

29. Could there be life on Mars?

30. Searches for Life on Mars
This photo shows a panorama taken by Opportunity. Spend a couple minutes reviewing why Mars is a promising place for life: evidence of past water, evidence for subsurface ice today… You might wish to repeat some slides from Ch. 7 on Mars to show the evidence for past water from orbit.
Mars had liquid water in the distant past.
Mars still has subsurface ice—possibly subsurface water near sources of volcanic heat.

31. In 2004, NASA’s Spirit and Opportunity rovers sent home new mineral evidence of past liquid water on Mars.

32. In 2012 and 2013, NASA’s Mars Science Lab explorer confirmed mineral evidence of past liquid water!

33. The Martian Meteorite Debate
Composition indicates origin on Mars
If you wish to discuss the martian meteorite debate, it’s good to start with a brief history of the meteorite as reconstructed from its geology and dating of various components.
1984: meteorite ALH84001 found in Antarctica
13,000 years ago: fell to Earth in Antarctica
16 million years ago: blasted from surface of Mars
4.5 billion years ago: rock formed on Mars

34. Does the meteorite contain actual fossil evidence of life on Mars?
These microscopic photos show structures with a fossil-like appearance, but they may also have been formed by nonbiological processes. Bottom line: the meteorite is intriguing, but certainly not definitive. We’ll need much more evidence to conclude that life ever existed on Mars.
Depending on level of coverage, you might wish to go into the pro and con debate in greater detail, as discussed in the text on p. 512.
Most scientists are not yet convinced.

35. Could there be life on Europa or other jovian moons?
Review evidence for liquid water ocean on Europa, in which case there might be undersea volcanoes. Artists conception of volcanic eruption temporarily disrupting surface ice.

36. Ganymede, Callisto also show some evidence for subsurface oceans
Relatively little energy available for life, but still…
Intriguing prospect of THREE potential homes for life around Jupiter alone
Ganymede
Callisto

37. Saturn’s Moon Titan
Surface too cold for liquid water (but deep underground?)
Liquid ethane/methane on surface

38. Saturn’s Moon Enceladus
Ice fountains suggest that it might have liquid water below the surface

39. Are habitable planets likely?
Be sure students understand that “habitable” refers to a potential for life, not actually for life itself. And emphasize that while we may soon be able to search for worlds with habitable surfaces around other stars, we will NOT soon be able to look for worlds like Europa—even though these may well be more common.

40. 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.
Be sure students understand that “habitable” refers to a potential for life, not actually for life itself. And emphasize that while we may soon be able to search for worlds with habitable surfaces around other stars, we will NOT soon be able to look for worlds like Europa—even though these may well be more common.

41. How many are possible?
Be sure students understand that “habitable” refers to a potential for life, not actually for life itself. And emphasize that while we may soon be able to search for worlds with habitable surfaces around other stars, we will NOT soon be able to look for worlds like Europa—even though these may well be more common.

42. How many are possible? If each star was a grain of sand…
There are more stars in our galaxy than grains of sand on a beach…
AND, as many galaxies in the universe as grains of sand on a beach…
Be sure students understand that “habitable” refers to a potential for life, not actually for life itself. And emphasize that while we may soon be able to search for worlds with habitable surfaces around other stars, we will NOT soon be able to look for worlds like Europa—even though these may well be more common.

43. But not every star is viable!
Constraints on star systems:
Old enough to allow time for evolution (rules out high-mass stars ~1%)
Need to have stable orbits (might rule out binary/multiple star systems ~50%)
Size of habitable zone: region where a planet of the right size could support liquid water
Be sure students understand that “habitable” refers to a potential for life, not actually for life itself. And emphasize that while we may soon be able to search for worlds with habitable surfaces around other stars, we will NOT soon be able to look for worlds like Europa—even though these may well be more common.

44. First question in the search for habitable worlds is how many stars could be homes to life…
Even so… billions of stars in the Milky Way seem at least to offer the possibility of habitable worlds.

45. Even if we focus only on G-type stars like our Sun, there are billions in the Milky Way Galaxy alone. And we can’t rule out habitable worlds around smaller stars. (But much more massive stars have lifetimes too short for evolution.)
The more massive the star, the larger the habitable zone—higher probability of a planet in this zone.

46. Spectral Signatures of Life
Venus
oxygen/ozone
Earth
Can discuss how we might determine whether life exists on a distant world.
Mars

47. Are Earth-like planets rare or common?
The text goes into a fair amount of detail on the rare Earth hypothesis, primarily because it has been in the news so much over the past few years. You may or may not want to go into the same level of detail in class.

48. Elements and Habitability
Some argue that proportions of heavy elements need to be just right for formation of habitable planets.
If so, Earth-like planets are restricted to a habitable zone in the galaxy…

49. Impacts and Habitability
Some argue that Jupiter-like planets are necessary to reduce the rate of impacts.
If so, then Earth-like planets are restricted to star systems with Jupiter-like planets.

50. Climate and Habitability
Some argue that plate tectonics and/or a large moon are necessary to keep the climate of an Earth-like planet stable enough for life.

51. The Bottom Line
We don’t yet know how important or negligible these concerns are.

52. What have we learned? Are habitable planets likely?
Billions of stars have sizable habitable zones, but we don’t yet know how many have terrestrial planets in those zones.
Are Earth-like planets rare or common?
We don’t yet know because we are still trying to understand all the factors that make Earth suitable for life.

53. How many civilizations are out there?

54. The Drake Equation
Number of civilizations with whom we could potentially communicate = NHP  flife  fciv  fnow
It’s usually worth going through this equation slowly so that students can see how it leads to the number of civilizations that we could communicate with.

55. The Drake Equation
Number of civilizations with whom we could potentially communicate = NHP  flife  fciv  fnow
NHP = total number of habitable planets in galaxy
It’s usually worth going through this equation slowly so that students can see how it leads to the number of civilizations that we could communicate with.

56. The Drake Equation
Number of civilizations with whom we could potentially communicate = NHP  flife  fciv  fnow
NHP = total number of habitable planets in galaxy
flife = fraction of habitable planets with life
It’s usually worth going through this equation slowly so that students can see how it leads to the number of civilizations that we could communicate with.

57. The Drake Equation
Number of civilizations with whom we could potentially communicate = NHP  flife  fciv  fnow
NHP = total number of habitable planets in galaxy
flife = fraction of habitable planets with life
fciv = fraction of life-bearing planets with civilization at some time
It’s usually worth going through this equation slowly so that students can see how it leads to the number of civilizations that we could communicate with.

58. The Drake Equation
Number of civilizations with whom we could potentially communicate = NHP  flife  fciv  fnow
NHP = total number of habitable planets in galaxy
flife = fraction of habitable planets with life
fciv = fraction of life-bearing planets with civilization at some time
fnow = fraction of civilizations around now
It’s usually worth going through this equation slowly so that students can see how it leads to the number of civilizations that we could communicate with.

59. Drake Equation: Number of communicating civilizations in the Galaxy = NHP  flife  fciv  fnow We do not know the following values:
NHP : probably billions
flife : ??? Hard to say (near 0 or near 1)
fciv : ??? It took 4 billion years on Earth
fnow : ??? Can civilizations survive long-term?

60. Are we “off-the-chart” smart?
Humans have comparatively large brains.
Does that mean our level of intelligence is improbably high?
Insert ECP6 Figure 18.18
One interesting question on Fciv is whether it is likely or unlikely that a planet with life would ever get a species as smart as US. This is a fun slide to show, since it can be used to argue the question both ways. On the one hand, we have much larger brains in proportion to body mass than any other species that has ever lived on Earth. On the other hand, while we are a statistical outlier, statistically some outliers are to be expected…

61. How does SETI work?

62. SETI experiments look for deliberate signals from E.T.
Emphasize that current SETI efforts could not detect signals as weak as our own radio/TV broadcasts. For now, at least, we are looking for deliberately broadcast signals..
SETI experiments look for deliberate signals from E.T.

63. We’ve even sent a few signals ourselves…
Earth to globular cluster M13: Hoping we’ll hear back in about 42,000 years!
Message sent from Arecibo in 1974… M13 distance approx. 21,000 light-years—but offers a lot of potential targets with its high density of stars.

64. Your computer can help! SETI @ Home: a screensaver with a purpose
Optional: There’s a lot of data to sift though, and you can be a part of the effort… .
Your computer can help! Home: a screensaver with a purpose

65. How difficult is interstellar travel?

66. Current Spacecraft
Current spacecraft travel at <1/10,000c; 100,000 years to the nearest stars
Our first interstellar emissaries: the Pioneer and Voyager spacecraft.
Pioneer plaque
Voyager record

67. Difficulties of Interstellar Travel
If you discuss the difficulty of interstellar travel in any detail, you might wish to discuss the implications to UFOs; see box on p. 523.
Far more efficient engines are needed.
Energy requirements are enormous.
Ordinary interstellar particles become like cosmic rays.
There are social complications of time dilation.

68. Where are the aliens?

69. Fermi’s Paradox
Plausible arguments suggest that civilizations should be common. For example, even if only 1 in 1 million stars gets a civilization at some time  100,000 civilizations!
So why haven’t we detected them?
This is one of our favorite topics, and if you have time it is worth using these slides as a capstone to your course…

70. Possible solutions to the paradox
We are alone: life/civilizations much rarer than we might have guessed
Our own planet/civilization looks all the more precious…

71. Possible solutions to the paradox
Civilizations are common, but interstellar travel is not, perhaps because:
interstellar travel is more difficult than we think.
the desire to explore is rare.
civilizations destroy themselves before achieving interstellar travel.
These are all possibilities, but they are not very appealing.

72. Possible solutions to the paradox
There IS a galactic civilization…
… and someday we’ll meet them.
A truly incredible possibility to ponder…