1. Chapter 18 Life in the Universe

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!

4. What is Life? Non-linear chains of silicon & oxygen => inert gels or liquids OR => inert rigid rocks

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! Lysine – an amino acid

6. Common to all life on Earth? Chemically interacts with environment –Takes in nutrients selectively –Expels waste products chemically

7. Common to all life on Earth? Transforms food into energy for metabolic processes –Add cream of wheat to a rock?

9. Common to all life on Earth? Transforms food into energy for metabolic processes –Add cream of wheat to a rock? => No transformation!

10. Common to all life on Earth? Transforms food into energy for metabolic processes –Add cream of wheat to a person? –Transformation!

11. Common to all life on Earth? Reproduction!

12. Common to all life on Earth? DNA!

13. What is Life? Sequence of nucleo base-pairs tied together with sugar & phosphates? YES!!

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

15. Earliest Life Forms Life probably arose on Earth more than 3.85 billion years ago, shortly after the end of heavy bombardment.

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.

17. Fossils in Sedimentary Rock 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.

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

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.

29. Could there be life on Mars?

30. 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.

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 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? Most scientists are not yet convinced.

35. Could there be life on Europa or other jovian moons?

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?

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.

41. How many are possible?

42. 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…

43. But not every star is viable! 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 where a planet of the right size could support liquid water

44. Even so… billions of stars in the Milky Way seem at least to offer the possibility of habitable worlds.

45. The more massive the star, the larger the habitable zone—higher probability of a planet in this zone.

46. Spectral Signatures of Life Earth Venus Mars oxygen/ozone

47. Are Earth-like planets rare or common?

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 = N HP  f life  f civ  f now

55. The Drake Equation Number of civilizations with whom we could potentially communicate = N HP  f life  f civ  f now N HP = total number of habitable planets in galaxy

56. The Drake Equation Number of civilizations with whom we could potentially communicate = N HP  f life  f civ  f now N HP = total number of habitable planets in galaxy f life = fraction of habitable planets with life

57. The Drake Equation Number of civilizations with whom we could potentially communicate = N HP  f life  f civ  f now N HP = total number of habitable planets in galaxy f life = fraction of habitable planets with life f civ = fraction of life-bearing planets with civilization at some time

58. The Drake Equation Number of civilizations with whom we could potentially communicate = N HP  f life  f civ  f now N HP = total number of habitable planets in galaxy f life = fraction of habitable planets with life f civ = fraction of life-bearing planets with civilization at some time f now = fraction of civilizations around now

59. Drake Equation: Number of communicating civilizations in the Galaxy = N HP  f life  f civ  f now We do not know the following values: N HP : probably billions f life : ??? Hard to say (near 0 or near 1) f civ : ??? It took 4 billion years on Earth f now : ??? 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

61. How does SETI work?

62. 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!

64. Your computer can help! SETI @ 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 Pioneer plaqueVoyager record

67. Difficulties of Interstellar Travel 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?

70. Possible solutions to the paradox 1.We are alone: life/civilizations much rarer than we might have guessed Our own planet/civilization looks all the more precious…

71. 2.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. Possible solutions to the paradox

72. 3.There IS a galactic civilization… … and someday we’ll meet them. Possible solutions to the paradox