Chapter 19: Life in the Universe

Chapter 1
How Science Works

  • The Scientific Method
  • Evidence
  • Measurements
  • Units and the Metric System
  • Measurement Errors
  • Estimation
  • Dimensions
  • Mass, Length, and Time
  • Observations and Uncertainty
  • Precision and Significant Figures
  • Errors and Statistics
  • Scientific Notation
  • Ways of Representing Data
  • Logic
  • Mathematics
  • Geometry
  • Algebra
  • Logarithms
  • Testing a Hypothesis
  • Case Study of Life on Mars
  • Theories
  • Systems of Knowledge
  • The Culture of Science
  • Computer Simulations
  • Modern Scientific Research
  • The Scope of Astronomy
  • Astronomy as a Science
  • A Scale Model of Space
  • A Scale Model of Time
  • Questions

Chapter 2
Early Astronomy

  • The Night Sky
  • Motions in the Sky
  • Navigation
  • Constellations and Seasons
  • Cause of the Seasons
  • The Magnitude System
  • Angular Size and Linear Size
  • Phases of the Moon
  • Eclipses
  • Auroras
  • Dividing Time
  • Solar and Lunar Calendars
  • History of Astronomy
  • Stonehenge
  • Ancient Observatories
  • Counting and Measurement
  • Astrology
  • Greek Astronomy
  • Aristotle and Geocentric Cosmology
  • Aristarchus and Heliocentric Cosmology
  • The Dark Ages
  • Arab Astronomy
  • Indian Astronomy
  • Chinese Astronomy
  • Mayan Astronomy
  • Questions

Chapter 3
The Copernican Revolution

  • Ptolemy and the Geocentric Model
  • The Renaissance
  • Copernicus and the Heliocentric Model
  • Tycho Brahe
  • Johannes Kepler
  • Elliptical Orbits
  • Kepler's Laws
  • Galileo Galilei
  • The Trial of Galileo
  • Isaac Newton
  • Newton's Law of Gravity
  • The Plurality of Worlds
  • The Birth of Modern Science
  • Layout of the Solar System
  • Scale of the Solar System
  • The Idea of Space Exploration
  • Orbits
  • History of Space Exploration
  • Moon Landings
  • International Space Station
  • Manned versus Robotic Missions
  • Commercial Space Flight
  • Future of Space Exploration
  • Living in Space
  • Moon, Mars, and Beyond
  • Societies in Space
  • Questions

Chapter 4
Matter and Energy in the Universe

  • Matter and Energy
  • Rutherford and Atomic Structure
  • Early Greek Physics
  • Dalton and Atoms
  • The Periodic Table
  • Structure of the Atom
  • Energy
  • Heat and Temperature
  • Potential and Kinetic Energy
  • Conservation of Energy
  • Velocity of Gas Particles
  • States of Matter
  • Thermodynamics
  • Entropy
  • Laws of Thermodynamics
  • Heat Transfer
  • Thermal Radiation
  • Wien's Law
  • Radiation from Planets and Stars
  • Internal Heat in Planets and Stars
  • Periodic Processes
  • Random Processes
  • Questions

Chapter 5
The Earth-Moon System

  • Earth and Moon
  • Early Estimates of Earth's Age
  • How the Earth Cooled
  • Ages Using Radioactivity
  • Radioactive Half-Life
  • Ages of the Earth and Moon
  • Geological Activity
  • Internal Structure of the Earth and Moon
  • Basic Rock Types
  • Layers of the Earth and Moon
  • Origin of Water on Earth
  • The Evolving Earth
  • Plate Tectonics
  • Volcanoes
  • Geological Processes
  • Impact Craters
  • The Geological Timescale
  • Mass Extinctions
  • Evolution and the Cosmic Environment
  • Earth's Atmosphere and Oceans
  • Weather Circulation
  • Environmental Change on Earth
  • The Earth-Moon System
  • Geological History of the Moon
  • Tidal Forces
  • Effects of Tidal Forces
  • Historical Studies of the Moon
  • Lunar Surface
  • Ice on the Moon
  • Origin of the Moon
  • Humans on the Moon
  • Questions

Chapter 6
The Terrestrial Planets

  • Studying Other Planets
  • The Planets
  • The Terrestrial Planets
  • Mercury
  • Mercury's Orbit
  • Mercury's Surface
  • Venus
  • Volcanism on Venus
  • Venus and the Greenhouse Effect
  • Tectonics on Venus
  • Exploring Venus
  • Mars in Myth and Legend
  • Early Studies of Mars
  • Mars Close-Up
  • Modern Views of Mars
  • Missions to Mars
  • Geology of Mars
  • Water on Mars
  • Polar Caps of Mars
  • Climate Change on Mars
  • Terraforming Mars
  • Life on Mars
  • The Moons of Mars
  • Martian Meteorites
  • Comparative Planetology
  • Incidence of Craters
  • Counting Craters
  • Counting Statistics
  • Internal Heat and Geological Activity
  • Magnetic Fields of the Terrestrial Planets
  • Mountains and Rifts
  • Radar Studies of Planetary Surfaces
  • Laser Ranging and Altimetry
  • Gravity and Atmospheres
  • Normal Atmospheric Composition
  • The Significance of Oxygen
  • Questions

Chapter 7
The Giant Planets and Their Moons

  • The Gas Giant Planets
  • Atmospheres of the Gas Giant Planets
  • Clouds and Weather on Gas Giant Planets
  • Internal Structure of the Gas Giant Planets
  • Thermal Radiation from Gas Giant Planets
  • Life on Gas Giant Planets?
  • Why Giant Planets are Giant
  • Gas Laws
  • Ring Systems of the Giant Planets
  • Structure Within Ring Systems
  • The Origin of Ring Particles
  • The Roche Limit
  • Resonance and Harmonics
  • Tidal Forces in the Solar System
  • Moons of Gas Giant Planets
  • Geology of Large Moons
  • The Voyager Missions
  • Jupiter
  • Jupiter's Galilean Moons
  • Jupiter's Ganymede
  • Jupiter's Europa
  • Jupiter's Callisto
  • Jupiter's Io
  • Volcanoes on Io
  • Saturn
  • Cassini Mission to Saturn
  • Saturn's Titan
  • Saturn's Enceladus
  • Discovery of Uranus and Neptune
  • Uranus
  • Uranus' Miranda
  • Neptune
  • Neptune's Triton
  • Pluto
  • The Discovery of Pluto
  • Pluto as a Dwarf Planet
  • Dwarf Planets
  • Questions

Chapter 8
Interplanetary Bodies

  • Interplanetary Bodies
  • Comets
  • Early Observations of Comets
  • Structure of the Comet Nucleus
  • Comet Chemistry
  • Oort Cloud and Kuiper Belt
  • Kuiper Belt
  • Comet Orbits
  • Life Story of Comets
  • The Largest Kuiper Belt Objects
  • Meteors and Meteor Showers
  • Gravitational Perturbations
  • Asteroids
  • Surveys for Earth Crossing Asteroids
  • Asteroid Shapes
  • Composition of Asteroids
  • Introduction to Meteorites
  • Origin of Meteorites
  • Types of Meteorites
  • The Tunguska Event
  • The Threat from Space
  • Probability and Impacts
  • Impact on Jupiter
  • Interplanetary Opportunity
  • Questions

Chapter 9
Planet Formation and Exoplanets

  • Formation of the Solar System
  • Early History of the Solar System
  • Conservation of Angular Momentum
  • Angular Momentum in a Collapsing Cloud
  • Helmholtz Contraction
  • Safronov and Planet Formation
  • Collapse of the Solar Nebula
  • Why the Solar System Collapsed
  • From Planetesimals to Planets
  • Accretion and Solar System Bodies
  • Differentiation
  • Planetary Magnetic Fields
  • The Origin of Satellites
  • Solar System Debris and Formation
  • Gradual Evolution and a Few Catastrophies
  • Chaos and Determinism
  • Extrasolar Planets
  • Discoveries of Exoplanets
  • Doppler Detection of Exoplanets
  • Transit Detection of Exoplanets
  • The Kepler Mission
  • Direct Detection of Exoplanets
  • Properties of Exoplanets
  • Implications of Exoplanet Surveys
  • Future Detection of Exoplanets
  • Questions

Chapter 10
Detecting Radiation from Space

  • Observing the Universe
  • Radiation and the Universe
  • The Nature of Light
  • The Electromagnetic Spectrum
  • Properties of Waves
  • Waves and Particles
  • How Radiation Travels
  • Properties of Electromagnetic Radiation
  • The Doppler Effect
  • Invisible Radiation
  • Thermal Spectra
  • The Quantum Theory
  • The Uncertainty Principle
  • Spectral Lines
  • Emission Lines and Bands
  • Absorption and Emission Spectra
  • Kirchoff's Laws
  • Astronomical Detection of Radiation
  • The Telescope
  • Optical Telescopes
  • Optical Detectors
  • Adaptive Optics
  • Image Processing
  • Digital Information
  • Radio Telescopes
  • Telescopes in Space
  • Hubble Space Telescope
  • Interferometry
  • Collecting Area and Resolution
  • Frontier Observatories
  • Questions

Chapter 11
Our Sun: The Nearest Star

  • The Sun
  • The Nearest Star
  • Properties of the Sun
  • Kelvin and the Sun's Age
  • The Sun's Composition
  • Energy From Atomic Nuclei
  • Mass-Energy Conversion
  • Examples of Mass-Energy Conversion
  • Energy From Nuclear Fission
  • Energy From Nuclear Fusion
  • Nuclear Reactions in the Sun
  • The Sun's Interior
  • Energy Flow in the Sun
  • Collisions and Opacity
  • Solar Neutrinos
  • Solar Oscillations
  • The Sun's Atmosphere
  • Solar Chromosphere and Corona
  • Sunspots
  • The Solar Cycle
  • The Solar Wind
  • Effects of the Sun on the Earth
  • Cosmic Energy Sources
  • Questions

Chapter 12
Properties of Stars

  • Stars
  • Star Names
  • Star Properties
  • The Distance to Stars
  • Apparent Brightness
  • Absolute Brightness
  • Measuring Star Distances
  • Stellar Parallax
  • Spectra of Stars
  • Spectral Classification
  • Temperature and Spectral Class
  • Stellar Composition
  • Stellar Motion
  • Stellar Luminosity
  • The Size of Stars
  • Stefan-Boltzmann Law
  • Stellar Mass
  • Hydrostatic Equilibrium
  • Stellar Classification
  • The Hertzsprung-Russell Diagram
  • Volume and Brightness Selected Samples
  • Stars of Different Sizes
  • Understanding the Main Sequence
  • Stellar Structure
  • Stellar Evolution
  • Questions

Chapter 13
Star Birth and Death

  • Star Birth and Death
  • Understanding Star Birth and Death
  • Cosmic Abundance of Elements
  • Star Formation
  • Molecular Clouds
  • Young Stars
  • T Tauri Stars
  • Mass Limits for Stars
  • Brown Dwarfs
  • Young Star Clusters
  • Cauldron of the Elements
  • Main Sequence Stars
  • Nuclear Reactions in Main Sequence Stars
  • Main Sequence Lifetimes
  • Evolved Stars
  • Cycles of Star Life and Death
  • The Creation of Heavy Elements
  • Red Giants
  • Horizontal Branch and Asymptotic Giant Branch Stars
  • Variable Stars
  • Magnetic Stars
  • Stellar Mass Loss
  • White Dwarfs
  • Supernovae
  • Seeing the Death of a Star
  • Supernova 1987A
  • Neutron Stars and Pulsars
  • Special Theory of Relativity
  • General Theory of Relativity
  • Black Holes
  • Properties of Black Holes
  • Questions

Chapter 14
The Milky Way

  • The Distribution of Stars in Space
  • Stellar Companions
  • Binary Star Systems
  • Binary and Multiple Stars
  • Mass Transfer in Binaries
  • Binaries and Stellar Mass
  • Nova and Supernova
  • Exotic Binary Systems
  • Gamma Ray Bursts
  • How Multiple Stars Form
  • Environments of Stars
  • The Interstellar Medium
  • Effects of Interstellar Material on Starlight
  • Structure of the Interstellar Medium
  • Dust Extinction and Reddening
  • Groups of Stars
  • Open Star Clusters
  • Globular Star Clusters
  • Distances to Groups of Stars
  • Ages of Groups of Stars
  • Layout of the Milky Way
  • William Herschel
  • Isotropy and Anisotropy
  • Mapping the Milky Way
  • Questions

Chapter 15
Galaxies

  • The Milky Way Galaxy
  • Mapping the Galaxy Disk
  • Spiral Structure in Galaxies
  • Mass of the Milky Way
  • Dark Matter in the Milky Way
  • Galaxy Mass
  • The Galactic Center
  • Black Hole in the Galactic Center
  • Stellar Populations
  • Formation of the Milky Way
  • Galaxies
  • The Shapley-Curtis Debate
  • Edwin Hubble
  • Distances to Galaxies
  • Classifying Galaxies
  • Spiral Galaxies
  • Elliptical Galaxies
  • Lenticular Galaxies
  • Dwarf and Irregular Galaxies
  • Overview of Galaxy Structures
  • The Local Group
  • Light Travel Time
  • Galaxy Size and Luminosity
  • Mass to Light Ratios
  • Dark Matter in Galaxies
  • Gravity of Many Bodies
  • Galaxy Evolution
  • Galaxy Interactions
  • Galaxy Formation
  • Questions

Chapter 16
The Expanding Universe

  • Galaxy Redshifts
  • The Expanding Universe
  • Cosmological Redshifts
  • The Hubble Relation
  • Relating Redshift and Distance
  • Galaxy Distance Indicators
  • Size and Age of the Universe
  • The Hubble Constant
  • Large Scale Structure
  • Galaxy Clustering
  • Clusters of Galaxies
  • Overview of Large Scale Structure
  • Dark Matter on the Largest Scales
  • The Most Distant Galaxies
  • Black Holes in Nearby Galaxies
  • Active Galaxies
  • Radio Galaxies
  • The Discovery of Quasars
  • Quasars
  • Types of Gravitational Lensing
  • Properties of Quasars
  • The Quasar Power Source
  • Quasars as Probes of the Universe
  • Star Formation History of the Universe
  • Expansion History of the Universe
  • Questions

Chapter 17
Cosmology

  • Cosmology
  • Early Cosmologies
  • Relativity and Cosmology
  • The Big Bang Model
  • The Cosmological Principle
  • Universal Expansion
  • Cosmic Nucleosynthesis
  • Cosmic Microwave Background Radiation
  • Discovery of the Microwave Background Radiation
  • Measuring Space Curvature
  • Cosmic Evolution
  • Evolution of Structure
  • Mean Cosmic Density
  • Critical Density
  • Dark Matter and Dark Energy
  • Age of the Universe
  • Precision Cosmology
  • The Future of the Contents of the Universe
  • Fate of the Universe
  • Alternatives to the Big Bang Model
  • Space-Time
  • Particles and Radiation
  • The Very Early Universe
  • Mass and Energy in the Early Universe
  • Matter and Antimatter
  • The Forces of Nature
  • Fine-Tuning in Cosmology
  • The Anthropic Principle in Cosmology
  • String Theory and Cosmology
  • The Multiverse
  • The Limits of Knowledge
  • Questions

Chapter 18
Life On Earth

  • Nature of Life
  • Chemistry of Life
  • Molecules of Life
  • The Origin of Life on Earth
  • Origin of Complex Molecules
  • Miller-Urey Experiment
  • Pre-RNA World
  • RNA World
  • From Molecules to Cells
  • Metabolism
  • Anaerobes
  • Extremophiles
  • Thermophiles
  • Psychrophiles
  • Xerophiles
  • Halophiles
  • Barophiles
  • Acidophiles
  • Alkaliphiles
  • Radiation Resistant Biology
  • Importance of Water for Life
  • Hydrothermal Systems
  • Silicon Versus Carbon
  • DNA and Heredity
  • Life as Digital Information
  • Synthetic Biology
  • Life in a Computer
  • Natural Selection
  • Tree Of Life
  • Evolution and Intelligence
  • Culture and Technology
  • The Gaia Hypothesis
  • Life and the Cosmic Environment

Chapter 19
Life in the Universe

  • Life in the Universe
  • Astrobiology
  • Life Beyond Earth
  • Sites for Life
  • Complex Molecules in Space
  • Life in the Solar System
  • Lowell and Canals on Mars
  • Implications of Life on Mars
  • Extreme Environments in the Solar System
  • Rare Earth Hypothesis
  • Are We Alone?
  • Unidentified Flying Objects or UFOs
  • The Search for Extraterrestrial Intelligence
  • The Drake Equation
  • The History of SETI
  • Recent SETI Projects
  • Recognizing a Message
  • The Best Way to Communicate
  • The Fermi Question
  • The Anthropic Principle
  • Where Are They?

Are We Alone?



Buckminster Fuller, 1972-3 tour at UC Santa Barbara.

One of the most intriguing questions in astronomy is whether or not the Earth alone harbors intelligent life. Either extraterrestrial life exists or it does not. Both possibilities have striking consequences. As American architect and designer Buckminster Fuller (1895-1983) said, "Sometimes I think we're alone. Sometimes I think we're not. In either case, the thought is staggering." The universe is a large and bountiful place. There are an enormous number of potential sites for life, and the chemical constituents of life are distributed widely across space. At first sight, it appears unlikely that we should be alone. If intelligent life exists beyond the solar system, our world might well be influenced by it, for better or worse. At the very least, as anthropologist D.K. Stern has pointed out, the discovery of alien life "would irreversibly destroy our self-image as the pinnacle of creation." The alternative is equally profound. If we are the only intelligent creatures in the universe, it would imply a universe of incredible grandeur with us as the only, and quite temporary, spectators.


Enrico Fermi, Italian-American physicist, received the 1938 Nobel Prize in physics for identifying new elements and discovering nuclear reactions by his method of nuclear irradiation and bombardment

In the 1940s, the physicist Enrico Fermi took a back-of-the-envelope approach to this problem. He was heavily persuaded by the argument that the vast number of stars in the universe must imply that some of them must host planets with intelligent life. This line of reasoning led Fermi to ask the question "Where are they?" He estimated an advanced society could populate the entire Milky Way in just 5 to 50 million years. If there is intelligent life out there, why have we not been contacted? He considered how radio astronomers have listened for radio messages and heard none and how our skies are not filled with alien visitors observing us or trying to contact us. Looking around, all he saw was a lack of evidence for aliens in a galaxy that potentially could be as fully colonized as the land masses of our own planet Earth. Even looking at history, there is no concrete evidence of "ancient astronauts" or alien visitations in earlier Earth history.


An artist's concept of a possible Moon colony. Just a few kilometers from the Apollo 17 Taurus Littrow landing site, a lunar mining facility harvests oxygen from the resource-rich volcanic soil of the eastern Mare Serenitatis. Here a marketing executive describes the high iron, aluminum, magnesium, and titanium content in the processed tailings, which could be used as raw material for a lunar metals production plant. This image produced for NASA by Pat Rawlings, (SAIC). Technical concepts for NASA's Exploration Office, Johnson Space Center (JSC).

Fermi and others have postulated that an advanced race could colonize the Milky Way on a timescale that is short compared to the age of the galaxy. Such a civilization could feasibly even explore the galaxy without biological colonization by sending unmanned (unaliened?) spacecraft to other planetary systems. These probes could then use local materials to replicate themselves and they could rapidly propagate through the galaxy, carrying out technological colonization while sending information back at light speed to the originators. If this sounds far-fetched, remember that such a scenario requires only a modest extrapolation of our current technology; we are probably less than 100 years from robots that can construct other robots and propulsion systems that can accelerate a small payload to a tenth the speed of light in space. Already, the Japanese are looking to build a fully robotic base on the Moon.

There are several logical answers to Fermi's "Where are they?" question. One possibility is that there simply isn't intelligent life out there; intelligent life is a unique consequence of random events in the universe. Alternatively, the universe could be heavily populated, but very sparsely so the nearest civilizations are in distant galaxies. Their radio messages would be millions of years old by the time they reached Earth. Spaceships would be unlikely to reach Earth if limited to speeds less than that of light, as current physics demands. It is entirely consistent with our current knowledge to propose that simple microbial life is quite common in the universe, but that intelligence and technology are extremely rare.

It is also possible that space exploration and the desire for communication are uniquely human characteristics. After all, it can be argued that there are more than one intelligent species on our planet but that the technology and desire to explore and communicate are unique to humans. Technology is not even universal among human societies. Are humans fated to be explorers, bridge-builders, and scientists rather than artists, athletes, or daydreamers? Is the stereotyped aggressive Westerner more representative of the essence of humanity than the stereotyped contemplative Easterner? Our technocracy may be just one type of cultural activity rather than a natural consequence of biological evolution. Historically, patterns we once assumed to be results of our biology have turned out to be consequences of cultural influences (confusion between these two has led to racist and sexist biases that we are still trying to overcome). We have all been influenced by the appealing image from science fiction of space exploration and communication as a universal cultural activity. In fact, it is absurdly anthropocentric to suppose that beings on other planets would resemble us physically, psychologically, or socially.


Three types of fossil microbes in the Archaean

A diagram of a typical prokaryotic cell.

Possibly the most significant answer to the question "where are they?" is that we may be separated from aliens more by evolutionary time than by actual physical space. Let us conduct a hypothetical experiment. Imagine a planetary twin of Earth that started evolving at exactly the same time. Even if life on both planets chose similar biochemical pathways, organisms on the two planets are likely to be out of evolutionary phase with one another. Just a slight difference in temperature between the planets could cause the evolutionary "clocks" on the two planets to be out of sync. If even 1 percent out of sync, life on our twin would be 40 million years behind or ahead of us. This is as far from us evolutionarily as we are from early mammals. If the clocks differ by 10% to 15%, then we are talking about the enormous evolutionary difference between single-celled microorganisms and ourselves! The timing argument carries one important consequence. We have had the capability for interstellar communication for only 50 years, which is a mere instant in evolutionary and cosmic time. Due to the time it takes signals to travel through interstellar space, it is likely that any civilization with which we could make contact will be far more advanced than us, by thousands or perhaps millions of years. Even if we were at the same evolutionary stage as our twin, the large distances coupled with the anticipated lifetime of civilizations (the oldest civilizations on Earth have lasted only thousands of years) make the idea of communication futile.

These aren't answers that satisfy everyone. Polls in the


A poll on how many people believe that aliens exist.
United States show that the public has an enormous susceptibility to the idea of alien visitation. Even without convincing evidence, over 50 percent of the population believes that we have already made contact. This isn't so surprising given that aliens have been in the popular culture for over 100 years, beginning with the influential H.G. Wells book War of the Worlds, and progressing to more recent phenomena like the TV shows X-Files V, and the entire Stargate franchise and movies like Men in Black. Long a staple of science fiction, alien life forms took a big step into the public consciousness through the powerful media of TV and film. As an example, consider the rise in popularity of the TV show Star Trek and the Star Wars movie series from small cults to the level of widespread cultural phenomena.

Popular culture paints two opposing versions of the alien myth. The first is the optimistic view, expressed by movies such as E.T., Close Encounters of the Third Kind, and more recently Contact. This view demonstrates our desire for knowledge, camaraderie in a vast universe, and even salvation. Second is the pessimistic view, seen in movies such as Alien and Independence Day, which places us in jeopardy in a universe of superior life forms. That the latter is more likely the truth has been a concern of scientists as eminent as Stephen Hawking.


An artist's conception of the NASA Spitzer Space Telescope.

Despite our fears, we do continue to look. The search for alien life is a new scientific adventure in the making. Astronomers continue to study the possibilities of life beyond the Earth as a direct way of questioning our role in the universe. Admittedly, discussions of the existence, intelligence, psychology, or appearance of higher alien life forms are almost highly speculative. But an interdisciplinary group of researchers has begun to take these issues very seriously. Astronomers have detected planets in orbit around nearby stars, and modern observatories like Spitzer can actually measure the chemical composition of some of these planets' atmospheres. While we haven't yet discovered any habitable worlds, they have also found complex, carbon-based molecules in interstellar space and in meteorites. This confirms that complex chemistry is active beyond our own solar system. Chemists have studied the pathways by which replicating molecules and simple life forms can be synthesized from simple constituents. Evolutionary biologists have considered how life might evolve in complexity starting with single-celled organisms. Physicists have even calculated the rates at which interstellar cultures might populate the galaxy. Together, all these scientists have worked to predict what atmospheric clues life might create. It just may be that intelligent life is found first by how it pollutes chemically rather than how it transmits radio signals!

All this work feels like progress, but it still doesn't answer "Where are they?"


Freeman Dyson at Harvard University in 2004

Optimists in the search for extraterrestrial intelligence have one additional, hopeful, answer for the bleak scenario that intelligent life is rare in the galaxy. Rather than use signals for communication from point to point, alien civilizations might use signals to store information in a vast, cosmic internet. If one civilization succeeded in sending probes across the galaxy, they could use these probes to set up a communication network across the galaxy. These artificial stations could beam information at planets, collect information from planets with intelligent life forms, and store the information in a growing database. Each newly intelligent civilization would not have to wait thousands of years of light travel time to communicate across the galaxy; they would only have to wait the much shorter time to tap into the nearest node of the network. The information in this cosmic internet would survive the death of any civilization and act as a kind of galactic consciousness.

All of these are hypothetical ideas, but we should recall the words of physicist Freeman Dyson: "Nature always has more imagination than us." We are a young intelligent species, peering into the vastness of our cosmic environment with the naivety of a newborn. We may be surprised at what we find.


Author: Chris Impey
Editor/Contributor: Pamela Gay
Editor/Contributor: Erika Offerdahl