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  • Shows Index
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    Past Shows
    • Ep. 166: Multiverses
    • Ep. 165: Doppler Effect
    • Ep. 164: Inside the Atom
    • Ep. 163: Auroras
    • Ep. 162: Edwin Hubble
    • Ep. 161: Launch Facilities
    • Ep. 160: Eclipses
    • Ep. 159: Planet X
    • Ep. 158: Pulsars
    • Ep. 157: Constellations
    • Ep. 156: Famous Stars
    • Ep. 155: Dwarf Stars
    • Ep. 154: Dragon*Con Live with Seth Shostak
    • Ep. 153: Dark Skies
    • Ep. 152: Binary Stars
    • Ep. 151: Atmospheres
    • Ep. 150: Telescopes, the Next Level
    • Ep. 149: Constellation Program
    • Ep. 148: Astronomy and New Media
    • Ep. 147: How to Be Taken Seriously By Scientists
    • Ep. 146: Astronomy Research from Idea to Publication
    • Ep. 145: Interstellar Travel
    • Questions Show: Imaging Extrasolar Planets, Infinite Universe, Inside a Black Hole
    • Ep. 144: Space Elevators
    • Questions Show: Matter Balance, Jumping Light Speed and Black Hole Star Formation
    • Ep. 143: Astrobiology
    • Questions Show: Black black holes, Unbalancing the Earth, and Space Pollution
    • Ep. 142: Plate Tectonics
    • Questions Show: Avoiding the Heat Death, Orbiting Galaxies, and the Dangers of Space Radiation
    • Ep. 141: Volcanoes, Hot and Cold
    • Ep. 140: Entanglement
    • Questions Show: Galileoscope, Black Hole Time, and What Exactly is Energy?
    • Questions Show: Telescope Suggestions, Black Hole Energy, and Universal Time
    • Ep. 139: Energy Levels and Spectra
    • Questions: An Unlocked Moon, Energy Into Black Holes, and the Space Station's Orbit
    • Ep. 138: Quantum Mechanics
    • Questions Show: Hidden Fusion, the Speed of Neutrinos, and Hawking Radiation
    • Ep. 137: Large Scale Structure of the Universe
    • Questions Show: The Source of Atmospheres, the Vanishing Moon, and a Glow After Sunset
    • Ep. 136: Gamma Ray Astronomy
    • Questions Show: Dangerous Solar Flares, Higgs Boson Insights, and Light Speed Flashlights
    • Ep. 135: X-Ray Astronomy
    • Questions Show: NorthEast Astronomy Forum (NEAF)
    • Ep. 134: Ultraviolet Astronomy
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    • Questions Show: Undoing Inflation, Searching for Water, and Seeing Everything a Black Hole's Ever Eaten
    • Ep. 132: Infrared Astronomy
    • Episode 131: Submillimeter Astronomy
    • Questions Show: Decelerating Black Holes, Earth-Sun Tidal Lock, and the Crushing Gravity of Dark Matter
    • Episode 130: Radio Astronomy
    • Questions Show: Multiple Big Bangs, Satellite Collisions and the Size of the Universe
    • Ep. 129: Interferometry
    • Questions Show: Shooting Lasers at the Moon and Losing Contact with Rovers
    • Ep. 128: Dust
    • Ep. 127: The US Space Shuttle
    • Ep. 126 From Skeptics Guide with Questions
    • Ep. 125: A Zoo of Extrasolar Planets
    • Questions Show: Moons and the Drake Equation, Stars in the Void, and Rings Around Stars
    • Ep. 124: Space Capsules, Part 1 – Vostok, Mercury and Gemini
    • Ep. 123: Homogeneity
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    • Questions Show: Stellar Roche Limits, Seeing Black Holes, and Water on Mars
    • Ep. 121: Spacesuits
    • Ep. 120: The Christmas Star
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    • Ep. 119: Robots in Space
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    • Ep. 118: Sky Surveys
    • Ep. 117: Time
    • Ep. 116: Molecules in Space
    • Ep. 115: The Moon, Part 3: Return to the Moon
    • Questions Show: Spiral Arms, Seismic Waves on the Sun, and our Favorite Gear
    • Ep. 114: The Moon, Part 2 – Exploration of the Moon
    • Questions Show: Ice in Space, Expansion of the Universe, and Death from the Skies
    • Ep. 113: The Moon, Part 1
    • Questions Show: Orbit of the Planets, Green Stars, and Oort Cloud Contamination
    • Ep. 112: Death From the Skies, Interview with Phil Plait
    • Questions Show: Relativity, Relativity and More Relativity
    • Ep. 111: Nebulae
    • Questions Show: Galactic Dust, the Speed of Photons, and the Big Bang Calculations
    • Ep. 110: The Search for Extraterrestrial Intelligence
    • Questions Show: Alignment with the Galactic Plane, Destruction from Venus, and the Death of the Solar System
    • Ep. 109: The Life of Other Stars
    • Questions Show – Running Out of Gravitons and Hitting the Brakes at Light Speed
    • Ep. 108: The Life of the Sun
    • Questions Show – light speed, Andromeda galaxy, dark matter and black holes
    • Ep. 107: Nucleosynthesis: Elements from Stars
    • Questions Show – Black Hole Surfaces, Magnetic Field Strengths, and the Speed of Gravitons
    • Ep. 106: The Search for the Theory of Everything
    • Student Questions Show: Leelanau School
    • Ep. 105: The Strong and Weak Nuclear Forces
    • Ep 104: Science Fiction at Dragon*Con with Plait and Grazier
    • Ep. 103: Electromagnetism
    • Ep 102: Gravity
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    • Ep. 99: The Milky Way
    • Ep. 98: Quasars
    • Ep. 97: Galaxies
    • Ep. 96: Humans to Mars, Part 3 – Terraforming Mars
    • Student Questions: Collinsville High School
    • Ep. 95: Humans to Mars, Part 2 – Colonists
    • Ep 94: Humans to Mars, Part 1 – Scientists
    • Ep. 93: Missions to Mars, Part 2
    • Ep. 92: Missions to Mars, Part 1
    • Ep. 91: The Search for Water on Mars
    • Ep. 90: The Scientific Method
    • Ep. 89: Adaptive Optics
    • Ep. 88: The Hubble Space Telescope
    • Ep. 87: The End of the Universe Part 2: The End of Everything
    • Ep. 86: The End of the Universe Part 1: The End of the Solar System
    • Ep. 85: Detectors
    • Ep. 84: Getting Around the Solar System
    • Ep. 83: Wave Particle Duality
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    • Ep. 81: Questions on the Shape, Size and Centre of the Universe
    • Ep. 80: Craters
    • Ep. 79: How Big is the Universe?
    • Ep. 78: What is the Shape of the Universe?
    • Ep. 77: Where is the Centre of the Universe?
    • Ep. 76: Lagrange Points
    • Student Questions: Curtis High School
    • Ep. 75: Stellar Populations
    • Ep. 74: Antimatter
    • Ep. 73: Questions Show #8
    • Ep. 72: Cosmic Rays
    • Ep. 71: Gravitational Waves
    • Ep. 70: How To Win a Nobel Prize
    • Student Questions: Farmersburg
    • Ep. 69: The Large Hadron Collider and the Search for the Higgs-Boson
    • Ep. 68: Globular Clusters
    • Ep. 67: Building a Career in Astronomy
    • Ep. 66: How Amateurs Can Contribute to Astronomy
    • Ep. 65: The End of Our Tour Through the Solar System
    • Ep. 64: Pluto and the Icy Outer Solar System
    • Ep. 63: Neptune
    • Ep. 62: Uranus
    • Ep. 61: Saturn's Moons
    • Ep. 60: Questions Show #7
    • Ep. 59: Saturn
    • Ep. 58: Inflation
    • Ep. 57: Jupiter's Moons
    • Ep. 56: Jupiter
    • Ep. 55: The Asteroid Belt
    • Ep. 54: Questions Show #6
    • Ep. 53: Astronomy in Science Fiction
    • Special Episode: Panspermia
    • Ep. 52: Mars
    • Ep. 51: Earth
    • Ep. 50: Venus


Ep. 154: Dragon*Con Live with Seth Shostak

  • October 1st, 2009
  • Like it? Digg-it | Reddit | del.icio.us
Seth Shostak. Image credit: SETI.org

Seth Shostak. Image credit: SETI.org

This week we step away from our regular programming to bring you a live show from Dragon*Con in Atlanta. Pamela shares the stage with SETI researcher Seth Shostak. Together they discuss the technology and science of searching for intelligence, And answer questions from the audience.

Ep. 154: Dragon*Con Live with Seth Shostak

  • SETI
  • Dr. Shostak's bio
  • Arecibo Observatory, Puerto Rico
Pamela Gay and Seth Shostak at Dragon*Con. Photo courtesy Chuck Tomasi

Pamela Gay and Seth Shostak at Dragon*Con. Photo courtesy Chuck Tomasi

  • Magnetic Fields – GSU
  • SETI:  Sorting Intelligent Signals from Witless Cosmic Noise
  • Allen Telescope Array
  • "Bumps in the night" or transient phenomena:  the Rio Scale
  • Black Body Curve – Harvard
  • Infrared Excess — Internet Encyclopedia of Science
  • Dr. Frank Drake
  • NASA's involvement with SETI
  • Dr. John Billingham
  • Locations of SETI:
  1. SETI Institute
  2. Harvard
  3. UC Berkeley
  4. SETI in Italy
  • SETI@Home
  • Contact, the book by Carl Sagan
  • Contact, the movie
  • Academy of Astronautics SETI group
  • "Quiet Skies" for radio astronomy
  • 365 Days of Astronomy podcast about quiet skies by the NRAO (Oct. 11 — link will be added when episode airs)
  • Are We Sending a Bit Too Much Information into the Cosmos — Universe Today
  • XKCD comic about broadcasting to the aliens
  • "When Does SETI Throw in the Towel?" — written by Seth Shostak
  • Less Than 20 Years Until First Contact? — Universe Today

More pictures from Dragon*Con

Seth Shostak at Dragon*Con. Photo courtesy Chuck Tomasi

Seth Shostak at Dragon*Con. Photo courtesy Chuck Tomasi

Pamela facepalm. Photo courtesy Chuck Tomasi

Pamela facepalm. Photo courtesy Chuck Tomasi

Pamela and Chuck Tomasi.  Photo couresty Chuck Tomasi

Pamela and Chuck Tomasi. Photo couresty Chuck Tomasi




Comments
  1. Yiannis, Athens, Greece Says:
    October 2nd, 2009 at 5:22 pm

    One of your best episodes, in my opinion. I am sure we all agree that Mrs Pamela Gay was so good as a host here, as for Mr Seth Shostak, he gave all the answers I wanted to know about this subject since very long time. Congratulations and a big "Thank You" for offering your time to prepare this excellent show.

  2. Pink Zebra Comforter Says:
    October 2nd, 2009 at 7:51 pm

    Isn't it amazing what turn of events can take place? Appreciate you letting your readers know about this.

  3. christian_s Says:
    October 7th, 2009 at 5:55 am

    Excellent episode! Thanks again for doing this great podcast.
    Good sound quality too. (Teach your friends over at SGU a thing or two on that subject)

  4. Sayed Naveed Says:
    October 8th, 2009 at 5:12 pm

    Funny of that ceiling tile to drop serendipitously! I guess something IS terribly wrong with the way SETI's doing it all. Thanks a megawatt! Great episode. Nice to hear everyone chuckle and giggle and whisper in the background!

  5. Steven Athearn Says:
    October 9th, 2009 at 8:46 am

    There's obviously no hard data on which to base our estimates of the probability of success of SETI programs, but I'd like to note some perhaps realistic considerations that seem to be completely ignored in these discussions.

    Let's suppose the solar system is on the order of 4.5 billion years old. The oil and gas resources on which modern civilization (and modern science) are utterly dependent, were formed, on the standard account, during epochs of extreme global warming (with their accompanying algal blooms and die-offs) around 90 and 150 million years ago. Those resources will be extensively utilized only during a 150 or 200 year window, with something like 3/4 of that total occurring within a window of only 60 or 70 years. This may well be the approximate lifetime of an advanced industrial civilization, one with the capacity to produce powerful radar signals of the kind which radio astronomers on other worlds might perchance pick up during the lifetime – no more than an astronomical instant – of their own advanced civilization.

    Here I will merely state that I think the above scenario is not unrealistic – arguably, no combination of "alternatives" to fossil fuels (which are themselves generally highly fossil fuel dependent), is likely to provide useful energy on the same _scale_. Note also that the number of BTUs contained in principle in some yet-to-be-used-up energy resource – whether this be the quantity of sunlight hitting the earth, or of uranium in seawater, or of oil-in-place underground – is _never_ the relevant number. What is relevant is the _rates_ they can be extracted or produced, utilizing available technology and resources, _at an energy profit_.

    So in thinking about the probabilities of relatively long-lived industrial civilizations on other worlds, we might consider our own potential to have taken a different path. Say one that voluntarily self-imposed a global plateau of fossil fuel use in 1905, say, or even 1945. Doing so would have greatly extended the length of the fossil fuel window. Industrialization would have already reached the point that had begun (among other things) to provide the infrastructure for advanced experimental research. Perhaps society might have wisely concluded that it was not a good idea to become dependent on exhaustible resources, particularly for food production and distribution, and so explicitly adopted a list of legitimate uses of the resource (e.g. longer range storage and transportation of food for localized famine alleviation, not for customary use). This would have entailed, among other things, giving up fractional reserve banking and any other economic system requiring continued growth to avoid collapse (also measures to stop population growth). Perhaps the society could have chosen to support scientific research – with a practical view toward ultimately replacing fossil fuels at levels of use always below life-and-death dependence – or even in recognition of the value of scientific culture itself – including the fact that a cultural products (including scientific knowledge) can be much more widely distributed at a much lower cost in terms of sustainability than can the material products of our present civilization.

    How likely is such an outcome? Whether they are one-in-a hundred or one-in-a-million, I don't know. But those interested in SETI need to be thinking not only about the length of time it takes an advanced civilization to evolve, but also the likelihood that such such civilizations are very short-lived.

  6. Torbjörn Larsson, OM Says:
    October 25th, 2009 at 6:36 am

    "no combination of "alternatives" to fossil fuels (which are themselves generally highly fossil fuel dependent), is likely to provide useful energy on the same _scale_"

    That remains to be proven. AFAIU ilooks like they can, but at a higher cost.

    Other points not touched on in the analysis are the population size (which, in our case, is likely to start decreasing soon) and continuing efficiency improvements inherent in developing economies.

  7. Curtis Says:
    November 2nd, 2009 at 12:26 pm

    I was sitting next to the guy that the ceiling tile landed on. It hit his right shoulder; I was to the left. It just about startled me out of my skin. I'm glad the "H— S—!" I exclaimed didn't make it into the episode's audio! :D


       

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