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SETI The search for extraterrestrial intelligence Dominated by quests for radio beacons, but with some searches for narrow-band laser transmissions.

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Presentation on theme: "SETI The search for extraterrestrial intelligence Dominated by quests for radio beacons, but with some searches for narrow-band laser transmissions."— Presentation transcript:

1 SETI The search for extraterrestrial intelligence Dominated by quests for radio beacons, but with some searches for narrow-band laser transmissions

2 Fig , p.423

3 Fig , p.428

4 Why SETI will Fail

5 High-resolution imaging of young planets New infrared results from the VLT and the HST

6 Essentials of planet imaging Young, preferably nearby, target stars A high spatial resolution infrared camera system on a large ground- based telescope or on the Hubble Space Telescope

7 Adaptive Optics Imaging At current state of the art, AO is sufficiently sensitive to detect only thermal emission from self-luminous, young planets. Reflected light is too feeble to be seen. AO detectability is a function of a planets age, distance from Earth, and contrast with its primary star.

8 Planet imaging programs Keck AO VLT AO HST/NICMOS To date, each telescope has been used to image ~100 stars

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12 Fig. 20-3a, p.418

13 Where do humans stand on the scale of cosmic intelligence? Carl Sagans natural evolution of the Universe: Origin of the Universe => origin of galaxies, stars, elements, planets => origin of life => chemical and biological evolution => technological intelligence

14 From the SETI Institute webpage (10/15/05), on The future of SETI research Scientists who participate in this research are more optimistic than ever before that they could find signals from space that would indicate that were not alone. They are bolstered in this view by several recent developments. In the past 5 years astronomers have found that many stars have planets…

15 Discoveries of extrasolar planets Exoplanets => ETI is *less* likely for two reasons: Minor reason: planetary systems are unfavorable for life as we know it (but only for ~10%) Primary reason: peoples great interest in these discoveries

16 We live in a unique moment in history: SETI, but no terrestrial planet finder (TPF)

17 AIRS spectrum

18 TPF/Darwin design concepts

19 These are first-generation instruments. Later generations could image Earth-size worlds revealing continent-ocean dichotomies, annual seasonal variations, the coming and going of ice ages, and long-term changes in vegetation patterns, both natural and human induced.

20 Suppose that TPF discovers a living world What happens next? SETI: For a decade? A century? A millennium?

21 If there is no answer, then our descendants can choose between two options: 1) do nothing (for a million years) 2) send a spaceship

22 Everything we know about human nature and history indicates that intelligent creatures will follow the latter path -- Exploration of our solar system began with telescopic observations from Earth. But as soon as we developed the capability, we launched spaceships to explore planets and moons up close because observing from afar is limited and, ultimately, unsatisfying.

23 Biologist Penelope Boston, from the Discovery Channels program Destination Mars: I am a biologist; I have a burning need to know about life in the Universe

24 But dinosaurs, bugs, and flowers dont do radio telescopes Passively pointing a radio telescope at a living world that lacks a technological civilization will never get Dr. Boston to where she wants to be -- e.g., knowledge of whether all life is carbon based or uses liquid water as a solvent, or is constructed from proteins and nucleic acids.

25 Robotic Interstellar Exploration in the 21 st Century 1998 NASA/JPL 2-day workshop Engineers & Scientists What hook might motivate humankind to provide the $$ needed to fund a mission to a nearby star?

26 Now lets turn the situation around and look at things from the perspective of a technological extraterrestrial. Earth, thanks to life, has had an oxygenic atmosphere for about 2 billion years. Any extraterrestrials who possess the equivalent of our TPF and who passed near our Sun during those years, would have discovered our unusual atmosphere.

27 In summary, three simple postulates have major implications for SETI. 1)Soon after development of technology, all civilizations will build the equivalent of TPF. 2)Intelligent life is curious about other life forms, simple or technological. 3) Having used TPF to discover a nearby living world, spaceships will be constructed to visit that world.

28 Extrasolar planets => ETI is now *less* likely than previously because of peoples great interest in such discoveries. (because of life)

29 If these simple postulates are true, then the absence of intelligent aliens in our solar system is strong evidence that they do not exist anywhere in our region of the Milky Way and SETI searches of nearby stars are destined to fail.

30 What is a planet? The IAU Definition: Mass < 13.6 Jupiter masses Orbits a star or stellar remnant Dont use formation mechanism to decide if yes or no

31 Science Camera Light from science target Telescope System Perfect Plane Wave Atmosphere corrugates the wavefront Creates blurred images Seeing disk ~ 1 arcsecond

32 Science Camera Light from science target Light from reference star Deformable Mirror Beam Splitter Computer Wavefront Sensor Creates partially sharpened images FWHM ~ arcsecond

33 Log 10 Age (years) 80M jup 14M jup JUPITER SATURN STARS (Hydrogen burning) BROWN DWARFS (Deuterium burning) PLANETS 200M jup Evolution of M Dwarf Stars, Brown Dwarfs and Giant Planets (from Adam Burrows) Log 10 L/L sum sun Cooling Curves for Substellar Objects NICMOS Companion Detection Limit (M type primary) 2M1207A 2M1207b

34 Epoch 5 astrometry - NICMOS Unequivocal common P.M.

35 Solar system time scales and ages of young nearby stars Formation of Jupiter< 10 Myr Formation of Earths core~ 30 Myr Era of heavy bombardment in inner solar system ~ 600 Myr Cha cluster8 Myr TW Hydrae Assoc.8 Myr Pictoris moving group 12 Myr Tucana/Horologium Assoc. 30 Myr AB Dor moving group 70 Myr

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37 2M1207A/b - 26 APR 05 NICMOS F160W (1.6 m) -2 to +2 ADU/second/pixel HST/NICMOS CAMERA 1 2nd FOLLOW-UP IMAGING


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