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

Slides:



Advertisements
Similar presentations
THESIS – the Terrestrial and Habitable-zone Exoplanet Spectroscopy Infrared Spacecraft a concept for a joint NASA/ESA exoplanet characterization mission.
Advertisements

Space Facts Section B – The Planets.
© 2005 Pearson Education Inc., publishing as Addison-Wesley Extrasolar Planets Since our Sun has a family of planets, shouldnt other stars have them as.
The Traveling Exhibit Science Background Part D: Search for Life prepared by Dr. Cherilynn Morrow for the Space Science Institute Boulder, CO.
Is there life on other planets?
Speaker: Laird Close University of Arizona ADAPTIVE OPTICS IN ASTRONOMY THE PROBLEM: Since Newton’s time it was realized that the mixing of hot and cold.
Exoplanet Atmospheres: Insights via the Hubble Space Telescope Nicolas Crouzet 1, Drake Deming 2, Peter R. McCullough 1 1 Space Telescope Science Institute.
8-1 The key characteristics of the solar system that must be explained by any theory of its origins 8-2 How the abundances of chemical elements in the.
Life in the Universe. Conditions may be right for primitive life to exist on Mars (or existed in the past) and Europa. Possibly some complex molecules.
All About Exoplanets Dimitar D. Sasselov Harvard-Smithsonian Center for Astrophysics.
1 Briefing to the CAA on the Terrestrial Planet Finder (TPF): Finding and Characterizing Earth-like Planets Zlatan Tsvetanov, NASA Program Scientist Charles.
March 21, 2006 Astronomy Chapter 29: Life in the Universe Does life exist beyond Earth? In our own solar system? Does intelligent life exist? How.
The Next 25(?) Years Future Missions to Search for Extra-solar Planets and Life.
Life on other planets Are we alone in the universe ? Some men were convinced to have discovered outerspaced life, but were debunked. - David McKay of NASA's.
Theories Of Existence Pranshu Sanghai IX C. The Need To Search For Aliens In the past couple of decades, the study of life on Earth has revealed the existence.
The Search for Extraterrestrial Life Chapter Thirty.
Group F – Liam Duffy, Darsh Kodwani and Stuart Keenan.
Announcements Pick up graded homework Total homework score so far (out of 26) is written in corner Projects will be graded by Thursday Bring questions!
Solar System J. Wunderlich, Ph.D. Image from
The Big Bang and The Expanding Universe Dr. Michael J Passow.
THE FERMI PARADOX First articulated by Enrico Fermi in If there is a high possibility for ETL (extra terrestrial life) then where is everybody???
A Systematic Search and Characterization of Dusty Debris Disks M. McElwain, B. Zuckerman (UCLA) Joseph H. Rhee, & I. Song (Gemini Obs.) Photo Credit: T.
SPACE SYSTEMS UNIT Chapters 26 & 30.
Extra-Solar Planets Astronomy 311 Professor Lee Carkner Lecture 24.
NASA and us Ms. Wood. Things you should know Moon revolves around sun as it revolves around Earth Millions of galaxies Solar system is made of: Sun Planets.
1 An emerging field: Molecules in Extrasolar Planets Jean Schneider - Paris Observatory ● Concepts and Methods ● First results ● Future perspectives.
Our Solar system YouTube - The Known Universe by AMNH.
The Search for Extrasolar Planets Since it appears the conditions for planet formation are common, we’d like to know how many solar systems there are,
Searching for Brown Dwarf Companions to Nearby Stars Michael W. McElwain, James E. Larkin & Adam J. Burgasser (UC Los Angeles) Background on Brown Dwarfs.
18.3 Life Around Other Stars Our goals for learning Are habitable planets likely? Are Earth-like planets rare or common?
Worlds Unnumbered Lecture Twenty-Nine, Apr. 14, 2003.
Are We Alone? Chris De Pree RARE CATS June The Questions Are there other planetary systems? How do we detect other planetary systems? What is Life?
Worlds around Distant Suns Mini University June 16, 2003 Among the most significant discoveries of the 20th Century.
2011: TWO MAJOR DEVELOPMENTS IN ASTRONOMY AND THE SPACE PROGRAM.
Medium-Rare Earth. Rare Earth Right distance from star Right mass of star Stable planetary orbits Right planetary mass Jupiter-like neighbor Plate tectonics.
Extra-terrestrial life: Is there anybody out there? Dr Martin Hendry University of Glasgow Reach for the Stars.
Exoplanets: direct detection ASTR 1420 Lecture 17 Sections 11.2.
DARWIN The InfraRed Space Interferometer. Status of exo-planet search Stars (Solar type) observed: Planets detected: ~ 86 Radial velocity measurement.
Extra-terrestrial life: Is there anybody out there?… Saturday Sept 24 th 2005 Dr Martin Hendry University of Glasgow.
Chapter 18 Life In The Universe. We have already launched our first robotic spacecraft into interstellar space Pioneers 10 and 11 carry a copy of this.
Extrasolar Planets The Search For Ever since humans first gazed into the night sky, the question of whether we are alone in the universe has remained unanswered.
Announcements Observing on the roof of Van Allen Hall, “clear sky patrol”, will begin on Tuesday, September 7 th. For that week, it will run from Tuesday.
Extraterrestrial Life Antígona Segura Peralta Penn State University, College of Earth and Mineral Sciences Penn State Astrobiology Research Center.
THE LIGHTS IN THE SKY ARE STARS. SPECULATION: IS THERE LIFE ON OTHER WORLDS - PLANETS AROUND OTHER STARS OR PLANETS AND MOONS WITHIN OUR OWN SOLAR SYSTEM?
Extra-Solar Planetary Systems. Current Planet Count: 331 Stars with Planets: 282 Earthlike Planets: 0 Four of the five planets that orbit 55 Cancri.
The Search for Extra-Solar Planets Dr Martin Hendry Dept of Physics and Astronomy.
Leaning objectives: Explain that: Elements as heavy as iron are formed inside stars by nuclear fusion. Heavier elements are formed in supernovas. Exploding.
What Does the Infrared Have to Do With Space?
Adaptive Optics for Astronomy Kathy Cooksey. AO Basics Photons –Travel in straight lines Wavefront –Line perpendicular to all photons’ paths Atmospheric.
Lecture 13 6/29/07 Astronomy Difficulties It is extremely difficult to detect extrasolar planets Stars are a billion times brighter than the reflected.
Homework 8 Due: Monday, Nov. 28, 9:00 pm, Exam 2: Weds., Nov. 30.
The Search for Life in the Universe. Criteria Defining Life 1.Made up of one or more cells 2.Organized 3.Grows & develops 4.Reproduces 5.Responds to stimuli.
Big Idea: Life Beyond Earth Chris Impey Department of Astronomy University of Arizona Chris Impey Department of Astronomy University of Arizona.
Are We Alone? Objective 1: The process of cosmic evolution as it is currently understood. 2: Evaluate the chances of finding life in the solar system.
NASA’s Kepler and K2 Missions:
Q4, A1143, Au15, Pradhan: Curve +5%. Life: Definition, Origin, Criteria What is the scientific definition of life? Collection of atoms  Organic molecules.
Universe Tenth Edition Chapter 27 The Search for Extraterrestrial Life Roger Freedman Robert Geller William Kaufmann III.
Life on Other Worlds? Please pick up your transmitter and swipe your ID.
The Search for Another Earth Exoplanets and the Kepler Spacecraft.
Page 1 Adaptive Optics in the VLT and ELT era François Wildi Observatoire de Genève Credit for most slides : Claire Max (UC Santa Cruz) Basics of AO.
The Search for Another Earth. Exoplanets and the Kepler Space Telescope An exoplanet or extrasolar planet is a planet that orbits a star other than the.
Goal: To understand life in our universe.
Goal: To understand intelligent life in our universe.
Life: Definition, Origin, Criteria
Guiding Questions What role could comets and meteorites have played in the origin of life on Earth? Have spacecraft found any evidence for life elsewhere.
Where are the little green men? Are “they” out there?
Life: Definition, Origin, Criteria
Planets Tuesday, March 4.
Astronomical Technology
Presentation transcript:

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

Fig , p.423

Fig , p.428

Why SETI will Fail

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

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

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.

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

Fig. 20-3a, p.418

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

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…

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

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

AIRS spectrum

TPF/Darwin design concepts

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.

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

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

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.

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

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.

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?

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.

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.

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

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.

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

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

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

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

Epoch 5 astrometry - NICMOS Unequivocal common P.M.

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

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