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The Search for Life in the Universe Dr. Dan Caton Professor and Observatory Director November 9, 2011 What we will look at… Overview of the search for extraterrestrial life Brief review of exploration in our solar system The chances for life elsewhere in our Galaxy The problem of SETI—the search for extraterrestrial intelligence Historical, current and planned searches Efforts to transmit Why have we not found ET? The search for respectability International Astronomical Union created a Commission on ETL in 1982 Long of Interest Poster from 1800-01 Intelligent Life Here? Started by panspermia? Venus too hot? Our Moon Life from Earth, in subsurface ice? Mars—we looked at this already… Jupiter or Saturn? Maybe on one of the moons? Beneath the ice on Europa? Or… Saturn’s Titan: Cassini / Huygens Mission Cassini still orbiting Saturn, Huygens probe landed on its moon, Titan a few years ago. Beyond our Solar System: we turn to the stars… SETI: Turn outward for the Search for Extraterrestrial Intelligence: Searches and Transmissions Will confine ourselves to Milky Way Galaxy Questions to investigate What are the chances that intelligent life exists? What evidence is there for life-supporting extrasolar planets? How does life form and evolve? How do we communicate? Can they exist? Frank Drake first calculated the chances of there being civilizations in our Galaxy with whom we could communicate. He developed his equation, which became known as the Drake Equation… Frank Drake The Drake Equation N = R fS fP ne fl fi fc L R = Average rate of star formation (stars/year) fS = fraction of stars that are “good” Suns fP = Fraction of good stars with planets ne = number of planets per star in ecoshell fl = fraction of planets on which life develops fi = fraction that develop intelligence fc = fraction that reach electromagnetic communicative phase L = Lifetime in communicative phase (years) R = rate of star fromation R ~ 4 stars/year in our Galaxy This probably the best known variable in the Drake Equation FS = fraction of stars that are “good” Suns O, B stars too short-lived K, M stars – flares dangerous? A –F stars just right? Fp = Fraction of good stars with planets Several hundred exoplanets now known (+ Kepler) Something on the order of 0.1 or 10% of stars have planets? Or, most? Don’t really know since just starting to find small planets. ne = number of planets per star in ecoshell (the habitable zone) ne ~ 1 - 2 fl = fraction of planets on which life develops fl = fraction of planets on which life develops How does life begin? The Miller-Urey Experiment 1952, University of Chicago. Produced amino acids. Recent analysis (published 4/2011) After Miller’s death in 2007 the vials were re-examined, including some from unpublished experiments. Vials associated with the original, published experiment contained far more organic molecules than Stanley Miller realized — 14 amino acids and five amines. The 11 vials scientists recovered from the unpublished aspirator experiment, however, produced 22 amino acids and the same five amines at yields comparable to the original experiment. Newest idea: life formed in ocean bottom Timeline of Life on Earth Our Ancestors began several million years ago Primates Extinction of dinosaurs allowed mammals (and us) to develop 65 My ago Are we the pinnacle? Is intelligence inevitable? fi = fraction that 00 develop intelligence Evolution and natural selection not pointed to intelligence Dominant life form? If replayed the tape (Stephen J. Gould) fi = 1? fc = fraction that reach electromagnetic communicative phase Fraction that invent radio Same physics everywhere in Universe L = Lifetime in communicative phase (years) So far, ~ 100 years Lots of ways to end … bad ones here end life Or, we end the “communicative” part… … by having signals disappear! Optical fiber Satellite TV/Radio Low power Wi-Fi Small cell phone transmitters Internet TV Cell radio L is important because… … “f’s” multiply out to ~ 1, so N ~ 1 N = R fS fP ne fl fi fc L So may be 100 + 10x or so civilizations in the MWG to find Let’s go look! We will look in the radio—why? Where in radio? Meet ET at the “Water Hole” TV First search was at Greenbank, WV … … Project Ozma • 1960 • 200 hours observing two nearby solar stars in 21-cm • nothing found but a secret satellite 85-ft Harvard Dish has been used Paul Horowitz NASA thinks big: Cyclops Details… A thousand 100-meter dishes • Could detect ET’s broadcast, if within 100 ly (>6,000 stars) • ~5 billion $ (half what we spend in US every day, or <0.5% of US wars cost since 2001) NASA’s nemesis William Proxmire, the late Senator from Wisconsin Golden Fleece Awards Called off by Carl Sagan NASA’s initial hardware Software: see a pattern? This is a plot of signal (intensity of dots) in frequency vs. time Here it is A test: detection of Pioneer 10 But—Congress killed NASA’s SETI project… First Intentional Transmission The signal: digital Let’s look at why digital … Digital advantage sketch… Graphical The message consists of 1679 bits, arranged into 73 lines of 23 characters per line (these are both prime numbers, and may help the aliens decode the message). It consists, among other things, of the Arecibo telescope, our solar system, DNA, a stick figure of a human, and some of the biochemicals of earthly life. For less than 3 minutes it was the brightest source in the MWG at that frequency. Target: M13 (30,000 ly…) Our unintentional signals Radio is line-of-sight What is not received (most is not), leaks out into space Lets tune into … …Channel Earth As seen from Barnard’s Star NA East NA East Coast sets Coast rises Western Europe rises Aust. Japan rise Aust. Japan set Western Europe sets Cartoon… Pioneer 10 & 11 Plaques (1972-3) Voyager Record: “Best of Earth” Images and Sounds • “Best of Earth” • Narrated by Kurt Waldheim (19182007), then U.N. Secretary General and now known (embarrassingly..) to have been a Nazi war criminal. Friend of fellow Austrian Aaaaanold…. SETI@home Uses data from … “Parasitic” observations at Arecibo Telescope Allen Array 350 6.1-m dishes 1 – 10GHz (the “water hole”) Artist concept Funded by Microsoft co-founder Paul Allen (and COB, Charter Communications) Newer, offset Gregorian design SETI Inspired Carl Sagan’s Contact Ellie Arroway (Jodi Foster) loosely based on (real) Jill Tarter, former head of NASA SETI, now at the SETI Institute Why no detection? … …Enrico Fermi: “Where is everybody?” Would not be complete without mentioning Maybe in Historical Times? (Ezekiel 1) 4 I looked, and I saw a windstorm coming out of the north—an immense cloud with flashing lightning and surrounded by brilliant light. The center of the fire looked like glowing metal, 5 and in the fire was what looked like four living creatures. In appearance their form was human, 6 but each of them had four faces and four wings. 7 Their legs were straight; their feet were like those of a calf and gleamed like burnished bronze. 8 Under their wings on their four sides they had human hands. All four of them had faces and wings, 9 and the wings of one touched the wings of another. Each one went straight ahead; they did not turn as they moved. …. Interesting, but which myths do we choose to believe? (Brown Mountain Lights and the Cherokee myths… That’s our SETI discussion .. Questions?