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Transcript
Drake Equation Lecture Thirty-Three, April 23, 2003 Project • Due Friday April 25. • Discuss as much of the science from class as possible. • If your project is in electronic form you can turn in a disk or email it. • However, also turn in a hard copy! • Everyone should turn in a paper copy. SETI: Message in a Cosmic Bottle • How to send or receive a radio beacon? • Want signal to look “unnatural” and stand out • • above background of natural radio noise in Galaxy. Broad frequency region around a few GHZ (few times 109 cycles per second). This is in the microwave region (high frequency radio) of the spectrum. Here natural noise is relatively small. Radio communication over interstellar distances is feasible with present technology! Is anyone there? • Intelligence is ability to use radios. • Important differences searching for intelligent compared to primitive life! • How many civilizations are there in the galaxy that might try to call us? • The Drake equation is away to discuss our ignorance of this fundamental question. Drake Eq. • Is there likely to be anyone • • trying to send radio signals? Is SETI likely to succeed? Assumes a steady state: rate of new civilizations is nearly equal to rate of their death. “Writes one number, that we do not know, as the product of seven numbers, that we do not know.” Drake Equation • • • • • • • • Nc=Rs fp n fl fi fc L Rs=rate of (suitable) star formation fp=fraction of stars with planets n=number of “Earthlike” planets per solar system fl=fraction of “Earths” with life fi=fraction that is intelligent fc=fraction that develops a civilization L=lifetime of civilization Drake Equation Ns = A ¢ B ¢ C A = Astronomy = Rs¢ fp ¢ n B = Biology = fl¢ fi C = Civilization = fc¢ L Astronomy factors Rs, fp, n • Rs =# of suitable stars born each year in galaxy. • If suitable stars mean sun like. Rs¼ 2 (Probably • • want single stars not binary) fp = fraction of stars with planets. We are measuring fp as we find planets. fp > 0.1 n=# of earths per solar system. We will start to measure this with Terrestrial Planet Finder or similar spacecraft in near future. Now we have no reason to assume n is small. Note, how much like earth do we require?? Astronomy Factors • So far Rs, fp and n are straight forward factors from astronomy that we either know or will soon at least partially measure. • Therefore these factors are not very controversial and probably not very small. • Thus these factors do not dampen enthusiasm for SETI. Biology Factors fl, fi • Fraction of earths that develop life fl. • Some requirements for life: – Elements such as H, C, N, O… – Liquid H_2O – Energy source (chemical or star light…) – Primitive organic compounds such as amino acids. – Time to allow chemical reactions to increase the complexity of molecules. fl may be large • We assume fl may be large • • • because life started relatively quickly on earth. Simple organic compounds may be common. (Remember Miller exp.) However, there is a lot we don’t know about the origin of earth life. Finding life on Mars or elsewhere would strongly suggest that fl is large. Origin of Intelligence fi= fraction of life that develops intelligence • Intelligence may provide evolutionary • • • • advantage. However brain needs massive resources. Evolution will not favor intelligence unless advantages are very large. Low level intelligence needed for vision, mobility, eye-limb coordination… How large is the leap from this to humans? How long does intelligence need to evolve? Fraction that develops Civilization • What is civilization? Working together? Using technology? … • Do army ants or bees have a civilization? • What role does civilization play in evolution? • Here civilization means technology and radios. Lifetime of Civilization • Many civilizations on earth come and go: Egypt, Greece, Rome,… • We face many man made and natural dangers. • Vast majority of species that every lived on earth are now extinct. Total Extinction • How close have we ever come to the total extinction of all life on earth? • A very large impact could kill all life. – It would have to be so large that the heat boiled away all the oceans and filled the atmosphere with molten rock! – Perhaps this happened very early on and life had to start more than once. – We don’t think there has been this large an impact since. Snowball Earth • We have evidence that about 700 million years ago earth was covered in a global and very deep ice age. • Originally it was thought such an ice age would be disastrous with no way out. – Snow and ice reflect sun’s heat and this would keep earth cold with no way to melt the ice. – Apparently there is a way out. CO2 Cycle Controls Temp. • Volcanoes continue to put CO_2 into atmosphere • • • even in ice world. However, ice covers rock. Thus no way to capture CO2 back into the rock to make new carbonates. Greenhouse CO2 continues to build up in atmosphere. This finally melts ice and converts earth from frozen to very warm. With ice gone, eventually high CO2 in atmosphere recaptured into rocks. Snowball earth and life • Ice killed much life. However, some small • • pockets survived perhaps in volcanically heated pools. This was before life had evolved hard parts (such as bones) that left clear fossils. Great explosion of life with great increase in complexity and diversity occurred just after the snowball. Space colonization and Lifetime • If we colonize Mars say this might protect some life against many dangers such as a single large impact or a disease. • Still depend on the same sun so the sun going red giant will kill both earth and mars. • Colonizing other stars may prevent total extinction of humans and increase L. Number in Galaxy • Provides an estimate of distance between civilizations thus how far one must communicate. • Represent galaxy as a disk about 50000 Lt-years in radius. • Area of galaxy= R2 = 7.85e9 (Lt-Y)2. • Density of civilizations =N/A Example N=10^6 • =1e6/7.85e9 = 1.3e-4 civilizations per square Lt-Y. • Average distance to next civilization L • ¼ 1/L2 assume uniform grid of civilizations each L apart. • Or L¼ [1/]1/2. • L¼ 90 Lt-Years. What makes Earth Special? Is this a physics/ astronomy question? Or a biological question? Or a religious /philosophical question? What are some of the physics that goes into Earth having a stable climate for five billion years? Are We Alone? • Yes! • But how can that be. All those worlds, all those Suns in • • • • • all those Galaxies. Why only us? How could the Universe be so big and so so lonely? What is our destiny? If we kill ourselves, what has it all been for? All those worlds we can not detect. What are they for? “It would be a great waste of space”. We are not alone! • The Universe may team with intelligent life! • Man has been here for only a few million years. • Less then one one thousandth the age of the Universe. It is very likely that other intelligences are much older and wiser then we. We are but an insignificant new comer in a vast crowd. – What do we matter? – What will the older and wiser races do with us? Either Way it’s Scary • How can we be so utterly alone! • Or • How can we be so insignificant. Just one among so many countless millions. Primitive Life • Primitive life may be common in the Universe. – Organic compounds may be easy to make, [Review Miller Exp.] , and they may be common [Amino acids found in meteorites, spectral lines from some compounds found in space and in the atmosphere of Titan…]. – Life appears to have started quickly on Earth. [What happened quickly may be highly probable to happen elsewhere.] • Life is extraordinarily complicated. We don’t understand very much about how it got started on Earth.