Atoms and Stars IST 2420 and IST 1990 Class 14 Winter 2006 Instructor: David Bowen Course web site: www.is.wayne.edu/drbowen/aasw06 IST 1990 Moodle: techtools.culma.wayne.edu/moodle 4/19/06 Atoms and Stars, Class 14 1 Agenda • Assignments, passbacks, initial signin sheet • Pick up: o Notes for Class 14 • Class information o Special Grade Request if much work will be late • • • • Review of readings Emphasizing main points one more time Updates: natural disasters & bird flu Lab 11: The Orbiting Bottle 4/19/06 Atoms and Stars, Class 14 2 Upcoming … • Tonight is the last regular class o Essay 2 due o Review for Final Exam • April 26: nothing that night but the Final Exam • Opportunities for extra help: o Review Session during class o 5 – 6 PM before Final (April 26) o Telephone, email, set up a time 4/19/06 Atoms and Stars, Class 14 3 My new cell phone number • 248-376-9848 • This is the number to call during 5 – 6 PM office hours 4/19/06 Atoms and Stars, Class 14 4 Semester is Ending! • If you have been relying on being able to turn work in late, it is late! o Alternatives: D, E, I, X, drop – see counselor! • Getting ready for Final: o Read Information Sheet carefully – a lot of information there o Look at Final Topics carefully o Use Review Session! • Final Where-Is handed out at the previous class 4/19/06 Atoms and Stars, Class 14 5 Course Grades • If you are turning a bunch of work in at the end, I may not get it graded in time for the regular grades (see the Syllabus). • If this is you (turning it in late), what grade do you want for the regular grade? E, X, I • Fill in the Grade Request form (get a copy from me) to let me know – otherwise it’s my choice. • You can withdraw (W) through April 25 • Medical Withdrawal 4/19/06 Atoms and Stars, Class 14 6 Your Current Status • Grades I have for you: o Online Grade Report, link off the course web site (see first slide) o Enter first name, last name, password the get report • Grade you are headed for: o Grade What-If on course web site • Ask for help with these if you are having problems 4/19/06 Atoms and Stars, Class 14 7 Makeup for Final Exam • Let me know by email that you want a makeup, within 24 hours after the Final (University regulation) • Date / Time Friday May 26 6 PM on campus • Watch for later email about building and room (but I won’t send you an email unless you send me the email at the top bullet) 4/19/06 Atoms and Stars, Class 14 8 Lab 7 Questions at end A. B. C. D. Weight does not set flotation Specific Gravity < 1 (water) float Ice floats Specific Gravity < 1 Specific Gravity useful in deciding what material an object is made of E. Archimedes right, displaced volume = object volume F. If S.G.object < S.G.liquid, then object floats in liquid. dumbbell floats in Mercury. 4/19/06 Atoms and Stars, Class 14 9 Lab 11: Orbiting Bottle • If your two results (A & B) for the horizontal (inward) force, FH, agree, then your data are consistent with Newton’s Laws (including Universal Law of Gravitation). • See Theory section for the proof of this 4/19/06 Atoms and Stars, Class 14 10 Brain Candy… Wormhole • A theoretical possibility within Einstein’s General Theory of Relativity (1916) o A shortcut through 4-D space-time that could dramatically speed travel between points connected by the wormhole, and into the future o Requires an undiscovered form of exotic matter that may not exist, with negative energy density – a “white hole,” contrasts with a black hole o Wormhole could collapse on the traveler • http://en.wikipedia.org/wiki/Wormhole 4/19/06 Atoms and Stars, Class 14 11 Wormhole From Wikipedia (see link on previous slide) 4/19/06 Atoms and Stars, Class 14 12 Global Warming (cont’d) • What to do? Options: o Nothing. Live with it. (Physical and ecosystem consequences not known) • Humans can adapt quickly, natural world cannot – evolution is slow, but humans are free of evolution • Many past examples of disasters from warming • Natural world is too complex for us to make good predictions in from our present science o Cosmetic actions. Cite uncertainty in effects, call for more research • May never have 100% certainty of the effects o “Invisible hand” of market 4/19/06 • Trade CO2 permits Atoms and Stars, Class 14 13 Global Warming (cont’d) • Options (cont’d): o Limit CO2 production • Increase energy efficiency, use waste energy, switch to low-carbon fuels (natural gas) away from coal and petroleum o Remove CO2 once it is generated • Sequestration – pressurized underground or under deep ocean (will warming release it?) • (DB) Recent poll says US thinks scientists are confused about Global Warming. NOT! o Deliberate confusion caused by industry groups opposed to controls – citing 2 or 3 out of 2,500 4/19/06 Atoms and Stars, Class 14 14 Readings: Icecaps and Hurricanes Evidence for Global Warming: • Thawing icecaps • Coral bleaching • Hurricanes • Melting glaciers • Desertification • Rising sea levels 4/19/06 Atoms and Stars, Class 14 15 DB: That’s not all… • Many worldwide resource issues – “the human footprint” o Water (drinking, irrigation, industrial), food, farmland, population (6 billion 9 billion), living in unsafe places, petroleum, trash, development, health care, education, rights • Managing the human footprint will be a major, continuing issue 4/19/06 Atoms and Stars, Class 14 16 Re-emphasizing Main Points • Two pillars of science o Experiment: makes science reliable • Scientists led astray by logic (Aristotle) and belief (church and geocentrism, Inquisition) • Experiments base science on direct experience o Theory: makes science valuable • Once you have a reliable theory, it tells you the answer in advance, can use it as technology • Two quotes from Copi, Reader Pg 8 4/19/06 Atoms and Stars, Class 14 17 Re-emphasizing Main Points • I have the experiments in this course to: o Give you direct experience o Illustrate experiments described in class o Illustrate social nature of science within the lab groups 4/19/06 Atoms and Stars, Class 14 18 Updates • Bird flu: o Some concern over transmission via domestic pets in rich countries o Also being spread through smuggling o Anthony Fauci (NIH): probably no disaster here, BUT • Natural disasters: o Hurricane season of 2005: with better measurements, more hurricanes o In addition to hurricanes, warm Gulf of Mexico also important in tornado formation • Tornadoes generated when warm air from Gulf meets cold air from Northwest 4/19/06 Atoms and Stars, Class 14 19 Updates (cont’d) • Plate tectonics: o Determines location of mineral resources and fossil fuels • Mineral resources brought near surface by old zones of rising magma • Fossil fuels generated when organic matter covered over before it rots, “cooked” when drawn down to warmer depths (but not hot – like baking a turkey) then brought back near surface so we can find it – Temperatures increase going down into the earth • Plate tectonics does both of these 4/19/06 Atoms and Stars, Class 14 20 Updates (cont’d) • Tenth planet? o In Class 5, mentioned “tenth planet” 2003 UB313 nicknamed “Xena,” larger than Pluto o That size based on inference from brightness o New direct measurement says Xena about the same size as Pluto o Inference from brightness fooled because Xena is highly reflective o Now, Pluto and Xena will probably be either accepted as planets or demoted, as a pair o Meaning of “planet” still being debated 4/19/06 Atoms and Stars, Class 14 21 Uncertainty Principle (Repeat) • No practical effect at macroscopic level o A philosophical problem with The Mechanical Universe and with “The God’s eye view” or The Clockwork Universe over age of universe • Important at atomic and molecular level o Uncertainties are large on atomic scale o What underlies our reality is strange 4/19/06 Atoms and Stars, Class 14 22 Readings: Knowledge or Certainty Jacob Bronowksi • Absolute certainty is impossible in science o Looking at an object with infrared, then visible, then x-rays should yield greater detail. Infrared is very blurry, visible is pretty good, but x-rays are too high energy to be focused. Perfect detail of “God’s-eye” view is impossible o Statistical uncertainty in measurements - Gauss 4/19/06 Atoms and Stars, Class 14 23 Knowledge or Certainty • 1795 • Science is discussion and argument preceding knowledge • Also Uncertainty Principal 1927 Werner Heisenberg – cannot locate particle exactly o Irreducible uncertainty or fuzzy focus 4/19/06 Atoms and Stars, Class 14 24 Knowledge or Certainty • No practical effect at macroscopic level, but a philosophical problem with The Mechanical Universe and with “The God’s eye view” • But certainty leads to tragedy – Nazis • (DB) Certainty and power combined 4/19/06 Atoms and Stars, Class 14 25 What is Science? Moti Nissani, What Is Science? • Difficult or impossible to give a dictionarytype definition for science • (DB) Working scientists rarely think about the history or philosophy of science • Start with philosophy of Thales – free inquiry 4/19/06 Atoms and Stars, Class 14 26 What Is Science? (cont’d) • Then hypothesis and experiment (Torricelli) • Falsifiability – reason and logic have not been not sufficient to discover the truth in science (DB: belief, either) o But contradiction by experiment does not always mean rejection of hypothesis – can lead to reexamination of experiment or modification of hypothesis o Scientists “on the trail” have personal concerns 4/19/06 Atoms and Stars, Class 14 27 What Is Science? (cont’d) o Scientists “on the trail” have personal concerns • Argument and community lead to progress o Semmelweiss and deaths in maternity ward • • • • • • 4/19/06 Neighboring ward far safer Did priest’s visit scare patients? Washing hands – doctors did dissections beforehand This fixed the problem Profession slow to accept this change Even scientists can be closed-minded, resist change Atoms and Stars, Class 14 28 What Is Science? (cont’d) • Theories unify many hypotheses and experiments o Price is often inaccessibility to non-scientists • Scientists usually not concerned with these issues or with philosophical uncertainty • Science many not be perfect, but it can still be very good • Many use technology but not the scientific foundation 4/19/06 Atoms and Stars, Class 14 29 Physical Science: Current Status • Newton’s Laws, Maxwell’s Equations and similar classical theories (before ~ 1900) describe world we know and see • For things the size of molecules and smaller, need Quantum Mechanics • Very fast, need Special Relativity • Very heavy, need General Relativity • All three have weird things going on 4/19/06 Atoms and Stars, Class 14 30 Special Relativity • For fast-moving objects o o o o Max speed = c (speed of light) Objects foreshortened Time slows down But the traveling person says the same about you! o Space and time space-time o E = mc2 light has mass, is bent by gravity 4/19/06 Atoms and Stars, Class 14 31 General Relativity • For very heavy objects o Space and time warp, cause gravity o Perihelion (closest approach to sun) of Mercury’s ellipse not fixed as in Newton’s Laws, but advances 43 seconds of arc per century (observed), other effects in addition o Light bent twice as much as Special Relativity, observed 1918 4/19/06 Atoms and Stars, Class 14 32 General Relativity (cont’d) • “Einstein Halo” – light from far galaxy bent by near galaxy • Variation on gravitational lens • 12 found so far • Picture: New York Times, 12/6/05, Pg D4 (Science) 4/19/06 Atoms and Stars, Class 14 33 Quantum Mechanics • At molecular level and smaller, waves and particles merge – everything is both o Wave – spread out, cannot contain it o Particle – have it or don’t o Q.M.: wave gives chance of “catching” particle • Cannot be made certain • Uncertainty Principle o Carries over to regular world, makes clockwork universe impossible over age of universe 4/19/06 Atoms and Stars, Class 14 34 Quantum Mechanics (cont’d) • Accounts for properties of ordinary materials o o o o o Theoretical: keeps matter from collapsing Color Solid (strength), elastic, gaseous Solid state electronics – semiconductors Forces – due to exchanges of particles • No Newtonian “action at a distance” • E.g. electrical force carried by photons – particles of light 4/19/06 Atoms and Stars, Class 14 35 Combinations • Fast (S.R.) and heavy (G.R.) – OK, since Special Relativity contained within General Relativity • Fast (S.R.) and small (Q.M.) – these two get along well – together, predict anti-particles • Heavy (G.R.) and small (Q.M.) – conflict o No “Quantum Theory of Gravity, ” union of both • General Relativity is the theory of gravity 4/19/06 Atoms and Stars, Class 14 36 Combinations (cont’d) • Heavy (G.R.) and small (Q.M.) – mathematical conflict o Competing theories of gravity – “embarrassing” • G.R.: gravity caused by masses warping space-time • Q.M. – gravity due to exchange of “gravitons” (not found yet) o “String Theory” might unite these two 4/19/06 • “Theory of Everything” – accelerating expansion(!) • Matter and energy composed of elemental vibrating strings and membranes • Eleven dimensions, seven curled up too small to experience directly – may have indirect experience • Theory still developing, no unique experimental evidence yet Atoms and Stars, Class 14 37 Three waves of science? 1. Physical science – the subject of this course – mature, quantitative (95%) • Very controversial when it was new • 1600 – 1800 AD, although very long roots & still developing • Now pretty much settled for everyday objects 2. Biological or life science – qualitative (30%?) • Much newer, still controversial publicly, but for scientists it is settled • 1800 – 1935 AD • • 4/19/06 Coming into general use in society & economy Will qualitative change to quantitative? Atoms and Stars, Class 14 38 Three waves of science? 3.Cognitive science – how emotions and the mind work – just starting (5%) o Will be as controversial, if not more o Potential for controversy: Science of Desire : The Gay Gene and the Biology of Behavior & The God Gene (spirituality) / Dean Hamer • Spirituality predestined for some, denied to others? • A single gene is unlikely to be the sole cause o Will call into question how we view ourselves 4/19/06 Atoms and Stars, Class 14 39 The end of the ride • Strong dose of the value of science here • One more time, about science: o Two pillars – repeatable experiment (what makes it reliable) and explanatory theory (what makes it valuable) • Developed 1600 – 1800 AD: Copernicus to Dalton o Developing hypotheses and theories is creative o Has a boundary but expands aggressively not a complete basis for living o o o o 4/19/06 Now drives technology We all use it Conflicts with some, but not all, religious beliefs People of all ethnicities have been able to contribute Atoms and Stars, Class 14 40 Review for Final 4/19/06 Atoms and Stars, Class 14 41