Atoms and Stars IST 2420 and IST 1990 http://www.is.wayne.edu/drbowen/aasW05 Class 11: March 30 Plagiarism • Starting tonight, all essays on diskettes • I believe I am seeing plagiarism in Essays. o Primary effect: lack of self-confidence • You should read the section on plagiarism in the Syllabus before doing this • If A copies from B, both are at fault. o o 3/30/05 If I cannot tell who did what, I will be impartial Plagiarism applies to (wrong) ideas as well as words Atoms and Stars, Class 11 2 Plagiarism • I have received plagiarized lab reports. Memo to Department o First time: treated as report not turned in (can be redone) o Second time: assignment failed, no re-do o Third time: course failed o • Starting with this week’s lab session, Reports must be turned in the following week. 3/30/05 Atoms and Stars, Class 11 3 Lab 9B 3 • C (a b) this is wrong, intentionally 7 o Correct formula is very complicated • Real point of lab – strength of authority • Points for report Realizing there is a disagreement o Checking measurements and calculations o Reporting the disagreement o 3/30/05 Atoms and Stars, Class 11 4 Lab Reports • As of tonight: Lab Reports that have only a data sheet get a grade of “D.” o Lab Reports without an original data sheet get a maximum grade of “C” o 3/30/05 Atoms and Stars, Class 11 5 From Last Week • Why do scientists think that space-time is curved (i.e., General Relativity)? Advance of the perihelion (point of closest approach to sun) of Mercury – ellipse rotates in space, not allowed if Newton is 100% right o Bending of light by objects o Gravitational and cosmological red shifts o Black holes o • Many consistent with modifications to G.R. 3/30/05 Atoms and Stars, Class 11 6 Error in Class 4 • Slide 18: Aristotle inferred spherical earth from its shadow on the moon (phases of moon). This is correct – he did. o I also said this was the modern explanation for the phases of the moon – it is not • Modern explanation is that the moon is illuminated by the sun, and we see it from different angles as it circles us and we circle the sun 3/30/05 Atoms and Stars, Class 11 7 About Science… • Science involves discourse between scientists – shared language, purpose, methods. Variations within scientific fields. o Study science now by studying scientists • When a new area is being explored, common for consensus to change, even drastically • Even after things settle down, do not expect 100% agreement 3/30/05 Atoms and Stars, Class 11 8 Epistemology • Several times you have asked me “Is this (absolutely) true?” I tend to hesitate with questions like this – here is why. • Epistemology – the study of knowledge – why do we accept things as true? • Properties we would like for knowledge/truth: Eternal – unchanging o Universal – the same everywhere o (Also that it be understandable) o (Also that it be right, of course) o 3/30/05 Atoms and Stars, Class 11 9 Epistemology • Science flunks “eternal” o Scientific truth is provisional – subject to change • Religions have problems with “universal” How can different religions differ, if there is one truth? o For science and religion, Galileo agreed with modern Catholic doctrine – there is one truth o • Reinterpret Bible if it disagrees with accepted science o 3/30/05 Today, religions generally ignore disagreements with each other Atoms and Stars, Class 11 10 “Expanding Circles” • So far, disconnected areas of knowledge: Air and water pressure o Speed of light o Falling and sliding objects o Motions of the planets and stars o • Each area (circle? blob?) expands • What happens next? 3/30/05 Atoms and Stars, Class 11 11 Expanding Circles • Eventually, expanding circles must meet and overlap o Before meeting, each area has a unique approach and theories – areas will not agree • Possible interactions: Withdrawal (NOMA in science) o One wins out over the other o Compromise o Synthesis o 3/30/05 Atoms and Stars, Class 11 12 Expanding Circles • Case of Newton (and Kepler) uniting terrestrial and celestial mechanics New theory o Each is understood more accurately and causally o A bonus – applies to all motion, calculus, applied in technology, model for new science o • Other examples coming up 3/30/05 Atoms and Stars, Class 11 13 Readings Atomic Nature of Matter, Hewitt • All matter is atoms Atoms are elements – “indivisible” – mostly empty o 109 types total, 90 are natural, rest radioactive o • Each type has its own properties, e.g. weight, reactions o Hydrogen most common atom in universe • Rare by itself on earth o Life primarily C, H, O, N • Atoms small enough to be invisible - waves 3/30/05 Atoms and Stars, Class 11 14 Atomic Nature of Matter • First direct evidence 1827 Robert Brown Noticed spores jiggling under microscope o “Brownian motion” – bombarded by molecules o Now we have more direct evidence o • Atoms bond into molecules – many types Molecules - compounds o Molecules have separate properties from atoms o Burning is combination with O o • New - modern automobiles very little CO 3/30/05 Atoms and Stars, Class 11 15 Atomic Nature of Matter • 1811 (Amedeo) Avogadro’s hypothesis At same T & P, equal Vs of gas have equal #s o Each atom, molecule heavier gas heavier o • Amu = atomic mass unit • C 12 amu, H 1 amu, O 16 amu, U 238 amu, H2O 18 amu – also combine in gm, lb etc. • Atom has electrons orbiting nucleus Electrons – volume but very little mass o Nucleus – mass but very little volume o 3/30/05 Atoms and Stars, Class 11 16 Atomic Nature of Matter • Electron, e – negative charge, flow of electrons is electrical current • Nucleus has neutrons, n (no charge) and protons, p (positive charge) o Cube 3/8” would weigh 133,000,000 tons • Like charges repel, unlike charges attract o o Nucleii positive, repel each other Atoms neutral; #e = #p • #e not = #p under special circumstances 3/30/05 Atoms and Stars, Class 11 17 Atomic Nature of Matter • Electrons in shells (2, 8, 18, …) If shells filled, element is inert o Unfilled shells determine activity o #p = atomic number, chemical characteristics o • Same element even if atom loses or gains electrons • Antimatter – anti-electron (1932), antineutron, anti-proton o Annihilate 100% energy (light) • Nuclear reactions normally 1% 3/30/05 Atoms and Stars, Class 11 18 Readings - Chemistry • Chemistry developed after Newton (physics) Alchemy – transmutation of elements o Medicine o Industry – much demand for chemicals 1700s o Mechanical approach from Descartes & Newton o • 1700 still Aristotelian elements Earth – fixed volume & shape o Water – fixed volume only o 3/30/05 Atoms and Stars, Class 11 19 Chemistry • 1700 still Aristotelian elements Air – volume & shape expanded to container o Fire passed through container walls o • 1727 – Stephen Hale: “fixed” air released from solids, much interest • 1749 Jean-Jacques DeMairan evaporated liquids (e.g. ether) in a vacuum, froze water But liquids supposed to evaporate into air o Fire combined with liquid = air? Many types? o • Water could be solid, liquid, vapor –differ by fire? 3/30/05 Atoms and Stars, Class 11 20 Chemistry • How could “big four” be elements? • 1750s Joseph Black experiments with “magnesia alba,” gave off “fixed air” that extinguished flame (CO2), denser than “common air,” turned limewater cloudy o Use limewater test to show fixed air came from fermentation & charcoal combustion, would not support life • “Fixed air” became specific name for this gas (CO2) 3/30/05 Atoms and Stars, Class 11 21 Chemistry • 1766 Henry Cavendish: “inflammable air” H • 1772 Joseph Priestley obtained “fixed air” in other ways, demonstrated solubility in water (& taste – birth of carbonated beverage industry) o Many other types of air – “dephlogisticated air” O • Phlogiston theory of combustion – burning releases phlogiston – from Germany, industrially useful • When air is saturated with phlogiston, combustion and life cease 3/30/05 Atoms and Stars, Class 11 22 Chemistry • Antoine Lavoisier (1743 – 1794) Graduated in law but continued science studies o Accurate weighing, also many practical results o (Calcination – turn a metal to powder (“calx”) by heating in air below melting point – phlogiston theory explained this as driving off phlogiston) o But Lavoisier’s weighing showed that weight increased, for all metals – a problem for phlogiston theory of combustion o 3/30/05 Atoms and Stars, Class 11 23 Chemistry • Calx of mercury (oxide of mercury) when heated gave off air (gas) but supported combustion and life o Priestley found this air better (5×) for combustion and life than “common air” (air) – “eminently respirable air” • Lavoisier had assumed it was common air o 3/30/05 Lavoiser confirmed this, but common air was then a mixture Atoms and Stars, Class 11 24 Chemistry • 1778 Lavoisier showed this air also formed acids, named it oxygen (“acid former”) (but we now know that hydrogen makes acid) • 1783 Cavendish’s assistant told Lavoisier about Cavendish’s experiment of applying spark to inflammable air (H), finding dew which was identified as water o 3/30/05 Lavoisier – water was not an element, combination with oxygen for all combustion Atoms and Stars, Class 11 25 Chemistry • Lavoisier named flammable air “hydrogen” for “water former” • Lavoisier and others formed new chemical terminology – speaking well was like reasoning well Oxide – combination with oxygen o Names indicated amount of oxygen (ous > ic) o • Sulfurous acid H2SO3 • Sulfuric acid H2SO4 3/30/05 Atoms and Stars, Class 11 26 Chemistry • Lavoisier terminology Gas – any vapor o Air – the atmosphere, a mixture (80% N, 20% O) o Fire was caloric (no correct theory until 19th century – started by Count Rumford) o • John Dalton (1766 – 1844), meteorologist o 3/30/05 Converted to chemistry when he understood air was a mixture – why didn’t different gases separate by gravity? Atoms and Stars, Class 11 27 Chemistry • John Dalton (1766 – 1844), meteorologist Also gases dissolved in water proportional to pressure – why? o Hypothesized gases composed of atoms, each gas interacted with itself o “Law of definite proportions” – chemicals combined by weight in simple ratios o Dalton proposed formulae based on these – chemical atomism o 3/30/05 Atoms and Stars, Class 11 28 Common Writing Problems • Functional grammar o o o o o o 3/30/05 Rules of grammar have a purpose – to transmit meaning Rules of grammar are always changing Different grammars for different groups Get too far from the group’s grammar and you are not understood (must change with changes) The further you get from the group’s grammar, the harder it is to understand you Being able to use good standard grammar is like dressing well for a job interview Atoms and Stars, Class 11 29 #1 Reason for Writing • To organize your own thinking #1 Way to Good Writing • Have something you want to say More Examples and Details • www.is.wayne.edu/olgt or The Everyday Writer 3/30/05 Atoms and Stars, Class 11 30 Organization • Many possibilities for organization Historical o Logical o Specific to general, or general to specific o Combination o • Signal transitions from one topic to another o 3/30/05 Paragraphs help here Atoms and Stars, Class 11 31 Quick-and-Easy Organization • Write body first • One you have figured out what you are going to say (the Body), write the Introduction and Conclusion afterwards • Body should have general statements and specific examples and quotes 3/30/05 Atoms and Stars, Class 11 32 Sentences • A sentence: Verb (easiest to find - action) o Subject (did the action) o Complete thought o (starts with capital, period at end) o • (Y/N) Because he hit the ball. • (Y/N) John hit the ball. 3/30/05 Atoms and Stars, Class 11 33 Sentences • Is it a sentence? Consider it all by itself. • Common sentence problem #1: o Sentence fragment – something that starts with a capital and ends with a period but is not a sentence • Because he hit the ball. John ran to first base. • Fix by joining to main thought with a comma (,) – Because he hit the ball, John ran to first base. 3/30/05 Atoms and Stars, Class 11 34 Sentences • Is it a sentence? Consider it all by itself. • Common sentence problem #2: o Run-on sentence – two or more sentences written as one • John hit the ball he ran to first base. • Fix by breaking into two sentences – John hit the ball. He ran to first base. • Or by joining with semicolon (;) to show causality – John hit the ball; he ran to first base 3/30/05 Atoms and Stars, Class 11 35 Number (singular/plural) • Both subject and verb have number o If these are not the same, signals conflict • Members join the club • A member joins the club • “One s” • Without a reason, do not change number from sentence to sentence o 3/30/05 (Bad) People should take care of their health. You should take your vitamins. Atoms and Stars, Class 11 36 Tense (past, present, future) • Without a reason, do not change tense from sentence to sentence Citations • “Scientific investigation is not, as many people seem to suppose, some kind of modern black art.” (Huxley, 1) • Cite the source even if you are paraphrasing o 3/30/05 Ideas: very important in academia, trace them Atoms and Stars, Class 11 37 Punctuation • Apostrophe (‘) o o Contraction Possession (‘s or s’) • Some words inherently possessive, no ‘ (e.g. theirs) o Never for pluralization (in 1600s, not in 1600’s) • Lists Separate list items with commas (last one is optional) o If any list has a comma inside an item, separate items with semicolon o List can be singular even if many members o • This group of authors travels by bus. 3/30/05 Atoms and Stars, Class 11 38 Wrong Word • Some words are commonly confused – memorize or use list or dictionary o o o o o o 3/30/05 its Vs it’s whose Vs who’s their Vs there too Vs to accept Vs except Many, many more Atoms and Stars, Class 11 39 Lab – Experiment 10; Lenses • • • • General – light is easier to see than bunny Lenses are in tissue paper inside envelopes Labels on envelopes do not mean anything Each envelope has five lenses – keep track by type Three convex with increasing thickness o One concave o Other types: plane, plano-convex, plano-concave o 3/30/05 Atoms and Stars, Class 11 40 Lab • Exercise I. o For this part, start with the lens touching the paper. As you move the lens towards you, if you see a dramatic change in the image, keep the lens closer to the paper. • Afterwards – what happens as you move lens past the point of dramatic change? What type of lens is magnifying? Reducing? o For magnifying lens, how does focal length vary with curvature? o 3/30/05 Atoms and Stars, Class 11 41 Lab • Exercise II: image properties Real (can be projected on a screen) Vs virtual (behind lens, can be seen but not projected) o Inverted (upside down) Vs non-inverted o Magnified (larger than object) Vs reduced o • Measure focal length in mm o 3/30/05 Measuring focal length for reducing lens Atoms and Stars, Class 11 42 Lab • Exercise III: Two lenses are objective (closer to object) and eyepiece o Good telescope – focal length for objective is longer than for eyepiece o Good idea to make screen for objective: cut hole in card, slightly smaller than lens, tape lens to card, bend card to stand lens up o • Do not do the WRITING ASSIGNMENT 3/30/05 Atoms and Stars, Class 11 43 For Next Week • Reader: 254 – 275 (Bronowski and Nissani articles) • Lab Manual: Experiment 11, Pp 64 - 77 on Centripetal Forces and Gravitational Motions • Turn in Lab 10 report 3/30/05 Atoms and Stars, Class 11 44 Future Due Dates • Essay 2 due April 13 o The Everyday Writer (DIS standard) and writing web site http://www.is.wayne.edu/olgt, link to Writing Guide • Last regular class April 20 o Work turned in after this date may not be included in regular grade • April 27 Final Exam (NOT April 23) 3/30/05 Atoms and Stars, Class 11 45 IST 1990 • Essays based on set questions, taking readings into account Get a set from me o Tell me which question you are answering, before title o 3/30/05 Atoms and Stars, Class 11 46 End Lab starts now, for everyone! Not like last week.