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HONORS CHEMISTRY

Explore the evolution of atomic theory from Democritus to Rutherford, including Dalton's theories, isotopes, subatomic particles, and the Gold Foil Experiment. Discover the historical milestones that shaped modern atomic structure knowledge.

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HONORS CHEMISTRY

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  1. HONORS CHEMISTRY Chapter 4 Atomic Structure

  2. History of the Atomic Theory

  3. DEMOCRITUS (400 BC) • 1st atomic theory • “World is made of empty space & tiny particles called ‘atoms’.” • Atomos - Greek for indivisible • Smallest poss. particles of matter • “Diff. types of atoms for every type of matter” • General & not supported by experiment • Not accepted - Contradicted Aristotle

  4. ARISTOTLE • “Matter is continuous” - not made of smaller particles • “Hyle” • Accepted until 17th Century

  5. Isaac Newton & Robt. Boyle • Published articles on belief in atomic nature of elements • No Proof • Attempted explanations, no predictions

  6. John Dalton • Logical hypothesis on existence of atoms • Studied & explained work of other scientists • Lavoisier - “In a closed syst., the mass of the reactants = the mass of the products” • LAW OF CONSERVATION OF MASS • Proust - “Specific substs. always contain elems. in the same ratio by mass” • LAW OF DEFINITE PROPORTIONS

  7. Dalton’s Atomic Theory • Basis of modern atomic theory • 1st atomic theory based on experimental evidence

  8. Dalton’s Atomic Theory Four important statements: 1. All matter is composed of indivisible atoms. 2. All atoms of the same elem. are identical. 3. Atoms of diff. elems. are not alike. 4. Atoms unite in simple ratios to form compounds.

  9. Dalton’s Atomic Theory • Explains Law of Cons. of Mass • atoms are rearranged in a chem. rxn. • Explains Law of Definite Proportions • Not exactly correct

  10. DALTON ALSO STATED: • Law of Multiple Proportions • The ratio of masses of one element that combines w/ a constant mass of another elem. can be expressed in small whole numbers.

  11. Other Scientists • Gay Lussac - “Under constant conditions, the volumes of reacting gases & gaseous products are in the ratio of small whole numbers.” • Avogadro explained this - “Equal volumes of gases, under the same conditions, contain the same # of molecs.”

  12. Cathode Ray Tube • Tube w/ charged metal electrodes in ea. end • Anode - Positive electrode • Cathode - Neg. electrode • Rays in tube seemed to travel from cathode to anode • Cathode Rays

  13. J. J. Thomson • Discovered electrons using cathode ray tube • Determined charge to mass ratio of e-

  14. Robt. Millikan • Oil Drop Experiment • Measured the charge on an e- • std. unit of neg. charge (-1) • e- mass is 1/1837 mass of a H atom

  15. J. J. Thomson • Discovered electrons using cathode ray tube • Determined charge to mass ratio of e- • Discovered the proton using a modified cathode ray tube • same amt. of chg. as e- but positive • std. unit of (+) chg. = +1 • Calculated mass of p+ (1836 X mass of e-)

  16. Lord Rutherford • 1920 - predicted 3rd particle

  17. James Chadwick • Discovered the neutron • high energy particle w/ no chg. & approx. same mass as p+

  18. Dalton’s Theory was revised. Subatomic particles had been discovered.

  19. J. J. Thomson • Discovered ISOTOPES • atoms of the same elem. that differ in mass • have same # of p+’s, but diff. # of no’s

  20. Henry Mosely • 1913 - using x-rays, found the number of p+’s in the nucleus of an atom is always the same for a given element • Atomic Number (Z) - # of p+’s in the nucleus • # p+’s = # e-’s in a neutral atom

  21. The number of p+’s determines the identity of the elem. and the # of no’s determines the particular isotope of the elem.

  22. Dalton’s Theory revised again Not all atoms of the same element are exactly alike. Atoms are NOT indivisible!

  23. Nuclide - a particular type of atom containing a definite # of p+’s & no’s • Nucleons - particles that make up the atomic nucleus • p+’s & no’s • Mass Number (A) - total # of nucleons in an atom • Number of no’s = A - Z • (mass # - atomic #)

  24. Rutherford’s Gold Foil Experiment • 1912-1913 led by Lord Rutherford, assisted by a team of physicists (Niels Bohr, Hans Geiger, & Ernest Marsden) • Procedure: shot (+) charged subatomic particles @ very thin sheet of gold foil.

  25. Observations 1. Most particles passed straight thru foil. 2. Few particles were deflected @ large angles. 3. Very few (1 in 8000) bounced almost straight back. Conclusions: 1. Most of the atom is empty space. 2. + particles came close to “core” of atom which must have a + charge. 3. + particles almost hit core straight on. Rutherford’s Gold Foil Experiment

  26. Rutherford’s Gold Foil Experiment • Overall Conclusion • Atoms consist of (+) charged nucleus surrounded by e-’s

  27. Diameter of an atom ~ 100-500 pm • Radii of nuclei of atoms vary between 1.2x10-3 and 7.5 x 10-3 pm • Nucleus is ~ 1 trillionth the vol. of the atom.

  28. Henri Becquerel • 1896 w/ Marie & Pierre Curie discovered Radioactive Substs. • When brought near charged electroscope, leaves become discharged

  29. Radioactivity • Phenomenon of rays being produced spontaneously by unstable atomic nuclei • mixture of particles & energy given off by nuclei during spontaneous nuclear decay • amt. of energy very large - E = mc2 • Half-Life - length of time needed for 1/2 an amt. of a radioactive nuclide to disintegrate.

  30. Nuclear Force - force which holds p+’s and No’s together in nucleus • effective over very short distance

  31. Scientists agree on: 1. Nucleons have a prop. that corresponds to spinning on an axis. 2. e-’s don’t exist in nucleus, but can be emitted from nucleus.

  32. Star Trek Science

  33. Subatomic particles • - particles composing atoms • 2 broad classes • Leptons - (light particles) - truly elementary • best known: electrons • Hadrons - appear to be made of smaller particles • best known: neutrons & protons

  34. For every particle, a mirror image particle called an Antiparticle is believed to exist • antielectron is a positron • When particle & its antiparticle collide, both are destroyed & energy is produced.

  35. Several Leptons • electrons • neutrinos - essentially massless • Muon - much more massive than e- • Tau - much more massive than e-

  36. Hadrons divided into 2 groups • Mesons • Baryons • p+’s and no’s are baryons • Both made of Quarks • 6 kinds of quarks • up, down, charmed, strange, top, bottom • ea. quark comes in 3 different “colors” - red, blue, green • ea. quark has antimatter counterpart - antiquark

  37. If structure of nucleus is unstable, ejects particle or energy to become stable • Some nuclei naturally unstable, some artificially unstable

  38. 3 forms of radiation from naturally radioactive nuclei • 2 are particles • Alpha particle - 42He - helium nucleus a • Beta particle - 0-1e - an e-b • 1 Form is energy • Gamma Rays- g - very high energy x-rays

  39. Short hand to represent particles • Upper rt. “corner” - charge on ion • Lower rt. - # of atoms in formula unit • Upper left - mass # • Lower left - charge on nucleus or particle

  40. Examples • 3216S - Sulfur nucleus or atom • 0-1e - electron • 42He - alpha particle (helium nucleus)

  41. Scientists create radioactive nuclides by bombarding stable nuclei w/ accelerated particles or w/ neutrons in nuclear reactor • Decay by emitting natural radiation & other methods.

  42. Planetary Atomic Model • Proposed by Rutherford and Bohr • e-’s “orbit” around nucleus • H atom similar to solar syst. w/ 1 planet

  43. Bohr exposed atoms to radiant energy • atoms absorb some energy • Excited Atoms • Excited atoms & molecs. produce energy changes • unique & can be used to identify particle • absorb and emit radiant energy

  44. SPECTROSCOPY • Method of studying substs. exposed to exciting energy

  45. SPECTRUM • Pattern of radiant energy studied in spectroscopy

  46. ELECTROMAGNETIC (RADIANT) ENERGY • Visible light, radio, ultraviolet, infrared, etc. • Travels in waves • variations in elect. & magnetic fields taking place in regular repeating fashion • Frenquency - n- # of wave peaks that occur in a unit of time • meas. in hertz (Hz) = 1 peak or cycle per sec.

  47. ELECTROMAGNETIC (RADIANT) ENERGY • Travels @ speed of light (c) • 3.00 x 108 m/s in vacuum • Wavelength - l - physical dist. betw. peaks • Related by c = ln • Amplitude - maximum displacement from zero

  48. Excited atoms lose energy • Energy emitted by gaseous atoms can be spread into a spectrum. • Emission Spectrum - shows l’sof light given off by excited atoms • Absorption Spectrum - have lines missing from continuous spectrum showing which l’s of light have been absorbed

  49. Lines missing in absorption spectrum are the same as lines shown in emission spectrum • unique to ea. elem. • used to identify elems.

  50. Electromagnetic Spectrum • Radio waves - longest l’s • Gamma waves - shortest l’s • Visible light????

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