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Unit 3: Atomic Structure

Outline. Chemistry. Unit 3: Atomic Structure. PowerPoint Presentation by Mr. John Bergmann. Basics of the Atom. Location in the Atom. Charge. Particle. Mass. proton. 1+. in nucleus. ~1 a.m.u. neutron. 0. in nucleus. ~1 a.m.u. electron. 1–. orbiting nucleus. ~0 a.m.u.

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Unit 3: Atomic Structure

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  1. Outline Chemistry Unit 3: Atomic Structure PowerPoint Presentation by Mr. John Bergmann

  2. Basics of the Atom Location in the Atom Charge Particle Mass proton 1+ in nucleus ~1 a.m.u. neutron 0 in nucleus ~1 a.m.u. electron 1– orbiting nucleus ~0 a.m.u. a.m.u.: unit used to measure mass of atoms

  3. 10 Ne 20.1797 atomic number: # of p+ -- the whole number on Periodic Table -- determines identity of atom mass number: (# of p+) + (# of n0) (It is NOT on “the Table.”) To find net charge on an atom, consider ____ and ____. e– p+

  4. + C ion.” A ion: a charged atom anion: a (–) ion cation: a (+) ion -- more e– than p+ -- more p+ than e– -- -- formed when atoms gain e– formed when atoms lose e– I think that a ions n are negative ions. “When I see a cation, I see a positive ion; that is, I…

  5. Net Charge Atomic Number Mass Number Ion Symbol Description 15 p+ 16 n0 18 e– 3– 31 15 P3– 38 p+ 50 n0 36 e– 2+ 38 88 Sr2+ 52 p+ 128 2– Te2– 52 76 n0 54 e– 19 p+ 19 1+ 39 20 n0 K1+ 18 e–

  6. different varieties of an element’s atoms Isotopes: -- have diff. #’s of n0; thus, diff. masses -- some are radioactive; others aren’t All atoms of an element react the same, chemically. Isotope p+ n0 Common Name Mass H–1 1 1 0 protium 2 deuterium H–2 1 1 3 tritium H–3 1 2 C–12 atoms C–14 atoms 6 p+ 6 p+ 6 n0 8 n0 stable radioactive

  7. Radioactive Isotopes: have too many or too few n0 Nucleus attempts to attain a lower energy state by releasing extra energy as __________. radiation e.g., a- or b-particles, g rays half-life: the time needed for ½ of a radioactive sample to decay into stable matter e.g., C–14: -- half-life is 5,730 years -- decays into stable N–14

  8. Say that a 120 g sample of C-14 is found today. = C–14 = N–14 Years from now g of C–14 present g of N–14 present 0 120 0 5,730 60 60 11,460 30 90 17,190 105 15 7.5 22,920 112.5

  9. mass # charge (if any) element symbol atomic # 125 1– I 53 iodine is now added to salt Goiter due to lack of iodine • Complete Atomic Designation …gives precise info about an atomic particle

  10. 238 U 92 23 1+ Na 11 79 2– Se 34 27 32 24 17 20 18 25 30 18 Complete Atomic Designation Protons Neutrons Electrons 92 146 92 11 12 10 34 45 36 59 3+ Co 27 37 1– Cl 17 55 7+ Mn 25

  11. Greek model of atom Historical Development of the Atomic Model Greeks (~400 B.C.E.) Democritus & Leucippus Matter is discontinuous (i.e., “grainy”).

  12. Hints at the Scientific Atom ** Antoine Lavoisier: law of conservation of mass ** Joseph Proust (1799): law of definite proportions: every compound has a fixed proportion e.g., water…………………….. 8 g O : 1 g H 13 g Cr : 4 g O chromium (II) oxide…….

  13. law of multiple proportions: When two different compounds have same two elements, equal mass of one element results in integer multiple of mass of other. e.g., water…………………….. hydrogen peroxide..……. chromium (II) oxide……. chromium (VI) oxide…… • Hints at the Scientific Atom (cont.) ** John Dalton (1803): 8 g O : 1 g H 2 16 g O : 1 g H 13 g Cr : 3 4 g O 13 g Cr : 12 g O

  14. Atoms are not indivisible. Isotopes! NaCl, H2O, NH3, Fe2O3, C6H12O6 John Dalton’s Atomic Theory (1808) 1. Elements are made of indivisible particles called atoms. 2. Atoms of the same element are exactly alike; in particular, they have the same mass. 3. Compounds are formed by the joining of atoms of two or more elements in fixed, whole number ratios. Dalton’s model of atom e.g., 1:1, 2:1, 1:3, 2:3, 1:2:1

  15. Maltese cross CRT computer monitor radar screen television ** William Crookes (1870s): Rays causing shadow were emitted from cathode.

  16. electric field lines “cathode rays” Crooke’s tube electrons phosphorescent screen • The Thomsons (~1900) J.J. Thomson discovered that “cathode rays” are… …deflected by electric and magnetic fields J.J. Thomson + + + + + + – – – – – – … (–) particles

  17. + + – + + – – + + + – – + – – – + – + + – – (plum pudding) William Thomson (a.k.a., Lord Kelvin): Since atom was known to be electrically neutral, he proposed the plum pudding model. Lord Kelvin -- Equal quantities of (+) and (–) charge distributed uniformly in atom. -- (+) is ~2000X more massive than (–) Thomson’s plum pudding model

  18. photo from liquid H2 bubble chamber ** James Chadwick discovered neutrons in 1932. -- n0 have no charge and are hard to detect -- purpose of n0 = stability of nucleus Chadwick And now we know of many other subatomic particles: quarks, muons, positrons, neutrinos, pions, etc.

  19. particle beam • Ernest Rutherford (1909) • Gold Leaf Experiment Beam of a-particles (+) directed at gold leaf surrounded by phosphorescent (ZnS) screen. gold leaf a-source lead block ZnS screen

  20. Most a-particles passed through, some angled slightly, and a tiny fraction bounced back. Conclusions: 1. Atom is mostly empty space. (+) particles are concentrated at center. 2. nucleus = “little nut” (–) particles orbit nucleus. 3.

  21. – – – – – + – + – + + – – – + + + – + – – + – – + – – + • Thomson’s Plum Pudding Model • Dalton’s (also the Greek) Model • Rutherford’s Model N

  22. only certain values are allowed  e– found here e– never found here • Recent Atomic Models Max Planck (1900): Proposed that amounts of energy are quantized Niels Bohr (1913): e– can possess only certain amounts of energy, and can therefore be only certain distances from nucleus. planetary (Bohr) model N

  23. Biology Experiment To conduct a biology experiment, you need 100 mL of cola per trial, and you plan to conduct 500 trials. If 1 can contains 355 mL of cola, and there are 24 cans in a case, and each case sells for $4.89, and there is 7.75% sales tax… A. How many cases must you buy? 6 cases B. How much will the cola cost? $31.61

  24. quantum mechanical model electron cloud model charge cloud model Schroedinger, Pauli, Heisenberg, Dirac (up to 1940): According to the QMM, we never know for certain where the e– are in an atom, but the equations of the QMM tell us the probability that we will find an electron at a certain distance from the nucleus.

  25. Ti has five naturally-occurring isotopes % abundance • Average Atomic Mass (Atomic Mass, AAM) This is the weighted average mass of all atoms of an element, measured in a.m.u. For an element with isotopes A, B, etc.: AAM = Mass A (% A) + Mass B (% B) + … (use the decimal form of the %; e.g., use 0.253 for 25.3%)

  26. 1 “average” atom 6.02 x 1023 atoms Lithium has two isotopes. Li-6 atoms have mass 6.015 amu; Li-7 atoms have mass 7.016 amu. Li-6 makes up 7.5% of all Li atoms. Find AAM of Li. Li batteries AAM = Mass A (% A) + Mass B (% B) AAM = 6.015 amu (0.075) + 7.016 amu (0.925) AAM = 0.451 amu + 6.490 amu AAM = 6.94 amu ** Decimal number on Table refers to… molar mass (in g) OR AAM (in amu).

  27. 0.031 0.031 % abundance Isotope Mass Si-28 27.98 amu 92.23% Si-29 28.98 amu 4.67% ? Si-30 3.10% AAM = MA (% A) + MB (% B) + MC (% C) 28.086 = 27.98 (0.9223) + 28.98 (0.0467) + X (0.031) 28.086 = 25.806 + 1.353 + 0.031X 28.086 = 27.159 + 0.031X 0.927 = 0.031X X = MSi-30 = 29.90 amu

  28. Electron Configurations “e– Jogging” Rules 1. Max. of two e– per jogging track (i.e., orbital). 2. Easier orbitals fill up first. s orbital (level) p orbital (rolling hills) d orbital (steep hills) 3. e– must go 100X around. 4. All orbitals of equal difficulty must have one e– before any doubling up. 5. e– on same orbital must go opposite ways.

  29. 3s orbital 3p orbitals 2p orbitals (1 of these, 2 e–) (3 of these, 6 e–) (3 of these, 6 e–) 2s orbital (1 of these, 2 e–) 4s orbital (1 of these, 2 e–) 3d orbitals (5 of these, 10 e–) 1s orbital 4p orbitals (1 of these, 2 e–) (3 of these, 6 e–) 4s2 2s2 2p6 3s2 3d10 4p6… 3p6 1s2 3,4 5-10 11,12 31-36 1,2 21-30 13-18 19,20

  30. Writing Electron Configurations: Where are the e–? (probably) 1s1 H He 1s2 Li 1s2 2s1 2p3 1s2 2s2 N 2s2 2p6 3s2 3p1 1s2 Al 4s2 2s2 2p6 3s2 3d2 Ti 3p6 1s2 4s2 As 4p3 2s2 2p6 3s2 3d10 3p6 1s2 5s2 4s2 Xe 5p6 4d10 4p6 2s2 2p6 3s2 3d10 3p6 1s2 4s2 2s2 2p6 3s2 3d10 4p6… 3p6 1s2

  31. Sections of Periodic Table to Know s-block p-block d-block f-block

  32. Friedrich Hund Wolfgang Pauli • Three Principles about Electrons 3d10… 4s2 Aufbau Principle: 3p6 e– will take lowest-energy orbital available 3s2 2p6 2s2 1s2 Hund’s Rule: for equal-energy orbitals, each must have one e– before any take a second Pauli Exclusion Principle: two e– in same orbital have different spins

  33. Orbital Diagrams …show spins of e– and which orbital each is in O 3p 2p 3s 2s 1s P 3p 2p 3s 2s 1s

  34. Shorthand Electron Configuration (S.E.C.) To write S.E.C. for an element: 1. Put symbol of noble gas that precedes element in brackets. 2. Continue writing e– config. from that point. [ Ne ] S 3s2 3p4 [ Ar ] 4s2 3d7 Co [ Kr ] 5s2 4d10 5p3 In [ Ne ] 3s2 3p5 Cl [ Kr ] 5s1 Rb

  35. coefficient superscript • The Importance of Electrons In “jogging tracks” analogy, the tracks represent orbitals: regions of space where an e– may be found In a generic e– config (e.g., 1s2 2s2 2p6 3s2 3p6…): # of energy level # of e– in those orbitals In general, as energy level # increases, e–… HAVE MORE ENERGY ARE FARTHER FROM NUCLEUS AND

  36. valence electrons: kernel electrons: in inner energy level(s); close to nucleus in outer energy level INVOLVED IN CHEMICAL BONDING 1s2 (2 v.e–) He: [ He ] 2s2 2p6 Ne: (8 v.e–) [ Ne ] 3s2 3p6 Ar: (8 v.e–) Kr: [ Ar ] 4s2 3d10 4p6 (8 v.e–) Noble gas atoms have FULL valence shells. They are stable, low-energy, and unreactive.

  37. chlorine atom, Cl 17 p+, 17 e– How to be like a noble gas…? F1– Cl1– Other atoms “want” to be like noble gas atoms. ** They give away or acquire e–. octet rule: the tendency for atoms to “want” 8 e– in the valence shell -- doesn’t apply to He, Li, Be, B (which want 2) or to H (which wants either 0 or 2) fluorine atom, F 9 p+, 9 e– steal 1 e– steal 1 e– 9 p+, 10 e– 17 p+, 18 e– F atom would rather be F1– ion. Cl atom would rather be Cl1– ion.

  38. How to be like a noble gas…? Li1+ Na1+ lithium atom, Li sodium atom, Na 3 p+, 3 e– 11 p+, 11 e– lose 1 e– lose 1 e– 3 p+, 2 e– 11 p+, 10 e– Li atom would rather be Li1+ ion. Na atom would rather be Na1+ ion.

  39. Know charges on these columns of Table: 1+ Group 1: Group 2: Group 13: Group 15: Group 16: Group 17: Group 18: 2+ 3+ 3– 2– 1+ 0 1– 3+ 2+ 3– 2– 1– 0

  40. Cations use element name and then say “ion” Anions change ending of element name to “ide” and then say “ion” Naming Ions e.g., Ca2+ calcium ion Cs1+ cesium ion Al3+ aluminum ion e.g., S2– sulfide ion P3– phosphide ion N3– nitride ion O2– oxide ion Cl1– chloride ion

  41. ENERGY (HEAT, LIGHT, ELEC., ETC.) • Light When all e– are in lowest possible energy state, an atom is in the ____________. ground state He: 1s2 e.g., If “right” amount of energy is absorbed by an e–, it can “jump” to a higher energy level. This is an unstable, momentary condition called the ____________. excited state e.g., He: 1s1 2s1

  42. EMITTED LIGHT When e– falls back to a lower-energy, more stable orbital (it might be the orbital it started out in, but it might not), atom releases the “right” amount of energy as light. Any-old-value of energy to be absorbed or released is NOT OK. This explains the lines of color in an emission spectrum.

  43. H discharge tube, with power supply and spectroscope Emission Spectrum for a Hydrogen Atom Lyman series: e– falls to 1st energy level Balmer series: e– falls to 2nd energy level Paschen series: e– falls to 3rd energy level typical emission spectrum

  44. Paschen Lyman Balmer (IR) (UV) (visible) 6TH E.L. 5TH E.L. 4TH E.L. ~ ~ ~ ~ ~ ~ 3RD E.L. 2ND E.L. 1ST E.L.

  45. Resources - Atomic Structure Objectives Worksheet - vocabulary Worksheet - development of atomic theory Worksheet - atomic number and mass number Worksheet - ions and subatomic particles Lab - isotopes Worksheet - orbital diagrams Worksheet - electron configuration Episode 6 - Atom Worksheet - light problems Worksheet - half-life Textbook - questions Outline(general)

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