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Chapter 14 Chemical Periodicity

Chapter 14 Chemical Periodicity. Charles Page High School Dr. Stephen L. Cotton. Section 14.1 Classification of the Elements. OBJECTIVES: Explain why you can infer the properties of an element based on those of other elements in the periodic table. Section 14.1 Classification of the Elements.

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Chapter 14 Chemical Periodicity

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  1. Chapter 14Chemical Periodicity Charles Page High School Dr. Stephen L. Cotton

  2. Section 14.1Classification of the Elements • OBJECTIVES: • Explain why you can infer the properties of an element based on those of other elements in the periodic table.

  3. Section 14.1Classification of the Elements • OBJECTIVES: • Use electron configurations to classify elements as noble gases, representative elements, transition metals, or inner transition metals.

  4. Periodic Table Revisited • Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. • Mid 1800’s - molar masses of elements were known. • Wrote down the elements in order of increasing mass. • Found a pattern of repeating properties.

  5. Mendeleev’s Table • Grouped elements in columns by similar properties in order of increasing atomic mass. • Found some inconsistencies - felt that the properties were more important than the mass, so switched order. • Also found some gaps. • Must be undiscovered elements. • Predicted their properties before they were found.

  6. The modern table • Elements are still grouped by properties. • Similar properties are in the same column. • Order is by increasing atomic number. • Added a column of elements Mendeleev didn’t know about. • The noble gases weren’t found because they didn’t react with anything.

  7. Horizontal rows are called periods • There are 7 periods

  8. Vertical columns called groups Elements are placed in columns by similar properties Also called families

  9. 8A0 1A • The elements in the A groups are called the representative elements outer s or p filling 2A 3A 4A 5A 6A 7A

  10. These are called the inner transition elements, and they belong here The group B are called the transition elements

  11. Group 1A are the alkali metals • Group 2A are the alkaline earth metals

  12. Group 7A is called the Halogens • Group 8A are the noble gases

  13. Why? • The part of the atom another atom sees is the electron cloud. • More importantly the outside orbitals. • The orbitals fill up in a regular pattern. • The outside orbital electron configuration repeats. • The properties of atoms repeat.

  14. H 1 Li 3 Na 11 K 19 Rb 37 Cs 55 Fr 87 1s1 1s22s1 1s22s22p63s1 1s22s22p63s23p64s1 1s22s22p63s23p64s23d104p65s1 1s22s22p63s23p64s23d104p65s24d10 5p66s1 1s22s22p63s23p64s23d104p65s24d105p66s24f145d106p67s1

  15. He 2 1s2 1s22s22p6 1s22s22p63s23p6 1s22s22p63s23p64s23d104p6 1s22s22p63s23p64s23d104p65s24d105p6 1s22s22p63s23p64s23d104p65s24d10 5p66s24f145d106p6 Ne 10 Ar 18 Kr 36 Xe 54 Rn 86

  16. S- block s1 • Alkali metals all end in s1 • Alkaline earth metals all end in s2 • really should include He, but it fits better later. • He has the properties of the noble gases. s2

  17. Transition Metals -d block s1 d5 s1 d10 d1 d2 d3 d5 d6 d7 d8 d10

  18. The P-block p1 p2 p6 p3 p4 p5

  19. f6 f13 f1 f2 f3 f4 f5 f7 f8 f10 f12 f14 f11 f9 F - block • inner transition elements

  20. 1 2 3 4 5 6 7 • Each row (or period) is the energy level for s and p orbitals.

  21. d orbitals fill up after previous energy level, so first d is 3d even though it’s in row 4. 1 2 3 4 5 6 7 3d

  22. 1 2 3 4 5 6 7 • f orbitals start filling at 4f 4f 5f

  23. Summary: Fig. 14.5, p. 395Sample Problem 14-1, p.396

  24. Writing electron configurations the easy way Yes there is a shorthand

  25. Electron Configurations repeat • The shape of the periodic table is a representation of this repetition. • When we get to the end of the column the outermost energy level is full. • This is the basis for our shorthand.

  26. The Shorthand • Write symbol of the noble gas before the element, in [ ]. • Then, the rest of the electrons. • Aluminum’s full configuration: 1s22s22p63s23p1 • previous noble gas Ne is: 1s22s22p6 • so, Al is: [Ne] 3s23p1

  27. More examples • Ge = 1s22s22p63s23p64s23d104p2 • Thus, Ge = [Ar] 4s23d104p2 • Hf = 1s22s22p63s23p64s23d104p65s2 4d105p66s24f145d2 • Thus, Hf = [Xe]6s24f145d2

  28. The Shorthand Again Sn- 50 electrons The noble gas before it is Kr Takes care of 36 Next 5s2 Then 4d10 Finally 5p2 [ Kr ] 5s2 4d10 5p2

  29. Section 14.2Periodic Trends • OBJECTIVES: • Interpret group trends in atomic radii, ionic radii, ionization energies, and electronegativities.

  30. Section 14.2Periodic Trends • OBJECTIVES: • Interpret period trends in atomic radii, ionic radii, ionization energies, and electronegativities.

  31. Trends in Atomic Size • First problem: Where do you start measuring from? • The electron cloud doesn’t have a definite edge. • They get around this by measuring more than 1 atom at a time.

  32. Atomic Size } • Atomic Radius = half the distance between two nuclei of a diatomic molecule. Radius

  33. Trends in Atomic Size • Influenced by three factors: 1. Energy Level • Higher energy level is further away. 2. Charge on nucleus • More charge pulls electrons in closer. • 3. Shielding effect (blocking effect?)

  34. Group trends H • As we go down a group... • each atom has another energy level, • so the atoms get bigger. Li Na K Rb

  35. Periodic Trends • As you go across a period, the radius gets smaller. • Electrons are in same energy level. • More nuclear charge. • Outermost electrons are closer. Na Mg Al Si P S Cl Ar

  36. Rb Overall K Na Li Atomic Radius (nm) Kr Ar Ne H Atomic Number 10

  37. Trends in Ionization Energy • The amount of energy required to completely remove an electron from a gaseous atom. • Removing one electron makes a 1+ ion. • The energy required to remove the first electron is called the first ionization energy.

  38. Ionization Energy • The second ionization energy is the energy required to remove the second electron. • Always greater than first IE. • The third IE is the energy required to remove a third electron. • Greater than 1st or 2nd IE.

  39. Table 14.1, p. 402 Symbol First Second Third 5247 7297 1757 2430 2352 2857 3391 3375 3963 1312 2731 520 900 800 1086 1402 1314 1681 2080 HHeLiBeBCNO F Ne 11810 14840 3569 4619 4577 5301 6045 6276

  40. Symbol First Second Third 11810 14840 3569 4619 4577 5301 6045 6276 5247 7297 1757 2430 2352 2857 3391 3375 3963 1312 2731 520 900 800 1086 1402 1314 1681 2080 HHeLiBeBCNO F Ne

  41. What determines IE • The greater the nuclear charge, the greater IE. • Greater distance from nucleus decreases IE • Filled and half-filled orbitals have lower energy, so achieving them is easier, lower IE. • Shielding effect

  42. Shielding • The electron on the outermost energy level has to look through all the other energy levels to see the nucleus. • Second electron has same shielding, if it is in the same period

  43. Group trends • As you go down a group, first IE decreases because... • The electron is further away. • More shielding.

  44. Periodic trends • All the atoms in the same period have the same energy level. • Same shielding. • But, increasing nuclear charge • So IE generally increases from left to right. • Exceptions at full and 1/2 full orbitals.

  45. He • He has a greater IE than H. • same shielding • greater nuclear charge H First Ionization energy Atomic number

  46. He • Li has lower IE than H • more shielding • further away • outweighs greater nuclear charge H First Ionization energy Li Atomic number

  47. He • Be has higher IE than Li • same shielding • greater nuclear charge H First Ionization energy Be Li Atomic number

  48. He • B has lower IE than Be • same shielding • greater nuclear charge • By removing an electron we make s orbital half-filled H First Ionization energy Be B Li Atomic number

  49. He C H First Ionization energy Be B Li Atomic number

  50. He N C H First Ionization energy Be B Li Atomic number

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