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Test II Hi Lo Average: Curve Raw grades: 92 9 37.3 25 pt. Grades (curved) are posted on BlazeVIEW Look at tests/ask questions after class or Wednesday 9 – 1pm (in my office) Analysis/solutions session can be scheduled if there is interest (email [email protected]) © 2009 Brooks/Cole - Cengage 1 2 Midterm Grades Based only on Test 1 (75.7%) and OWL (24.2%) The last day to drop without academic penalty: March 3d, by 11:59 pm; limited to five withdrawals per college life © 2009 Brooks/Cole - Cengage 3 Chem 1211 Class 13 Atomic Structure Chapter 6 © 2009 Brooks/Cole - Cengage 4 Atomic Line Spectra and Niels Bohr Niels Bohr (1885-1962) © 2009 Brooks/Cole - Cengage Bohr’s theory was a great accomplishment. Rec’d Nobel Prize, 1922 Problems with theory — • theory only successful for H. • introduced quantum idea artificially. • So, we go on to QUANTUM or WAVE MECHANICS 5 Quantum or Wave Mechanics L. de Broglie (1892-1987) © 2009 Brooks/Cole - Cengage de Broglie (1924) proposed that all moving objects have wave properties. For light: E = mc2 E = h = hc / Therefore, mc = h / and for particles (mass)(velocity) = h / 6 Quantum or Wave Mechanics Baseball (115 g) at 100 mph = 1.3 x 10-32 cm PLAY MOVIE Experimental proof of wave properties of electrons © 2009 Brooks/Cole - Cengage e- with velocity = 1.9 x 108 cm/sec = 3.88 x 10-10 m = 0.388 nm Uncertainty Principle W. Heisenberg 1901-1976 © 2009 Brooks/Cole - Cengage Problem of defining nature of electrons in atoms solved by W. Heisenberg. Cannot simultaneously define the position and momentum (= m•v) of an electron. We define e- energy exactly but accept limitation that we do not know exact position. 7 Quantum or Wave Mechanics 8 Schrodinger applied idea of ebehaving as a wave to the problem of electrons in atoms. He developed the WAVE EQUATION Solution gives set of math expressions called WAVE FUNCTIONS, (psi) E. Schrodinger Each describes an allowed energy 1887-1961 state of an eQuantization introduced naturally. © 2009 Brooks/Cole - Cengage WAVE FUNCTIONS, • is a function of distance and two angles. • Each corresponds to an ORBITAL — the region of space within which an electron is found. • does NOT describe the exact location of the electron. • 2 is proportional to the probability of finding an e- at a given point. There is a set of numbers that are parameters of : they are called quantum numbers © 2009 Brooks/Cole - Cengage 9 QUANTUM NUMBERS The shape, size, and energy of each orbital is a function of 3 quantum numbers: n (principal) → shell l (angular) → subshell ml (magnetic) → designates an orbital within a subshell According to that numbers, electrons in atom grouped in shells and subshells © 2009 Brooks/Cole - Cengage 10 11 Subshells & Shells • Subshells grouped in shells. • Each shell has a number called the PRINCIPAL QUANTUM NUMBER, n • The principal quantum number of the shell is the number of the period or row of the periodic table where that shell begins. © 2009 Brooks/Cole - Cengage 12 Subshells & Shells n=1 n=2 n=3 n=4 © 2009 Brooks/Cole - Cengage 13 Types of Orbitals s orbital © 2009 Brooks/Cole - Cengage p orbital d orbital Orbitals 14 • No more than 2 e- assigned to an orbital • Orbitals grouped in s, p, d (and f) subshells s orbitals d orbitals © 2009 Brooks/Cole - Cengage p orbitals 15 s orbitals p orbitals d orbitals s orbitals p orbitals No. orbs. 1 3 5 No. e- 2 6 10 © 2009 Brooks/Cole - Cengage d orbitals 16 QUANTUM NUMBERS Symbol Values Description n (major) 1, 2, 3, .. l (angular) 0, 1, 2, .. n-1 ml (magnetic) -l..0..+l Orbital size and energy where E = -R(1/n2) Orbital shape or type (subshell) Orbital orientation # of orbitals in subshell = 2l © 2009 Brooks/Cole - Cengage +1 17 Types of Atomic Orbitals See Active Figure 6.14 © 2009 Brooks/Cole - Cengage Shells and Subshells When n = 1, then l = 0 and ml = 0 Therefore, in n = 1, there is 1 type of subshell and that subshell has a single orbital (ml has a single value → 1 orbital) This subshell is labeled s (“ess”) Each shell has 1 orbital labeled s, and it is SPHERICAL in shape. © 2009 Brooks/Cole - Cengage 18 s Orbitals— Always Spherical Dot picture of electron cloud in 1s orbital. Surface density 4πr2y versus distance See Active Figure 6.13 © 2009 Brooks/Cole - Cengage Surface of 90% probability sphere 19 1s Orbital © 2009 Brooks/Cole - Cengage 20 2s Orbital © 2009 Brooks/Cole - Cengage 21 3s Orbital © 2009 Brooks/Cole - Cengage 22 p Orbitals 23 When n = 2, then l = 0 and 1 Therefore, in n = 2 shell there are 2 types of orbitals — 2 subshells For l = 0 ml = 0 this is a s subshell For l = 1 ml = -1, 0, +1 this is a p subshell with 3 orbitals See Screen 6.15 © 2009 Brooks/Cole - Cengage When l = 1, there is a PLANAR NODE thru the nucleus. p Orbitals The three p orbitals lie 90o apart in space © 2009 Brooks/Cole - Cengage 24 25 2px Orbital © 2009 Brooks/Cole - Cengage 3px Orbital d Orbitals When n = 3, what are the values of s? l = 0, 1, 2 and so there are 3 subshells in the shell. For l = 0, ml = 0 → s subshell with single orbital For l = 1, ml = -1, 0, +1 → p subshell with 3 orbitals For l = 2, m l = -2, -1, 0, +1, +2 →d © 2009 Brooks/Cole - Cengage subshell with 5 orbitals 26 27 d Orbitals s orbitals have no planar node (l = 0) and so are spherical. p orbitals have l = 1, and have 1 planar node, and so are “dumbbell” shaped. This means d orbitals (with l = 2) have 2 planar nodes See Figure 6.15 © 2009 Brooks/Cole - Cengage 28 3dxy Orbital © 2009 Brooks/Cole - Cengage 29 3dxz Orbital © 2009 Brooks/Cole - Cengage 30 3dyz Orbital © 2009 Brooks/Cole - Cengage 31 2 2 3dx - y © 2009 Brooks/Cole - Cengage Orbital 32 2 3dz Orbital © 2009 Brooks/Cole - Cengage f Orbitals When n = 4, l = 0, 1, 2, 3 so there are 4 subshells in the shell. For l = 0, ml = 0 → s subshell with single orbital For l = 1, ml = -1, 0, +1 → p subshell with 3 orbitals For l = 2, ml = -2, -1, 0, +1, +2 → d subshell with 5 orbitals For l = 3, ml = -3, -2, -1, 0, +1, +2, +3 → f subshell with 7 orbitals © 2009 Brooks/Cole - Cengage 33 34 f Orbitals One of 7 possible f orbitals. All have 3 planar nodal surfaces. Can you find the 3 surfaces here? © 2009 Brooks/Cole - Cengage Spherical Nodes 2 s orbital •Orbitals also have spherical nodes •Number of spherical nodes =n-l-1 •For a 2s orbital: No. of nodes = 2 - 0 - 1 = 1 © 2009 Brooks/Cole - Cengage 35 Arrangement of Electrons in Atoms Electrons in atoms are arranged as SHELLS (n) SUBSHELLS (l) ORBITALS (ml) © 2009 Brooks/Cole - Cengage 36