Presentation is loading. Please wait.

Presentation is loading. Please wait.

1 Electromagnetic Radiation and Energy Electromagnetic Radiation: –Energy traveling through space Three Characteristics of Waves: 1.Wavelength: (symbolized.

Similar presentations


Presentation on theme: "1 Electromagnetic Radiation and Energy Electromagnetic Radiation: –Energy traveling through space Three Characteristics of Waves: 1.Wavelength: (symbolized."— Presentation transcript:

1 1 Electromagnetic Radiation and Energy Electromagnetic Radiation: –Energy traveling through space Three Characteristics of Waves: 1.Wavelength: (symbolized  1.Distance between two consecutive peaks or troughs in a wave 2.Frequency: (symbolized  1.How many waves pass a given point per second 3.Speed: (symbolized c) 1.How fast a given peak moves through space

2 2

3 3 Electromagnetic Radiation and Energy c = λ x ν c = speed of light = 2.9979 x 10 8 m/s ν = frequency (s -1 or Hz) λ = wavelength (m)

4 4

5 5 Spectra Sunlight yields continuous spectrum Energized gaseous elements yield certain wavelengths –Line emission spectrum

6 6 Rydberg Why did gaseous atoms emit certain wavelengths? –Didn’t find out why, but came up with an equation Rydberg equation –N=3, red line –N=4, green line –N=5, blue line Lyman series –n > 1 to n = 1 UV (invisible) Balmer series –n > 2 to n = 2 Visible wavelengths

7 7 The Bohr Model of the Atom Explained Rydberg Electron energy quantized –Electron only occupies certain energy levels or orbitals If it didn’t, electron would crash into protons in nucleus As “n” increases energy becomes less negative –Increases Only certain amts of E may be absorbed/emitted If electron in lowest possible energy level –Ground state If electron in excited energy level –Excited state One can calculate energy needed to raise H electron per atom from ground state (n=1) to first excited state (n=2)

8 8 Bohr’s Model Explains emission spectrum of H –Movement of electrons from one quantized energy level to a lower one gave distinct emission wavelengths Model only good for one electron system

9 9 Atomic orbital The probability function that defines the distribution of electron density in space around the atomic nucleus.

10 10 The s-orbital The simplest orbital The only orbital in the s-subshell Occurs in every principal energy level “s” stands for “sharp” The first energy level only houses this orbital Can house up to 2 electrons

11 11 The p-orbitals Start in second principle energy level (n=2) There are three p-orbitals in the p-subshell (see below) –And one s-orbital “p” stands for “principle” Can house up to 6 electrons Has one nodal surface –Nodal plane = a planar surface in which there’s zero probability of find an electron 2p x 2p y 2p z

12 12 The d-orbitals Start in third principle energy level (n=3) There are five d-orbitals in the d-subshell –And one s-orbital –And three p-orbitals Can house up to 10 electrons “d” stands for “diffuse” Has two nodal surfaces 3d yz 3d xz 3d xy 3d x 2 -y 2 3d z 2

13 13 The f-orbitals Start in fourth principle energy level (n=4) There are seven f-orbitals in the f-subshell –And one s-orbital –And three p-orbitals –And five d-orbitals Can house up to 14 electrons “f” stands for “fundamental” Has 3 nodal surfaces

14 14 Electron configuration Electron must be identified as to where it is located –Hydrogen: One electron in first energy level and s-subshell –Thus, 1s 1 (= Aufbau electron configuration) 1 states energy level (n) s designates subshell Superscript 1 tells how many electrons are in the s- subshell Can also use orbital box or line diagrams –Let’s take a look

15 15 Pauli Exclusion Principle An atomic orbital holds a maximum of two electrons Both electrons must have opposite spins m s = +1/2 & -1/2

16 16 Hund’s Rule Electron configuration most stable with electrons in half-filled orbitals before coupling

17 17 Subshell filling order – not what one expected

18 18 Using the Periodic Table to advantage

19 19 Short-hand vs. long-hand Aufbau electron configuration F Al Ca Br

20 20 Exercises Give me the Aufbau electron configurations for: –Y –Te –Hf –Tl –112

21 21 Sundry matters pertaining to d-block metals Stability is increased when: –d-subshell is half-filled (d 5 ) –d-subshell is completely filled (d 10 ) Electrons will be taken from the s-subshell to fill the d- subshell –But there is a limit No more than 2 electrons taken from s-subshell Given the above, which subshell electrons will d-block metals lose first when they ionize? So what are the correct electron configurations of Cr and Ag? Caveat –Not all metals follow the above; i.e., take from s-subshell and give to d- subshell Ni & Pt, for example

22 22 Sundry matters pertaining to f-block metals Stability is increased when: –f-subshell is half-filled (f 7 ) –f-subshell is completely filled (f 14 ) Electron will be taken from the d-subshell to fill the f-subshell –Eu & Yb –Am & No


Download ppt "1 Electromagnetic Radiation and Energy Electromagnetic Radiation: –Energy traveling through space Three Characteristics of Waves: 1.Wavelength: (symbolized."

Similar presentations


Ads by Google