What is Light? electromagnetic radiation • a form of energy • travels in waves • exists in increments called photons (a packet of light) Revell Introductory Chemistry, © 2018 Macmillan Learning Electromagnetic radiation ranges from very low energy waves (TV and radio waves) to very high energy waves (X-rays and gamma rays). This broad continuum of electromagnetic energy is referred to as the electromagnetic spectrum. In the middle of this spectrum is a small range of radiation that our eyes can detect, and that we perceive as visible light. This narrow range of radiation is the visible spectrum. If we look more closely at the visible spectrum, we can see that it is made up of the colors of the rainbow: red, orange, yellow, green, blue, and violet. Revell Introductory Chemistry, © 2018 Macmillan Learning Types of Electromagnetic Radiation • Classified by the Wavelength – Radiowaves = l > 0.01 m. • Low frequency and energy. – Microwaves = 10-4m < l < 10-2 m. – Infrared (IR) = 8 x 10-7 < l < 10-5 m. – Visible = 4 x 10-7 < l < 8 x 10-7 m. • ROYGBIV. – Ultraviolet (UV) = 10-8 < l < 4 x 10-7 m. – X-rays = 10-10 < l < 10-8 m. – Gamma rays = l < 10-10. • High frequency and energy. 4 Revell Introductory Chemistry, © 2018 Macmillan Learning Describing Electromagnetic Waves amplitude – The height of one wave wavelength (λ) – The length of one wave (nm length) frequency (ν) – The number of waves per second 1 wave/second = 1 hertz (Hz) 10,000 Hz IR Revell Introductory Chemistry, © 2018 Macmillan Learning 10,000/s 10,000 s-1 UV Describing Electromagnetic Waves Wavelength and the frequency are inversely related to each other. This means that as the wavelength decreases, the frequency increases, and vice versa. wavelength frequency inversely related c = ln speed of light = wavelength x frequency m s = m x 1 s c = speed of light = 3.00 x 108 m/s Revell Introductory Chemistry, © 2018 Macmillan Learning A beam of green light has a wavelength of 500 nm. What is the frequency of this light? c = ln c = 3.00 x 108 m/s l = 500 nm = 500 x 10-9 m 1 nm = 10-9 m n = ? c = n l 3.00 x 108 m/s 500 x 10-9 m = n units: 1/s = Hz 6 x 1014 Hz = Revell Introductory Chemistry, © 2018 Macmillan Learning n Tro's "Introductory Chemistry", Chapter 9 Revell Introductory Chemistry, © 2018 Macmillan Learning 8 The energy of light depends on its frequency and wavelength. longer wavelength lower frequency lower energy shorter wavelength higher frequency higher energy Revell Introductory Chemistry, © 2018 Macmillan Learning Energy of a photon: akg-images / bilwissediti We can relate the energy of a single photon to the frequency using the relationship E = h nu, where E is the energy (measured in Joules), nu is the frequency, and h is Planck’s constant, which has a value of 6.63 x 10-34 Jˑs. E = hν energy frequency Planck’s constant = 6.63 x 10-34 J.s ν = c/ l This constant is named after Max Planck, a German physicist who was instrumental in developing the theories that relate light, energy, and electron structure. E = hc/l Revell Introductory Chemistry, © 2018 Macmillan Learning A photon has a frequency of 7.50 x 1014 Hz. What is the wavelength of this light? What color is this light? What is the energy of the photon? c = ln c n = l 3.00 x 108 m/s = 14 7.50 x 10 /s 4.00 x 10-7 m = = 400 nm E = hn l E = (6.63 x 10-34 J.s)(7.50 x 1014/s) l violet E = 4.97 x 10-19 J Revell Introductory Chemistry, © 2018 Macmillan Learning Summary • Light is a form of electromagnetic radiation • We describe light by its • frequency (n) • wavelength (l) • energy (E) • c = ln • E = hn = hc/l Revell Introductory Chemistry, © 2018 Macmillan Learning Color, Line Spectra, and the Bohr Model Lets explore the relationship between light and electronic structure. Fireworks: The explosive powder in fireworks often contains metals that produce distinctive colors as the mixture burns. (c) anterovium / depositphotos.com Revell Introductory Chemistry, © 2018 Macmillan Learning The Electromagnetic Spectrum • Light passed through a prism is separated into all its colors. This is called a continuous spectrum. • The color of the light is determined by its wavelength. 14 Revell Introductory Chemistry, © 2018 Macmillan Learning Color • The color of light is determined by its wavelength. – Or frequency. • White light is a mixture of all the colors of visible light. – A spectrum ROYGBIV – Red Orange Yellow Green Blue Indigo Violet. • When an object absorbs some of the wavelengths of white light while reflecting others, it appears colored. – The observed color is predominantly the colors reflected. Tro's "Introductory Chemistry", Chapter 9 Revell Introductory Chemistry, © 2018 Macmillan Learning 15 Flame tests observe colors emitted by different metal ions A wire is dipped in a solution containing metal ions. The ions give off a characteristic color when heated. For example, when a wire is dipped in a solution containing calcium, the flame burns bright orange. When dipped in a solution of copper, the flame burns bright green. Photo credits: GIPhotoStock/Science Source Revell Introductory Chemistry, © 2018 Macmillan Learning Gas lamps also produce unique colors: We see a similar effect in gas lamps, like those used in neon signs. These lamps produce light by passing an electric current through a tube filled with a gas such as helium, neon, argon, krypton, or xenon. Richard Megna / Fundamental Photographs Like the metals in a flame test, each gas in a lamp produces a characteristic color. Revell Introductory Chemistry, © 2018 Macmillan Learning Emission Spectrum Unique to each element; only certain wavelengths of light are given off. 18 Revell Introductory Chemistry, © 2018 Macmillan Learning Each element produces a unique line spectrum. He Li Kr Scientists often use line spectra as “fingerprints” to identify elements. For example, analyzing light from the sun shows fine lines that correspond to the spectral lines of hydrogen and helium. From this, they know that the sun and other stars are composed largely of these two elements, Revell Introductory Chemistry, © 2018 Macmillan Learning Revell Introductory Chemistry, © 2018 Macmillan Learning Early 20th Century: • Dense nucleus surrounded by electrons • Photoelectric effect: light causes atoms to eject electrons This effect showed that light energy was somehow connected to electron structure. But how did this relate to the line spectra? Revell Introductory Chemistry, © 2018 Macmillan Learning The Bohr Model (1913) • • • • Electrons orbit the nucleus. Only certain orbit energies are “allowed”. Electrons can jump between levels. Light is absorbed or released when electrons jump. • Ground state: all electrons in lowest possible levels. Revell Introductory Chemistry, © 2018 Macmillan Learning • To help think about the Bohr model, imagine standing on a staircase. • You can jump from one step to another, but you can’t hover between steps – you will always land on one of the steps. • Similarly, electrons only occupy specified energy “steps”. • Electrons can absorb energy to move to a higher level (step), or release energy to move to a lower level. Revell Introductory Chemistry, © 2018 Macmillan Learning releases energy (blue light) • When the atom gains energy, the electron leaps from a lower energy orbit to one that is further from the nucleus. – However, during that “quantum leap” it doesn’t travel through the space between the orbits, it just disappears from the lower orbit and appears in the higher orbit. releases energy (UV light) absorbs energy - • When the electron leaps from a higher energy orbit to one that is closer to the nucleus, energy is emitted from the atom as a photon of light—a quantum of energy. Revell Introductory Chemistry, © 2018 Macmillan Learning In a H atom, four transitions produce visible light, resulting in four spectral lines. Notice that the smallest transition produces the lowest energy light (red), while the biggest transition produces the highest energy light (purple). Other transitions also take place, but they produce radiation that is either too high in energy (ultraviolet) or too low in energy (infrared) for our eyes to detect. Revell Introductory Chemistry, © 2018 Macmillan Learning Bohr Model Explained • The hydrogen line spectrum (Framework of electron structure) • Some properties of main group elements Did not explain • More complex line spectra (Elements larger than hydrogen) • Properties of the transition elements Revell Introductory Chemistry, © 2018 Macmillan Learning The Quantum Model and Electron Orbitals Bohr Model: 1913 • Erwin Schrödinger applied the Quantum Model: mathematics of probability and 1920s-30s the ideas of quantizing energy to the physics equations that describe waves, resulting in an equation that predicts the probability of finding an electron with a particular amount of energy at a particular location in the atom. Revell Introductory Chemistry, © 2018 Macmillan Learning Heisenberg’s Uncertainty Principle It is impossible to precisely know the exact velocity and location of a particle. • The result is a map of regions in the atom that have a particular probability for finding the electron. • An orbital is a region where we have a very high probability of finding the electron when it has a particular amount of energy. – Generally set at 90 or 95%. Quantum mechanics: describes electrons most probable locations energies Photo credits: Ted Kinsman/Science Source Revell Introductory Chemistry, © 2018 Macmillan Learning The wave nature of electrons Tiny, fast-moving particles also behave as waves. Ted Kinsman/Science Source This explains electron energy levels. ? Revell Introductory Chemistry, © 2018 Macmillan Learning The Quantum Model Main Ideas: • uncertainty principle • wave nature of electrons QM describes electrons by • energy • probable locations Revell Introductory Chemistry, © 2018 Macmillan Learning Energy Levels and Sublevels 1. Electrons occupy different energy levels. • Level is identified by its principal quantum number, n (1, 2, 3…) • Higher energy levels can hold more electrons Level 1 2 3 4 Revell Introductory Chemistry, © 2018 Macmillan Learning Electron Capacity 2 8 18 32 Energy Levels and Sublevels 2. Each energy level contains one or more sublevels. Sublevel s p d f Revell Introductory Chemistry, © 2018 Macmillan Learning Energy Levels and Sublevels 3. Each sublevel contains one or more orbitals. Orbital: a region where electrons are most likely to be found. Sublevel s p d f Number of Orbitals 1 3 5 7 Revell Introductory Chemistry, © 2018 Macmillan Learning Orbits: Bohr model describes the pathways of the particles orbiting the nucleus. Orbitals: describes the region around the atom where the electron is most likely to be. Revell Introductory Chemistry, © 2018 Macmillan Learning Revell Introductory Chemistry, © 2018 Macmillan Learning Energy Levels and Sublevels 4. Each orbital holds up to two electrons. – Electrons have a magnetic field, called spin. – Electrons with opposite spins pair together. Revell Introductory Chemistry, © 2018 Macmillan Learning Energy Levels and Sublevels 1. 2. 3. 4. Electrons occupy different energy levels. Each level contains sublevels. Each sublevel contains orbitals. Each orbital holds up to two electrons. Sublevel Number of Orbitals Electron Capacity s p d f 1 3 5 7 2 6 10 14 Revell Introductory Chemistry, © 2018 Macmillan Learning Level 1: s only Revell Introductory Chemistry, © 2018 Macmillan Learning Level 2: s + p As you go to higher levels, the orbitals INCREASE in size. A 1s orbital is smaller than a 2s orbital is Revell Introductory Chemistry, © 2018 Macmillan Learning Level 2: s + p x Revell Introductory Chemistry, © 2018 Macmillan Learning Level 2: s + p Sublevel s p Number of Orbitals 1 3 Total: Revell Introductory Chemistry, © 2018 Macmillan Learning Electron Capacity 2 6 8 Level 3: s + p + d Revell Introductory Chemistry, © 2018 Macmillan Learning Level 3: s + p + d Sublevel s p d Number of Orbitals 1 3 5 Electron Capacity 2 6 10 Total: Revell Introductory Chemistry, © 2018 Macmillan Learning 18 Level 4: s + p + d + f Revell Introductory Chemistry, © 2018 Macmillan Learning Level 4: s + p + d + f Sublevel s p d f Number of Orbitals 1 3 5 7 Total: Revell Introductory Chemistry, © 2018 Macmillan Learning Electron Capacity 2 6 10 14 32 Summary Energy sublevels follow a predictable pattern: Each new level adds a new sublevel, and each new sublevel has two more orbitals (four more electrons) than the one before. Above energy level four, the trend continues: Level 5 has five sublevels, level 6 has six sublevels, etc. However, even the largest elements on the periodic table fit all of their electrons within the s, p, d, and f sublevels, so we don’t need to worry about any sublevels beyond these four. Revell Introductory Chemistry, © 2018 Macmillan Learning Aufbau Diagram: This diagram shows the relative energy differences between the different energy levels and sublevels. The s orbital is the lowest in energy, followed by the p, d, and f. As the energy levels get higher, they become more closely grouped together. As the energy levels branch out into more sublevels, they actually overlap each other. Ex: energy level 4s is actually lower than energy level 3d. Revell Introductory Chemistry, © 2018 Macmillan Learning Revell Introductory Chemistry, © 2018 Macmillan Learning Describing Electron Configuration Quantum Model: Energy levels – 1, 2, 3… Energy sublevels – s, p, d, f Revell Introductory Chemistry, © 2018 Macmillan Learning Filling an Orbital with Electrons • Each orbital may have a maximum of 2 electrons. – Pauli Exclusion principle. • Electrons spin on an axis. – Generating their own magnetic field. • When two electrons are in the same orbital, they must have opposite spins. – So their magnetic fields will cancel. Tro's "Introductory Chemistry", Chapter 9 Revell Introductory Chemistry, © 2018 Macmillan Learning 50 Tro's "Introductory Chemistry", Chapter 9 51 Orbital Diagrams • We often represent an orbital as a square and the electrons in that orbital as arrows. – The direction of the arrow represents the spin of the electron. Unoccupied orbital Orbital with 1 electron Revell Introductory Chemistry, © 2018 Macmillan Learning Orbital with 2 electrons As a general rule, electrons occupy the lowest available energy levels- this is called the ground state. Aufbau Principle Revell Introductory Chemistry, © 2018 Macmillan Learning Hydrogen: electron configuration: 1s1 Revell Introductory Chemistry, © 2018 Macmillan Learning Helium: 1s2 Revell Introductory Chemistry, © 2018 Macmillan Learning Lithium: 1s22s1 Revell Introductory Chemistry, © 2018 Macmillan Learning Beryllium: 1s22s2 e- Revell Introductory Chemistry, © 2018 Macmillan Learning Boron: 1s22s22p1 Revell Introductory Chemistry, © 2018 Macmillan Learning Hund’s Rule: If empty orbitals of the same energy are available, electrons singly occupy orbitals rather than pairing together. Carbon: 1s22s22p2 Revell Introductory Chemistry, © 2018 Macmillan Learning Li: 1s22s1 B: 1s22s22p1 Be: 1s22s2 C: 1s22s22p2 N: 1s22s22p3 O: 1s22s22p4 F: 1s22s22p5 Ne: 1s22s22p6 Revell Introductory Chemistry, © 2018 Macmillan Learning What is the electron configuration of silicon? 14 e- total 1s22s22p63s23p2 Revell Introductory Chemistry, © 2018 Macmillan Learning Examples: What is the electron configuration for: 1. Phosphorus 2. Potassium 3. Iron 4. Selenium Revell Introductory Chemistry, © 2018 Macmillan Learning Revell Introductory Chemistry, © 2018 Macmillan Learning Describing Electron Configuration (part 2) valence level: The highest occupied electron energy level • Up to 8 electrons in valence level Revell Introductory Chemistry, © 2018 Macmillan Learning Argon: (18 e-) 1s22s22p63s23p6 valence level Potassium: (19 e-) 1s22s22p63s23p64s1 valence level Revell Introductory Chemistry, © 2018 Macmillan Learning Noble Gases have Filled Valences 1s2 1s22s22p6 Octet Rule: An atom is stabilized by having its highest-occupied (valence) energy level filled. 1s22s22p63s23p6 1s22s22p63s23p64s23d104p6 Revell Introductory Chemistry, © 2018 Macmillan Learning Electron Configurations for Larger Atoms inner electrons Sodium: Phosphorous: Chlorine: Noble gas notation 1s22s22p63s1 [Ne]3s1 1s22s22p63s23p3 [Ne]3s23p3 1s22s22p63s23p5 [Ne]3s23p5 1s22s22p6 = [Ne] Revell Introductory Chemistry, © 2018 Macmillan Learning Electron Configurations for Larger Atoms not involved with bonding inner electrons Titanium: [Ar]4s23d2 valence + d, f sublevels essential to bonding outer electrons Revell Introductory Chemistry, © 2018 Macmillan Learning Write the electron configuration for selenium using the noble gas shorthand. Identify the inner electrons, the outer electrons, and the valence electrons. 1s22s22p63s23p64s23d104p4 [Ar] inner outer [Ar]4s23d104p4 valence Revell Introductory Chemistry, © 2018 Macmillan Learning Electron Configurations for Ions What is the electron configuration of a sodium atom? What is the electron configuration of a sodium ion with a +1 charge? full configuration noble-gas shorthand species Symbol sodium atom Na 1s22s22p63s1 [Ne]3s1 sodium ion (+1 charge) Na+ 1s22s22p6 [He]2s22p6 or [Ne] Revell Introductory Chemistry, © 2018 Macmillan Learning Electron Configurations for Ions What is the electron configuration of an oxide ion, which is an oxygen ion with a charge of -2? species symbol full configuration oxygen atom O 1s22s22p4 oxide ion (-2 charge) O2- 1s22s22p6 Revell Introductory Chemistry, © 2018 Macmillan Learning noble-gas shorthand [He]2s22p4 [He]2s22p6 or [Ne] Many ions form noble gas configurations O: 1s22s22p4 Na: 1s22s22p63s1 O2–: 1s22s22p6 Na+: 1s22s22p6 Ne: 1s22s22p6 These are isoelectronic Revell Introductory Chemistry, © 2018 Macmillan Learning Revell Introductory Chemistry, © 2018 Macmillan Learning Electron Configuration and the Stock Montage/Getty Images Periodic Table Sovfoto/Getty Images Revell Introductory Chemistry, © 2018 Macmillan Learning Lithium [He]2s1 (3 electrons): Sodium [Ne]3s1 (11 electrons): Potassium [Ar]4s1 (19 electrons): Photo credits from top: SPL/Science Source; SPL/Science Source; Andrew Lambert Photography/Science Source Revell Introductory Chemistry, © 2018 Macmillan Learning Fluorine: [He]2s22p5 Chlorine: [Ne]3s23p5 Bromine: [Ar]4s23d104p5 Revell Introductory Chemistry, © 2018 Macmillan Learning The row indicates the highest occupied electron energy level. Revell Introductory Chemistry, © 2018 Macmillan Learning The column gives the outermost electron configuration. s1 1 s2 p6 p1 p2 p3 p4 p5 f10 f11 f12 f13 f14 2 3 d1 d2 d3 d4 d5 d6 d7 d8 d9 d10 f1 f3 f4 f5 f6 f7 f8 4 5 6 7 f2 f9 Revell Introductory Chemistry, © 2018 Macmillan Learning Revell Introductory Chemistry, © 2018 Macmillan Learning Revell Introductory Chemistry, © 2018 Macmillan Learning What is the outermost electron configuration for sulfur? 3p 4 Revell Introductory Chemistry, © 2018 Macmillan Learning Write the configuration for the highest-energy occupied sublevel for potassium, phosphorus, and iron. K: 4s1 P: 3p3 Fe: 3d6 Revell Introductory Chemistry, © 2018 Macmillan Learning Write the electron configuration for aluminum. How many valence electrons does aluminum have? [Ne] 3s2 3p1 3 valence electrons Revell Introductory Chemistry, © 2018 Macmillan Learning C Si Ge Revell Introductory Chemistry, © 2018 Macmillan Learning The column gives the outermost electron configuration. The row indicates the highest occupied electron energy level. Revell Introductory Chemistry, © 2018 Macmillan Learning Revell Introductory Chemistry, © 2018 Macmillan Learning