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The Bohr Atom Model: Electrons Arrangement in an Atom

Learn about the refinements of the atomic model through Dalton, Thomson, and Bohr, including the Bohr model explaining electron orbits around the nucleus. Explore the Electromagnetic Spectrum and Bright Line Spectrum to study elements' unique light emissions.

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The Bohr Atom Model: Electrons Arrangement in an Atom

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  1. Chapter 4 Arrangement of Electrons in an Atom

  2. 4.1 Refinements of the atomic model • Models of the atom so far: • Dalton – atoms are like little “bb’s” - then the electrongets discovered • Thomson – atom is like a charged “bb” • Rutherford - Gold foil experiment – hollow charged “bb” • Bohr model of the atom (1913) – Neils Bohr – Danish Physicist • The Bohr model of the atom comes from the idea that light is waves of energy http://web.visionlearning.com/custom/chemistry/animations/CHE1.2-an-atoms.shtml

  3. The Bohr Atom (1913) • All the positive charge was in the nucleus • Electrons orbited the nucleus much like planets orbit the sun (at fixed distances) • The closer the electrons to the nucleus, theless energy it has. • The farther the electron is from the nucleus, the more energy it has.

  4. The Electromagnetic Spectrum • Visible light, x-rays, ultraviolet radiation, infrared radiation, microwaves and radio waves are all part of the electromagnetic spectrum

  5. The Electromagnetic Spectrum • The spectrum consists of electromagnetic radiation – energy that travels like a wave • Waves can be described by the wave equation which includes velocity (c = speed of light), wavelength (λ) and frequency (ν). • Wavelength (definition) = the distance between peaks of a wave • Light through prism leads to high energy (violet) low energy (red)

  6. The Electromagnetic Spectrum • ROYGBIV - colors of the visible spectrum • Bright Line Spectrum (BLS) – caused by e- emitting energy as they return tolower energy levels energy level. • heat sodium - yellow light 2 c • heat lithium - red light • elements can appear to give off the same color light, but each will have its own BLS • BLS - used to determine identity of an element • BLS - validates Bohr’s idea that electrons jump to different energy levels and give off different wavelengths of light

  7. The Electromagnetic Spectrum • Light from the sun (white light) appears as a continuous spectrum of light. • Continuous Spectrum of Light (definition) = There are no discrete, individual wavelengths of light but rather all wavelengths appear, one after the other in a continuous fashion • Spectroscopy (definition) = the study of substances from the light they emit. • We will use spectroscopes (An instrument that splits light into its component colors) and flame tests to study elements because each element emits a different spectrum of light when exited .

  8. Birght Line Spectrum • Bohr proposed that the energy possessed by an e- in a H- atom and the radius of the orbit are quantized (bls) • Quantized (definition): a specific value (of energy) Like a set of stairs, the energy states of an electron is quantized – i.e. electrons are only found on a specific step The ramp is an example of a continuous situation in which any energy state is possible up the ramp

  9. Bohr’s Energy Absorption Process • Light or energy excites an e- from a lower energy level (e- shell) to a higher energy level • These energy levels are “ quantized “ (the e- cannot be in between levels), the e- disappears from one shell and reappears in another • This absorption or excitation process is called a quantum leap or quantum jump

  10. Bohr’s Energy Absorption Process • Ground State Analogy = a spring and two balls This is an energy emission process and what we observe in the hydrogen line spectrum Both the atom and e- now have higher energy The e- absorbs energy in the ground state and is excited to a higher level

  11. Bohr’s Energy Absorption Process • When energy is added, the electron is found in the “excited state.” • The Excited State (definition) = an unstable, higher energy state of an atom • An illustration of Bohr’s Hydrogen atom (from ground to excited state):

  12. Bohr’s Energy Absorption Process • The atomic line spectral lines - when an e- in an excited state decays back to the ground state The electron loses energy, light (colors) is emitted and the e- returns to the ground state This is another illustration of bls.

  13. The Bohr Model - Summary

  14. The Bohr Model - Summary • Bohr also predicted that since electrons would occupy specific energy levels and each level holds a specific number of electrons • The maximum capacity of the first (or innermost) electron shell is twoe-. • Any element with more than twoe-, the extra e- reside in additional electron shells.

  15. The Bohr Model - Summary Electron Configurations for Selected Elements • The number of e- per shell = 2n2 (where n is the shell number)

  16. Bohn Models Draw Bohr Diagrams for the elements 1-10. Save room to draw them short hand also

  17. Short Hand Bohr Model • Write the symbol of the element • Use a ) to represent each shell • Write the # of e- in each shell • Ex.

  18. The Truth About Bohr Models • At atomic # 19 (z = 19), there is a a break in the pattern. One would expect that energy level #3 would continue to fill up. However, the next two electrons go into the next energy level. Look at K and Ca:

  19. The Truth Continued…… • So, there is a relationship between the main column # and the number of outershell electrons. • Column # = the number of valence electrons • And, there is a relationship between the row # and the number of energy levels. • Row # = the number of shells • The Bohr model truly works well for the H atom only • for elements larger than H the model does not work.

  20. Bohr Summed Up • Bohr made 2 huge contributions to the development of modern atom theory • He explained the atomic line spectra in terms of electron energies • He introduced the idea of quantized electron energy levels in the atom • The Bohr atom lasted for about 13 years and was quickly replaced by the quantum mechanical model of the atom. The Bohr model is a good starting point for understanding the quantum mechanical model of the atom Do ws# 1, question 1- Use short-hand configuration

  21. 4.2 Quantum Numbers and Atomic Orbitals • 4.3 Electron Configuration

  22. Quantum Numbers & Atomic Orbitals • The Bohr model describes the atom as having definite orbitals occupied by electron particles. • Schrödinger (1926) introduced wave mechanics to describe electrons – proved Bohr’s Model to be a lie • Based his idea that electrons behaved like light (photons). • Electrons show diffraction (interference) properties like light. • Treats electrons as waves that are found in orbitals. • Orbitals (definition) = clouds that show region of probable location of a particular electron.

  23. Wave Mechanical Model • The Bohr model really is the wave mechanical model • There are many types of orbitals – we can see them on the periodic table

  24. Subatomic Orbitals S P D

  25. Quantum Numbers • An electron’s address • principle (n): what shell, level, the e- is in n = 1,2,3...7 • azimuthal (l): energy sub level - s, p, d, f • magnetic – orientation of orbital about the nucleus (s has only 1, p has 3, etc.) • spin - clockwise or counterclockwise (+1/2 or -1/2)

  26. Label Your Periodic Tabel • On your periodic table, shade azimuthals,p,d,f blocks different colors • Label the principal quantum numbers…1-7 • Label the valence electrons across the top

  27. Electron Configuration • Electron Configuration - a representation of the arrangement of electrons in an atom

  28. Electron Configuration • Examples of electron Configuration • 1. Li 1s22s1 • 2. C 1s22s22p6 # of e- in that shell principle azimuthal

  29. Electron Configuration • Take note that after 4s is filled, 3d is than filled before 4p. • …… 6s than 4f than 5d than 6p • When writing out the electron configuration, always write your numbers in numerical order • Y 1s22s22p63s23p64s23d104p65s24d1 – NO! • Y 1s22s22p63s23p63d104s24p64d15s2

  30. Electron Configuration • Examples: • Be • O • Ca • Mn

  31. Electron Configuration • Examples • Pb • Os

  32. Electron Configuration • Short Hand • Write the name of the last noble gas • Write the electron config. that follows • Ex. Fe [Ar]3d64s2 • Exceptions • Cr [Ar] 3d54s1 • Cu, Ag, Au- all s’s donate 1 e- to make the d orbital full • Cu [Ar] 4s13d10

  33. Orbital Notation • Electrons enter orbitals in a set pattern. For the most part, they follow these rules: • 1) The Aufbau Principle - electrons must fill lower energy levels before entering higher levels.

  34. Orbital Notation • Orbitals are like "rooms" within which electrons "reside". • The s subshell has one s-orbital. The p subshell has three p-orbitals. The d subshell has 5 and f has 7. • Each orbital can hold at most 2 electrons

  35. Orbital Notation • 2. Hund’sRule (better known as the Bus Rule) • Before any second electron can be placed in a sub level, all the orbitals of that sub level must contain at least one electron – spread out the e- before pairing them up. • 3. Pauli Exclusion Principle - electrons occupying the same orbital must have opposite spin. • See a good online illustration at http://www.avogadro.co.uk/light/aufbau/aufbau.htm

  36. Orbital Notation H 1s F 1s 2s 2p

  37. Orbital Notation • Examples: • Li F • Na Sc

  38. Orbital Notation • We can also do shorthand orbital notation (outer shell only) • Ca N • Fe Ag [Kr] 4d105s1 Ag [Kr] 4d 5s

  39. Significance of Electron Configurations • Valence shell electrons - outermost electrons involved with bonding • no atom has more than 8 valence electrons • Noble gases - 8 valence electrons – least reactive of all elements • Lewis Dot structures: NSEW (cheating) also show correct way, count to 8

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