the electron dr. m hazlett mandeville high school

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The Electron Dr. M Hazlett Mandeville High School

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Werner Heisenberg concluded that since electrons are affected by photons (light), no one can be certain as to their actual location Louis de Broglie explained that electrons exhibit both particle and wave behavior and determined its wave function (ψ) The electron is considered a lepton, part of non- baryonic matter Electrons are created through neutron decay Finally, Millikan determined the electron’s mass (9.109 x g) and charge (1.602 x C).

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Page 1: The Electron Dr. M Hazlett Mandeville High School

The Electron

Dr. M HazlettMandeville High School

Page 2: The Electron Dr. M Hazlett Mandeville High School

A Brief Review• J.J. Thompson and others at first believed

that the electrons floated in a sphere filled with a positive substance

• Later, Neils Bohr came up with the Planetary Model where the electrons orbited the nucleus in 7 layers

• Erwin Schrodinger showed that since the electrons are orbiting at the speed of light, it creates an electron cloud around the nucleus

Page 3: The Electron Dr. M Hazlett Mandeville High School

• Werner Heisenberg concluded that since electrons are affected by photons (light), no one can be certain as to their actual location

• Louis de Broglie explained that electrons exhibit both particle and wave behavior and determined its wave function (ψ)

• The electron is considered a lepton, part of non-baryonic matter

• Electrons are created through neutron decay• Finally, Millikan determined the electron’s mass

(9.109 x 10-28 g) and charge (1.602 x 10-19C).

Page 4: The Electron Dr. M Hazlett Mandeville High School

Electrons and Ions• Atoms losing or gaining electrons become ions– If the atom has lost an electron, its has more p+

than e-, thus a positive charge cation– If the atom gains an electron, its has more e- than

p+ and a negative charge anion• This loss and/or gaining of electrons

determines chemical bonds and reactions

Page 5: The Electron Dr. M Hazlett Mandeville High School

The Standard Model and Electrons• In the standard (quantum) model, the e- in the

atoms have discrete energies– There are seven energy levels (n)– Electrons start in their ground state – their lowest

energy level• If the electron gains energy, it moves up one or more

levels• The e- is now in its excited state• When the e- releases its energy in the form of a photon

(ϒ), it returns to its ground state

Page 6: The Electron Dr. M Hazlett Mandeville High School

• The wavelength of light (λ) is related to the energies of the electron’s ground and excited states– E High - E Low = h c

λ where h c = 1.196 x 105 KJ●nm/mol

Page 7: The Electron Dr. M Hazlett Mandeville High School

The Bohr Model and Lightwaves• Using spectroscopy, can determine the λ

series of electrons and photons of atoms• Bohr, using a CRT filled with H2 noted that

certain light wavelengths appeared when 5000 v of electricity connected to the tube

• Conclusion: The light represented the energy of the e- as it jumped from its ground to excited state and back

Page 8: The Electron Dr. M Hazlett Mandeville High School

Different wavelengths and frequencies, different colors and

thus – different elements

Page 9: The Electron Dr. M Hazlett Mandeville High School

• Other scientists used Bohr’s idea and created ranges or series of wavelength (λ) and frequency (ϒ) corresponding to the e- ground state, its excited state, and its final energy level

• Each series is based on light wavelength and frequency

• Series can measure absorbed and emitted energy in the form of photons

Page 10: The Electron Dr. M Hazlett Mandeville High School

Series:1. Lyman Series

Final energy level (n1) = 1Light will be in UV rangee- goes from n ≥ 2 to n1 = 1

e- Start Level λ (nm) 2 1223 1034 97.25 94.96 93.7+ 91.1

Page 11: The Electron Dr. M Hazlett Mandeville High School

2. Balmer Seriesn1 = 2Light is partially visible – R, B, Ve- goes from n ≥ 3 to n1 = 2 e- Start Level λ (nm) 3 656

4 4865 4346 4107 397+ 365

Page 12: The Electron Dr. M Hazlett Mandeville High School

3. Paschen Seriesn1 = 3Infrared light e- Start Level λ (nm) 4 1870

5 12806 10907 10008 954+ 820

Page 13: The Electron Dr. M Hazlett Mandeville High School

• Other series are used:– Brackett Series n1 = 4– Pfund Series n1 = 5– Hymphreys Series n1 = 6

Equations:c = λϒ (Wavelength x Frequency)

1 / λ = R ( 1 / (n1)2 - 1 / n2 ) Wavelength of emitted/absorbed photon R = Rydberg Constant (1.097373 x 107 m)

E photon = h ϒ = h c / λ

Page 14: The Electron Dr. M Hazlett Mandeville High School
Page 15: The Electron Dr. M Hazlett Mandeville High School

– If the e- goes to its ground state (n = 1) UV light and use the Lyman Series

– If the e- goes to its excited state (n = 2) visible light and the Balmer Series

– If the electron moves three levels (n = 3) infrared light and the Paschen Series is used

Page 16: The Electron Dr. M Hazlett Mandeville High School

Electron Wavelengths

Page 17: The Electron Dr. M Hazlett Mandeville High School
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Hydrogen’s Emission Spectrum

Page 20: The Electron Dr. M Hazlett Mandeville High School

In the Standard Model. . . . . .• There are four basic quantum numbers:

1. n = period = e- energy level, 1 through 7Maximum electron capacity per level =2n2

2. l = orbital type or sublevel = s, p, d, fs - sharp or spherical ○p – principle ∞d – diffuse, four-leaf clover shapedf – fundamental, 6 leaf clover shaped

Page 21: The Electron Dr. M Hazlett Mandeville High School

3. mL = orientation of orbitals

4. ms = spin, either +1/2 or -1/2

Pauli Exclusion Principle – No two e- in the same atom can have the same quantum numbersIn each suborbital, there will be two e-, and each will have opposite spins Aufbau Principle – Atoms will fill up their orbitals starting with the lowest energies to highest

Page 22: The Electron Dr. M Hazlett Mandeville High School

Hund’s Rule – Each suborbital will have a maximum of 2 e-; with opposite spins. Each suborbital in an energy level must have one e- before any receive a second one

Page 23: The Electron Dr. M Hazlett Mandeville High School

Valency• Valence Electrons – the electrons in the

outermost shell or energy level– Octet Rule – atoms seek to fill to completion the

outermost energy level by gaining or giving away electrons

– Valence electrons will determine bonds and reactions

– Valency provides grouping of elements on Periodic Table (Groups I through VIII)

Page 24: The Electron Dr. M Hazlett Mandeville High School

Noting Electron Configuration• We need to be able to show how an atom’s

electrons are configured (distributed) in order to explain chemical bonds and reactions

• There are several ways to do this, but first:– You must know and understand the element’s

valence energy level (the period)– You must know the # valence e- (Group I to VIII or

if a Transitional Metal)– And you must know the orbital grouping: s, p, d,

or f

Page 25: The Electron Dr. M Hazlett Mandeville High School

Aufbau Notation

• This gives the valence energy level, the valence orbital shape and the # of valence electrons in that level

Example: 2 p 5

Energy Level Orbital # e-

Page 26: The Electron Dr. M Hazlett Mandeville High School

Electron Diagram – Aufbau Principle

7 p 7 s

6 d 6 p

5 d 4 f

6 s 5 p

4 d 5 s

4 p 3 d

4 s 3 p

3 s 2 p

2 s 1 sStart

Page 27: The Electron Dr. M Hazlett Mandeville High School

Aufbau Notation:• Long Format: – Na w/ 11 electrons would be: 1s22s22p63s1

– Short Format only gives the LAST Energy Level and the number of electrons in it• Na 3s1

– Without this e-, Na would isoelectric w/ Ne (have the same e- configuration)

• Cl -17 would be 1s22s22p63s23p5 in Long Format• Cl – 17 would be 3s23p5 in Short Format and its Lewis

Dot Structure would have 7 dots around the elemental symbol

Page 28: The Electron Dr. M Hazlett Mandeville High School

• Often, you will see another shorthand way of writing an element’s electron configuration– This is called the Noble Gas Configuration– Noble Gases are in Column VIII– For example, using Na, Na’s configuration would

be: [Ne]3s1

– The [ ] means isoelectric (the starting point)– Li would be [He]2s1 - La [Xe]6s25d1

– Mn would be [Ar]4s23d5 - Ce [Xe]6s25d14f1

– Zn would be [Ar]4s23d10 - Pr [Xe]6s24f3

Page 29: The Electron Dr. M Hazlett Mandeville High School

Lewis Dot Diagrams• Dot diagrams demonstrate the type of

covalent bonds an element may make under certain conditions

• The element’s symbol is surrounded by up to 8 dots, each dot representing a valence e-

• Maximum of 2 dots per side (2 dots x 4 sides = 8 total, an octet valence level)

• It can be used for single atoms or to show molecules and their bonds and shapes

Page 30: The Electron Dr. M Hazlett Mandeville High School

• Determine dots from either doing the e- mapping OR learn to read the periodic table!

• Often, for transitional metals – need to do mapping (problem if ion)

• Remember Hund’s Rule• Watch for + and – ions and either add or subtract

the correct number of electrons• Each side of elemental symbol represents one of

the last 4 suborbitals (□) of the SAME Energy Level!

• Do not have to have 8 e- dots, can have openings– This is where bonds to other atoms can occur

Page 31: The Electron Dr. M Hazlett Mandeville High School

Lewis Dot Diagrams

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Lewis Dot Diagrams

Page 35: The Electron Dr. M Hazlett Mandeville High School

Orbitals

Page 36: The Electron Dr. M Hazlett Mandeville High School

Next Stop. . . . .• Once we have the diagramming conquered,

then it is onto the types of bonds – ionic and covalent

• From there – we can diagram bonded atoms (molecules and polyatomic ions)

• Then, we move onto reactions