Chapter 4: Arrangement of Electrons in Atoms

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Electrons can move as

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Electrons can move as

Particles and Waves

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Wave Nature

  • Proposed by Louis de Broglie

  • Electrons could be considered waves confined to the space around the NUCLEUS

  • Only certain wavelengths and frequencies could exist

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A wave can be describes at

wavelength ( labda)

Frequency v (nv)

Energy: E

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Wavelength

  • Symbol: Lambda

  • The distance between the crests of a wave

  • UNITS: meters or nanometers

  • 10^9nm = 1m

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Frequency

  • Symbol: v (nv)

  • The number of waves that pass/second

  • UNITS: 1/sec = 1 hertz

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Speed of Light

  • A constant

  • Symbol: C

  • fastest possible speed

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Speed of light equation

3.00 x 10^8 meters/second

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lambda and v are ….

inversely related

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long wavelength =

low frequency

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short wavelength =

long frequency

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Electromagnetic Spectrum

350 nm = violet to 750 nm = red

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Particle Nature of Light

Some properties of light cannot be explained by wave theory: white hot objects and the photoelectric effect

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“White Hot” Objects

  • When objects are heated they EMIT LIGHT

  • Wave theory predicts that only UV LIGHT would be emitted but white, yellow, and orange light

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Photoelectric Effect

  • Emission of electrons by certain metals when light shines on them

  • The light must be of a certain energy/frequency to “knock” an electron from the surface

    (Albert Einstein observed in 1905)

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Quantum Energy

  • MAX PLANCK

  • White hot objects and the photoelectric effect both emit small, specific amount of energy call QUANTA or PHOTONS

  • A specific amount “ bundle” of energy that can be gained or lost by an atom

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Energy of a Quantum

  • An individual Quantum is known as a PHOTON of light and has evergy

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Energy of a Quantum equation

  • h = Plack’s constant

  • h = 6.626 x 10 ^-34 joules x seconds

  • E = hv

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Energy + wavelength equation

E = hc/lambda

  • inversely related

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Wavelength of colors

750-625 nm - Red

625-590nm - Orange

590-565 nm - Yellow

565-520 nm - Green

520-435nm - Blue ( indigo)

435-350 nm - Purple

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Wavelengths ( highest to lowest)

Gamma Ray

X-Ray

Ultraviolet light

Visible

Infread

Microwave

Radio

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Bohr Model

Why did Bohr study hydrogen?

- After observing the H line emission spectrum

  • Simplest atom - only has one electron

  • The electrons of the gas are easily excited by a current

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  1. How are the electrons moving

  2. Where are the located

  3. How much energy do they have

  1. As particles with a definite circular path

  2. In rings, or orbits around the nucleus

  3. Th energy of an electron can be calculated

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  1. Electrons closer to the nucleus have …

  2. At higher energy levels, the energy is …

<ol><li><p>Lower energy values</p></li><li><p>Higher</p></li></ol><ul><li><p>each orbit is an energy lever designated by the variable n</p></li><li><p>N =1 is the ground state</p></li><li><p>N = infinity is when the electron has been removed from the atom</p></li><li><p>Energy is quantized, meaning there are no levels in between the levels designated by n = 1,2,3,4, ect</p></li></ul>
  1. Lower energy values

  2. Higher

  • each orbit is an energy lever designated by the variable n

  • N =1 is the ground state

  • N = infinity is when the electron has been removed from the atom

  • Energy is quantized, meaning there are no levels in between the levels designated by n = 1,2,3,4, ect

<ol><li><p>Lower energy values</p></li><li><p>Higher</p></li></ol><ul><li><p>each orbit is an energy lever designated by the variable n</p></li><li><p>N =1 is the ground state</p></li><li><p>N = infinity is when the electron has been removed from the atom</p></li><li><p>Energy is quantized, meaning there are no levels in between the levels designated by n = 1,2,3,4, ect</p></li></ul>
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Spectroscopy

When atoms are excited by a outside energy source ( heat, flame, or electric current) the electrons can be promoted to higher energy states. However, this situation is highly unstable and the electron will eventually return to a lower energy state.

  • when the electron returns to a lower energy level, energy is given off in the form of ( quanta), also known as a (photon of light)

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Energy input:

From LOWER levels to HIGHER level

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Energy output:

From HIGHER levels to LOWER levels

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Hyrogen produces lines in the

visible, ultraviolet, and infrared regions of the electromagnetic spectrum

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Balmer series

visible

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Lyman series

Uv

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Paschen series

IR ( infread)

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Energy at each level

E = -2.178 x 10^-18 J ( Z^2/ n^2)

Z = number of protons

n = energy level

  • Calculation: deltaE = Efinal - Einital

  • -2.178 x 10^-18 ( Z^2/n^2 (efinal) -Z^2/n^2 (einitial) )

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Bohr’s Model ( hydrogen)

  • Cannot successfully predict line spectra for an other element besides hydrogen

  • Electrons must not be moving in circular orbits at set distances from the nucleus

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Electrons

  • Moving as waves

  • Not in orbits

  • Located in Orbitals

  • Areas of high probability based on the wave motion and energy of an electron

  • Every orbital has an “address” given by a set of 4 Quantum numbers

  • Energy: determined by h (like Bohr)

  • Higher n= higher energy level = more energy = further from the nucleus

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  • Schrodinger

Proposed a complex mathematical relationship to predict where e- is located

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DeBroglie

  • Proposed the particle to describe electron motion

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Heisenberg

  • Proposed the Heisenberg uncertainty

  • The more you know about e- position, the less you know about it’s velocity (Inversely)

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  • Pauli

  • Every electron in an atom must have a unique set of quantum numbers

  • Electrons in the same orbital must have opposite spins

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Hund’s

  • Electrons will fill an unoccupied within a sublevel before pairing up with another electron in an orbital

  • This minimizes repulsion and leads to stability

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Principle Quantum Number

  • n

  • Tells what energy level the electron level is in

  • Possible values: 1 to infinity

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  • Orbital Quantum Number

  • l

  • Tells about the Shape of the orbital where the electron is housed

  • Possible values: 0 to ( n-1)

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  • Magnetic Quantum Number

  • Ml

  • Tells about the orientation of the orbital around the nucleus

  • Possible values: -l to +l including 0

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Spin Quantum Number

  • Ms

  • Tells the direction of the electron spin within an orbital

  • Possible values: +1/2 and -1/2

  • +1/2 : Clockwise spin

  • -1/2 : Counterclockwise spin

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S orbital:

  • spherical ( l =0)

  • 0

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P orbital

  • peanut shaped ( l =1)

  • -1,0,1

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D orbital:

  • daisy shaped ( l =2)

  • -2,-1,-0,1,2

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F orbital

flower shaped ( l =3)

-3,-2,-1,0,1,2,3

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Energy level Diagrams

  • A way to keep track of electrons

  • Includes line boxes that represent Orbitals

  • Also shows orbital types and energy levels

  • Once filled, it is possible to find the quantum number set for any electron in the atom

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Aufbau Principle

  • Meaning: Build up

  • Electrons must be filled from the lowest energy to the highest energy

  • Do not move to the next until the one below has been completely filled

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Hund’s Rule

  • Electrons will fill an unoccupied within a sublevel before pairing up with another electron in an orbital

  • This minimizes repulsion and leads to stability

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Octet Rule

  • Atoms become stable when their outermost energy level contains 8 electrons

  • Noble gases have a full OCTET

  • The outermost electrons are called Valance Electrons (except He)

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Electron Configuration

  • Shows every electron in the atom starting with the 1s orbital

  • Valence electrons exist in the highest energy level listed

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Noble Gas Configuration

  • Uses the preceding noble gas core to shorten the electron configuration

  • Allows the valence electrons to be determined easily

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