atomic spectra and electron orbitals. the classical atom electrons orbited the nucleus. electrons...
DESCRIPTION
The Bohr Atom Electrons orbit in specific energy levels without radiating Electrons orbit in specific energy levels without radiating Each energy level has a specific energy Each energy level has a specific energy To change energy levels, atoms must either absorb or emit energy (photons) To change energy levels, atoms must either absorb or emit energy (photons) Link Link LinkTRANSCRIPT
Atomic Spectra and Atomic Spectra and Electron OrbitalsElectron Orbitals
The Classical AtomThe Classical AtomElectrons orbited the nucleus.Electrons orbited the nucleus.
Problem!!Problem!!Accelerating charges emit radiation (energy)Accelerating charges emit radiation (energy)With less energy the electron orbitals should With less energy the electron orbitals should
shrink and the electrons should spiral into the shrink and the electrons should spiral into the nucleusnucleus
The Bohr AtomThe Bohr AtomElectrons orbit in specific energy levels Electrons orbit in specific energy levels
without radiatingwithout radiatingEach energy level has a specific energyEach energy level has a specific energyTo change energy levels, atoms must To change energy levels, atoms must
either absorb or emit energy (photons)either absorb or emit energy (photons)Link
Ground State vs. Excited StatesGround State vs. Excited StatesGround state is the lowest energy level in Ground state is the lowest energy level in
the atom.the atom.All other energy levels are known as All other energy levels are known as
excited states.excited states.
Quantization of EnergyQuantization of EnergyA result of the Bohr atom is that energy A result of the Bohr atom is that energy
cannot come in any amount it wants, it cannot come in any amount it wants, it must be in specific amounts of energy must be in specific amounts of energy called quantacalled quanta
Like steps or rungs of a ladderLike steps or rungs of a ladder
Electron Volts (eV)Electron Volts (eV)The energies involved in atomic spectra The energies involved in atomic spectra
are very small, making it inconvenient to are very small, making it inconvenient to use Joules as our units of energyuse Joules as our units of energy
1 eV = 1.6x101 eV = 1.6x10-19-19 J JeV eV J J multiply by 1.6x10multiply by 1.6x10-19-19
J J eV eV divide by 1.6x10divide by 1.6x10-19-19
Hydrogen Atom: Energy Levels Hydrogen Atom: Energy Levels and Energies of Transitionand Energies of Transition
2
6.13neVE
22
116.13if nn
eVE
n - energy level of atomn - energy level of atomprimary quantum numberprimary quantum numbern = 1, 2, 3, …n = 1, 2, 3, …
E = -2.176 x 10-18 J n2
Photon EnergyPhoton EnergyE = hf = hc/E = hf = hc/
h = 6.626 x 10h = 6.626 x 10-34-34 J*s J*sc = 3x10c = 3x1088 m/s m/s f – frequencyf – frequency – – wavelength wavelength
EEphotonphoton = = EEatomatom
EEatom atom > 0 if atom absorbs photon> 0 if atom absorbs photonEEatom atom < 0 if atom emits photon< 0 if atom emits photon
Emission SpectraEmission SpectraThe set of energies emitted by an atom.The set of energies emitted by an atom.Energy determines frequency which Energy determines frequency which
determine colordetermine color
Electromagnetic SpectrumElectromagnetic Spectrum
Absorption SpectrumAbsorption SpectrumHow we know the gaseous atmosphere How we know the gaseous atmosphere
surrounding the sunsurrounding the sun
Spectral SeriesSpectral SeriesSpectral series are the set of energies Spectral series are the set of energies
produced when electrons from excited produced when electrons from excited states emit photons and transition down to states emit photons and transition down to the same final energy levelthe same final energy level
Three important series for Hydrogen:Three important series for Hydrogen:Lyman Series: nLyman Series: nff = 1 = 1Ballmer Series: nBallmer Series: nff = 2 = 2Paschen Series: nPaschen Series: nff = 3 = 3
Atoms that aren’t HydrogenAtoms that aren’t HydrogenThe formulae in the previous slides only The formulae in the previous slides only
apply to Hydrogen.apply to Hydrogen.For other atoms, the energies cannot be For other atoms, the energies cannot be
so easily calculated, and will often be so easily calculated, and will often be given to you directly. given to you directly.
Energy Level DiagramEnergy Level Diagram
E = EE = Eff - E - Eii
Ionization EnergyIonization Energy In order to remove an electron from an In order to remove an electron from an
atom you have to add enough energy atom you have to add enough energy make the energy zero.make the energy zero. i.e. if you are at ground level and have an i.e. if you are at ground level and have an
energy of -10.38eV that means you need energy of -10.38eV that means you need 10.38eV if energy to ionize10.38eV if energy to ionize
All left over Energy become All left over Energy become Kinetic EnergyKinetic Energy
ExampleExampleAn atom’s only electron is in the fourth An atom’s only electron is in the fourth
energy level (-2.35 eV). energy level (-2.35 eV). How many different photon energies can be How many different photon energies can be
emitted as this photon returns to the ground emitted as this photon returns to the ground state (-15.8 eV)?state (-15.8 eV)?
What is the frequency of the photon that What is the frequency of the photon that would be emitted if the electron returned to would be emitted if the electron returned to the ground state in a single transition?the ground state in a single transition?