Rutherford, Planck and Bohr Flashcards
1
Q
Rutherford
A
- postulated that the atom had a dense, positively charged nucleus that made up only a small fraction of the volume of the atom
- first to show atom being mostly empty space
2
Q
Planck
A
- developed the first quantum theory
- Energy emitted as electromagnetic radiation from matter comes in discrete bundles called quanta
3
Q
Planck Relation
A
- determines energy of a quantum
- E=hf
- h is Planck’s constant (60626 x 10-34J•s)
- f is the frequency of the radiation (sometimes designated by the Greek letter nu, v)
- frequency of emitted radiation is proprtional to the energy of that radiation
4
Q
Planck’s constant
A
- 6.626 x 10-34J•s
5
Q
Bohr Model of the Atom
A
- A dense, positively charged nucleus is surrounded by electrons revolving aroung the nucleus in orbits with distinct energy levels
- Bohr placed restrictions on the possible values of angular momentum
- Bohr created an important conceptualization of atomic behavior but we now know electrons are NOT restricted to specific pathways but tend to be localized in certain regions of space
- proved inadequate to explain the structure and behavior of atoms containing more than 1 electron
6
Q
Bohr Formulas
A
- L=nh/2π
- E = - RH/n2
- Angular momentum of an electron is directly proprtional to it’s Principle Quantum number
- The energy of the electron increases expontially with the Principle Quantum Number
7
Q
ground state
A
- atom at the state of lowest energy (smallest, lowest-energy radius)
- n=1
8
Q
excited state
A
- when at least 1 electron has moved to a subshell higher than normal energy
9
Q
Atomic Emission Spectra
A
- When electrons return from the excited state to the ground state, they emit an amount of energy that is exactly equal to the energy difference between the 2 levels
- sometimes the electromagnetic energy emitted corresponds to a frequency in the visible light range
- used as a fingerprint for the elements
**moves higher to lower
10
Q
AHED
A
- As electrons go from a lower energy level to a higher energy level, they get AHED
- Absorb Light
- Higher potential
- Excited
- Distant (from nucleus)
11
Q
Electro magnetic Energy Emission of Photons equation
A
- E=hc/λ
- h = Plancks constant (6.626 x 10-34J•s)
- c = speed of light (3.00 x 108 m/s)
- λ = wave length of the radiation
- combination of E=hf and c=fλ
12
Q
Name the 3 series of hydrogen emission spectrum
A
- Lyman Series
- group of H emission lines transitioning from n ≥ 2 to n = 1
- larger energy transitions; therefore has shorter photon wavelengths
- UV light
- Balmer Series
- transitions from energy levels n ≥ 3 to n = 2
- visable light
- Paschen series
- transitions from n ≥ 4 to n = 3
- infared
13
Q
Equation for energy associated with a change in the principal quantum number
A
E = hc/λ = -RH [1/n2i - 1/n2f]
- RH = Rydberg Unit of energy = 2.18 x 10-18 J/electron
- energy of the emitted photon corresponds to the difference in energy between the higher-energy initial state and the lower-energy final state
- wavelength of emitted proton is inversely proportional to the energy of that photon
- the energy emitted or absorbed by an atom will increase as the energy level of the excited electron increases (decreases as energy level decreases)
14
Q
Atomic Absorption Spectra
A
- The atomic absorption spectra of an element is unique
- for an electron to jump from a lower energy level to a higher one, it must absorb an amount of energy equal to the energy difference of the 2 levels
- These wavelengths correspond to the wavelengths of emission
- Identification of elements in the gas phase requires absorption spectra
**moves lower to higher