Isotopes
Atoms of the same element with the same atomic number but different mass number
Radio Isotopes
Isotopes that have unstable nuclei and therefore emit radiation when they break up
Uses
Wavelength (frequency and energy)
The shorter the wavelength the higher the frequency of the wave and the more energy it contains
Emission Spectra
When electrons are excited to a higher energy level, and then return to a lower energy level, they release a photon of a specific energy, as shown by a specific frequency of light
*electrons moving back to the lowest energy states and over longer distances release more energy
as the electron moves to higher energy states, the spectral lines converge
Lyman series
U.V. radiation
from a higher sublevel to n=1
Balmer Series
Visible light radiation
From a higher sublevel to n=2
Paschen
Infrared radiation
From a higher sublevel to n=3
Electronic Configuration
1s2 2s2 2p6 3s2 3p6 4s2 3d10 4p6….
(4s electrons are lost first in transition metals)
Aufbau Principle
The order in which the energy levels are filled
2 exceptions:
chromium and copper fill up 3d first / electrons from 4s are lost first
Hund’s Rule
Electrons prefer to occupy orbitals on their own, and only pair up when no empty orbitals of the same energy are available
Pauli Exclusion Principle
Paired electrons have the opposite spin as this reduces the mutual repulsion between the paired electrons
First Ionization Energy
The energy required to remove one mole of electrons from one mole of atoms in the gaseous state to form one mole of univalent cations in the gaseous state
X(g) –> X+ + e- +ve dH
Factors affecting ionization energy
Successive Ionization energy
X+(g) –> X2+(g) + e-
Ionization Energy Trends on a Periodic Table - Across a period
Ionization Energy Trends on a Periodic Table - Down a group