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Amplitude
the height of a wave from the origin to a crest, or from the origin to a trough
Atomic emission spectrum
a set of frequencies of electromagnetic waves given off by atoms of an element; consists of a series of fine lines of individual colours
electromagnetic spectrum
consists of electromagnetic radiation (EMR) which is the release and transmission of energy in the form of waves
Electron configuration
the arrangement of electrons in an atom
electronegativity
ability of an atom in a molecule to attract electrons to itself
frequency (v)
the number of waves that pass a given point per second
UNITS—→ s-1 or Hz
Ionization energy
energy required to remove an electron from an atom in its gaseous state
photon
a particle of EMR (electromagnetic radiation) with no mass that carries quantum of energy
Wavelength
the shortest distance between equivalent points on a continuous wave.
UNITS—→ m,cm,nm, etc…
Atoms are observed with what instrument?
Scanning tunneling microscope
Democritus
Greek philosopher that believed atoms were indivisible and indestructible. Got booed at by Aristotle so no one believed him
Thomson
Made the plum pudding model, indicating that electrons were randomly scattered around the atom
Rutherford
Shot alpha particles (He2+) at a gold foil, noticed that sometimes it got repelled, meaning that something positive was repelling it. Later discovered that the nucleus was at the center of the atom and that an atom was mostly empty space
Niels Bohr
Proposed circular paths (orbitals) and that each possible electron orbit has a fixed energy called energy levels
Chadwick
Discovered neutrons
Quantum theory (by Marx Planck)
Matter can gain or lose energy only in small, specific amounts called quanta. That is, a quantum is the minimum amount of energy that can be gained or lost by an atom.
According to Planck’s theory, for a given frequency (v), matter can emit or absorb energy only in whole-number multiples of hv, that is Planck’s constant: 6.63 × 10-34
The energy of a quantum is related to the frequency of the emitted radiation
Photoelectric effect
While a beam of light has many wavelike characteristics, it can also be thought of as a stream of tiny particles called photons
Continuous spectra
Eye perceives it as white light
Looks like a rainbow when observed through a spectroscope
A spectrum of no lines and no bands
Bright light/ emission spectra
A unique line spectrum emitted by each element based on the different number of electrons they each possess.
Brightness and width of bands indicates how many photons of that wavelength are given off
Movement of excited electrons
Atomic emission spectra
spectral lines are produced by an atom in the excited state.
Absorption of energy (electricity)
Electrons are raised to a higher energy level (orbital)
Electrons lose energy as they come back to lower level and that energy is given off as a photon (light wavelength)
Heinsenberg Uncertainty Principle
At any one time it is impossible to calculate both the momentum and the location of an electron in an atom. It is possible to calculate the probability of finding an electron in a given space.
Number of electrons in each sublevel
s= 2, p=3, d=5, f=7
therefore, s= 2, pX2=6, dX2=10, fX7=14
Aufbua Principle
Each electron occupies the lowest energy orbital available
All orbitals in the same sublevel have the same energy
The energy levels within a principal energy level have different energies (EX: 2p has more energy than 2s)
Orbitals related to energy sublevels within one principal energy level can overlap orbitals related to energy sublevels within another principal level (EX: 4se- have less energy than 3de-)
Pauli exclusion
A maximum of 2 electrons may occupy a single atomic orbital, but only if the electrons have opposite spin (are in opposite directions)
Hund’s rule
Single electrons with the same spin must occupy each equal-energy orbital before additional electrons with opposite spins can occupy the same orbitals.