Unit 3 Flashcards
Electromagnetic Spectrum
the full range of electromagnetic radiation, organized by frequency or wavelength
En (total energy of nth state)
En= (-2.18 x 10^-18 J)(z^2/n^2)
or
En= (-13.6 eV)z^2/n^2)
Z
atomic number, the charge number of an atomic nucleus
eV (electric volt)
1.602 x 10^-19 J
a0
a0= 52.9 pm
Bohr radius (the most probable distance between the nucleus of a hydrogen atom and its single electron when the atom is in its ground state (lowest energy level))
pm
1 x 10^-12 m
rn
-rn= (n^2/z) x a0
-radius of orbit of electron when atom is in nth state
spectrum of incoming light
the distribution of different wavelengths of light (colors) that are hitting a substance
distinct energy
the concept that electrons in an atom can only occupy specific, fixed energy levels, meaning they can only have certain distinct values of energy, not a continuous range of energies
line in spectrum
each line represents a unique λ
spectrum of elements
each element has a unique spectrum
Bohr’s model of the atom
-atoms exist in discrete or quantized states
-these energy states are described by a quantum number (n=1, 2, 3,…)
-atom transitions between energy states in quantum leaps
-energy is conserved, the energy of the quantum leap is the energy of the photon emitted or absorbed by the atom
-Bohr’s energy equation is applied to one electron atoms/ions
-total energies of bound states are negative and conserved
quantum leap
a huge, often sudden, increase or advance in something
emission
-Eph= -∆E(atom)
-atom loses energy
-atom becomes more stable
absorption
-Eph=∆E(atom)
-atom (ion) gains energy
-atom becomes less stable