Objectives
1. Explain why scientists know the identity of the chemical compositions of stars
2. Describe a flame test
3. Describe the Bohr model in terms of energy
Atoms can absorb and release energy
When atoms release energy they emit light
Each atom emits only a certain frequency of light
Shell(Bohr) model A region of space around the atomic
nucleus where electrons may be
Each shell can hold a limited amount of electrons
Series of seven shells accounts for the seven periods
Number of electrons held in each period is equal to the shell’s capacity for electrons
Valence Electrons Electrons in the outermost shell “combining
power”
Directly exposed to the external environment
The first to interact with other atoms
When electrons absorb energy they get excited and jump around
When jump back to the original position they release that energy as light
Atomic Spectrum Light from atoms consist of a
number of individual frequencies
Pattern of frequencies of a particular element – atomic spectrum
White light separates into its color components by a prism
Each color corresponds to a different frequency of electromagnetic radiation
Atomic spectrum – atoms “finger print”
Emission – the frequencies the gas emitts Absorption – frequencies of all white light
EXCEPT those that are absorbed by the gas
http://jersey.uoregon.edu/vlab/elements/Elements.html