S.1.3.1 and S.1.3.2 Emission Spectra Flashcards
Continuous spectrum
Contains light of all wavelengths and all frequencies
Line spectrum
Contains selected frequencies; gaps in the spectrum
Spectrometry
Light interacting with matter
Light
All waves on the electromagnetic spectrum (waves of energy)
What does adding energy to electrons do?
Allows electrons to overcome the electrostatic attractive forces and move to the next shell
Attractive forces keep electrons as close to the nucleus as possible
Emission spectrum
A hot gas is placed in front of a prism and produces a line spectrum on a black background
Absorption spectrum
A cold gas is placed between a prism and a light source and produces a line spectrum with gaps on the background of a continuous spectrum
Electromagnetic radiation
Emitted in different forms of differing energies; travels at the speed of light; can be distinguished by different wavelengths
Frequency
Number of waves that pass a particular point in a second
Relationship between frequency and wavelength
Inversely proportional
Electron in the excited state
Unstable, immediately returns to ground state by giving out energy in the form of electromagnetic radiation
Photon
Packet of energy released for each electron transition between energy levels
IMPORTANT!
No answer needed
Gases produce a characteristic emission line spectrum when heated to a high temperature
Energy of photon
Proportional to the frequency of the radiation
E = hf
Quantization
The idea that electromagnetic radiation comes in discrete packets (quanta)