Webb image archive

Types of Spectra: Continuous, Emission, and Absorption

Scientists often classify spectra based on the key light–matter interactions they represent and how they are used.   Continuous Spectrum: A continuous spectrum contains all wa...

Date
Dec 13, 2023
Observatory
James Webb Space Telescope
Credit
NASA / ESA / CSA / STScI
Archive ID
01F8GF8DK2PRY4FP9DA2XPQC8S

Scientists often classify spectra based on the key light–matter interactions they represent and how they are used.  

Continuous Spectrum: A continuous spectrum contains all wavelengths of light in a certain range. Hot, dense light sources like stars, for example, emit a nearly continuous spectrum of light, which travels out in all directions and interacts with other materials in space. The broad range of colors that a star emits depends on its temperature. 

Absorption Spectrum: When starlight passes through a cloud of gas, some of the light is absorbed and some is transmitted through the gas. TThe wavelengths of light that are absorbed depends on what elements and compounds it is made of. An absorption spectrum has dark lines or gaps in the spectrum corresponding to wavelengths that are absorbed by the gas.

Emission Spectrum: Starlight can also heat up a cloud of gas, exciting the atoms and molecules within the gas, and causing it to emit light. The spectrum of light that a cloud of gas emits depends on its temperature, density, and composition. An emission spectrum consists of a series of colored lines that correspond to wavelengths emitted by the glowing gas.

Credits

Illustration

NASA, ESA, Leah Hustak (STScI)

Google Preferred Sources

See more from Space Telescope in Google

Choose Space Telescope as a preferred source to make our mission news, visual reporting, and independent explainers easier to find in Google Search.