The dark lines are absorption spectrum, the energy absorbed by Atoms in the atmosphere of the star. ================================ Fraunhofer's spectral lines.
Object lines are dark, thick lines used to define an object.
The dark lines reveal the atoms that are associated with the stars atmosphere. The dark lines are atom energy absorption signatures.
The dark lines represents the absorption of energy at that frequency, E=hf.
Yes!
dark-line spectrum...
Fraunhofer realised that some of these dark lines were at the same position in effect called the Zeeman effect can also cause splitting of the spectral lines.
Rivers
The dark lines in a star's spectrum are caused by absorption of specific wavelengths of light by the elements in the star's outer atmosphere. This absorption occurs when the elements in the atmosphere absorb photons of specific energies, leading to the creation of dark absorption lines in the spectrum.
Dark lines in the spectrum were named after German physicist Joseph von Fraunhofer, who first systematically studied them. They are commonly known as Fraunhofer lines and are formed when certain chemical elements absorb specific wavelengths of light, creating dark bands in the spectrum.
A spectroscope is a tool that separates a star's light into color bands and dark lines (absorption lines). These dark lines are produced due to the absorption of specific wavelengths of light by elements in the star's atmosphere. Spectroscopes are important in studying the composition and characteristics of stars.
Dark blue jersey with a white collar and light blue shoulders and breast