The bright line emission spectrum tells us the amount of energy between the exited and ground state. When electrons move from an exited state to a ground state, radiant energy of a specific frequency is emitted this creates spectral lines.
dark line spectrum
scientists can tell the stars composition and temperature from its spectrum. Hope tht helps :]
to identify elements
The bright line spectrum is useful because it shows us the different particles in the elements.
The spectrum of sunlight is continuous while for hydrogen is line spectrum (discontinuous)
dark line spectrum
scientists can tell the stars composition and temperature from its spectrum. Hope tht helps :]
The lines in a spectroscope tell what element(s) are being observed. The continuous color are background noise or put there for a reference.
to identify elements
how can you tell if an object is reflecting blue light from a star
Lippershey first discovered a dark-line spectrum.
Line Spectrum
No, its an absorption spectrum
The emission spectrum of a star is the spectrum of frequencies for emitted electromagnetic radiation during the transition of an atom's electrons from a high-energy state to a low-energy state. The emission spectrum can differ depending on the temperature and composition of the star.
it does your mom
The bright line spectrum is useful because it shows us the different particles in the elements.
Dark lines especially in solar spectrum have been named as Fraunhofer lines. These line are good examples for line absorption spectrum