An absorption spectrum can tell the astronomer or physicist what elements are in the starlight being observed. A diffraction grating is used to split the incoming light into a spectrum of colors. Sodium, for example, causes dark Fraunhofer lines at known points in the visible spectrum. Helium was discovered in the solar spectrum by Bunsen and Kirchoff using this technique. Hence the name derived from Helios for the Sun.
Composition of the gases. It can provide the relative amounts, temperature and pressure of the gases. It can also tell us about the stars magnetic field, and overall rotation.
scientists can tell the stars composition and temperature from its spectrum. Hope tht helps :]
Its elemental composition.
The light spectrum coming from the planet. Each element has its own distinct color spectrum.
Hubble
Stars can range from blue to red depending on temperature and mass, with yellow stars in the middle and white stars on the back end of the spectrum.
composition (and) temperature.
Infrared
All stars radiate infra-red along with the rest of the spectrum.
The spectrum produced by solid is continuous spectrum. Continuous spectrum is formed by all, solid liquid and gases if the pressure is high. In case of low pressure, gases produce line spectrum.
absorption spectrum
scientists can tell the stars composition and temperature from its spectrum. Hope tht helps :]
The differences in spectrum are mainly due to: * Differences in temperature between the stars * Differences in chemical composition * Differences in relative movement (redshift / blueshift, due to the Doppler effect)
stars are not magic they are just gases
Mostly gases
The spectrum is a kind of analysis of the light emitted by a star.
scientists can tell the stars composition and temperature from its spectrum. Hope tht helps :]
Its elemental composition.