The dark lines reveal the atoms that are associated with the stars atmosphere. The dark lines are atom energy absorption signatures.
Scientists determine a star's temperature by analyzing its spectrum of light. The color and intensity of certain lines in a star's spectrum reveal its temperature. Hotter stars appear blue or white, while cooler stars appear red.
A star's dark line spectrum reveals the elements present in its atmosphere. Each dark line corresponds to a specific element that has absorbed light at that particular wavelength, providing a fingerprint of the star's chemical composition. By analyzing these lines, astronomers can determine the types and abundances of elements in the star.
scientists can tell the stars composition and temperature from its spectrum. Hope tht helps :]
A prism, a lot of droplets...
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)
Most stars exhibit a continuous spectrum, which contains all wavelengths of light in a continuous distribution. This is often referred to as a blackbody spectrum due to its smooth curve.
scientists can tell the stars composition and temperature from its spectrum. Hope tht helps :]
Its elemental composition.
It's color.
Orange stars have a K-type spectrum with a wide distribtion of brightness.
spectrum, which can reveal information about the composition and properties of the object it originated from.
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.