By observing far away stars in our galaxy through a spectroscope, we are able to see the spectrum that appears from the substances in these stars. Each element has a unique spectrum when light is shone through it, so we are able to determine what elements make up certain stars.
The star's spectrum can tell you the relative motion of the star either toward or away from the viewer (you can tell by means of the Doppler shift), the temperature of the star, and the chemical composition of the star.
The composition of the star (elements that make up the star) can be determined by light split into its spectrum via spectroscopy.
Its distance from Earth can also be determined, relative to variable stars, supernovae, and other "standard candles".
Once can also determine how it is moving, what gravitational sources may be nearby, and what strong gravitational sources may lie between the star and the observer (all due to effects visible by its motion and relativistic gravitational lensing).
the temperature of a star
Primarily, it's spectrum (it's light seen through a spectrograph).
Spectroscopy shows what elements are present in the star, it's chemical composition. The different elements give off different energy signatures through radiation, which relate to the wavelength and therefore colour.
That's done by analyzing the star's spectrum.
The temperature of a star is determined for it's colour spectrum. The hotter the star the more the spectrum is towards blue where as a cooler star has a spectrum closer to red.
binary star systems
The star is moving away fro where it is. ~Justine... :))
Primarily, it's spectrum (it's light seen through a spectrograph).
love
Spectroscopy shows what elements are present in the star, it's chemical composition. The different elements give off different energy signatures through radiation, which relate to the wavelength and therefore colour.
That's done by analyzing the star's spectrum.
The temperature of a star is determined for it's colour spectrum. The hotter the star the more the spectrum is towards blue where as a cooler star has a spectrum closer to red.
Atoms in the atmosphere of the star is responsible for the dark lines in its spectrum.
No, a spectrum of light with no gaps can not be achieved.
if you are observing a star 100 light years away, you are looking at it as it was 100 years ago.
By the star's spectrum.
By the color.
They analyze the star's spectrum. Each element produces characteristic lines in a spectrum.