preguntale un scientist por que yo no se
Ok who ever wrote the above, get a life because if you write that as an answer it waist everybody else's time.
Ok the answer is they look at what color the star is using a telescope that determines about how hot it is and then they use a spectra of dark lines to determine the elaments it is composed of.
spectroscopy.
This branch of chemistry uses the colour, and likewise, the wave length of light to determine what chemicals are present during combustion. When compounds are heated, the electrons move between discreet energy levels, and when an electron decreases in energy, it emits radiation, often in the form or visible light. The wavelengths can then be separated and examined with a device called a spectrometer. Neat stuff.
As for the temperature, I'm pretty sure the type of material burning is important fact one, and I would assume important fact 2 for calculating temperature would be mass. The more mass being compacted, the more friction, the more heat there will be. That's just a guess though.
the light radiated from the stars
Yes
To determine a star's luminosity is from size and temperature.
Stars are classified by four different characteristics. Apparent magnitude (brightness) and absolute magnitude (how bright it would appear at 10 parsecs from the earth). Luminosity, another measure of brightness, compares the star to the sun's brightness. Spectral classifications are measured by the star's temperatures. Finally stars are signed a number by scientists through the Morgan-Keenan System.
brightness
the light radiated from the stars
scientists can tell the stars composition and temperature from its spectrum. Hope tht helps :]
Light wavelength and light spectrum i believe.
To determine the chemical composition of stars, scientists look at what's called the emission spectrum of the stars, which can be obtained from the light coming from the stars. Thin lines are observed in different parts of the spectrum, which correspond to different chemicals. In other words, the lines are like fingerprints of chemicals. By looking at these fingerprints, one can determine what type of chemicals are present in the star. To determine the surface temperature of stars, we use the Wien's Law. It states that: Peak wavelength x Surface Temperature = 2.898x10-3 Peak wavelength can be determined by looking at the light coming from the star in question. It is the wavelength with the highest intensity.
scientists can tell the stars composition and temperature from its spectrum. Hope tht helps :]
The purpose of stellar spectroscopy is to determine the chemical composition of stars, the temperature and some other characteristcs..
Scientists can learn the composition of a star from the amount and types of electromagnetic radiation, including light, that it gives off. Additionally, scientists can determine the rate of nuclear fusion from the amount of light released per unit of time.
Scientists study stellar spectra to learn about their properties such as temperature, chemical composition and relative chemical abundances, radial velocity, rotational speed etc.
Yes
Size and temperature determine the brightness of stars.
To determine a star's luminosity is from size and temperature.
Stars are classified by four different characteristics. Apparent magnitude (brightness) and absolute magnitude (how bright it would appear at 10 parsecs from the earth). Luminosity, another measure of brightness, compares the star to the sun's brightness. Spectral classifications are measured by the star's temperatures. Finally stars are signed a number by scientists through the Morgan-Keenan System.