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Q: How do astronomers determine the elements present in a star?
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How do astronomers identify elements of the stars?

Elements are identified based on their absorption spectra. Every element absorbs a unique set of frequencies when light passes through it. Scientists can determine which elements are present based on which portions of the star's light are absorbed.


What can a stars spectrum tell astronomers about a star?

What elements the star is made of.


What would be a common task for astronomers?

using a telescope to determine the coordinates of a star


How star made of?

Our Sun is about 70% Hydrogen and 28% Helium by mass, with traces of heavier elements. Other stars can be a little different, but with a spectrometer, scientists are able to determine the elements that are present in any star.


What Elements Are Present In The Star Sirius?

Hydrogen and helium are the most abundant elements in a star.


How do scientists determine the element present in a star?

By the star's spectrum.


How do astronomers determine if a star is moving towards or away from us?

They use a tool called a SPECTROSCOPE.


If Astronomers observe a typical star using a telescope and a spectrometer they will be able to determine what?

i have no idea but it uytr


How can astronomers determine whether a star is moving toward or a way from earth?

They can do so by examining the light from the star. Doppler shift can indicate this


What does the spectrum of a star determine?

Elements that exist in the start


How are stars made of?

Our Sun is about 70% Hydrogen and 28% Helium by mass, with traces of heavier elements. Other stars can be a little different, but with a spectrometer, scientists are able to determine the elements that are present in any star.


How can astronomers infer which elements are are found in a star?

Atoms in a star's corona are subjected to extremely high levels of energy from the photosphere. This energy excites electrons in the atoms, and causes the electrons to jump up to a higher energy state. When the electrons fall back to their rest state, they emit photons at a very specific set of wavelengths unique to each element. By examining the wavelengths of light coming from a specific star (in a process called astronomical spectroscopy) astronomers are able to decipher with complete certainty which elements are present in that star. . For example, hydrogen emissions are known to occur at 410.2nm (violet), 434.1nm (violet), 486.1nm (blue-green), and 656.3nm (red). When a star is seen to emit a combination of those wavelengths, astronomers can be certain hydrogen is present in the star under observation. . See the related link below for more information on emission spectra.