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Spectroscopy is the systematic study of spectra and spectral lines. Spectral lines are used to provide evidence about the chemical composition of distant objects. So the answer to your question is through spectroscopy.. not spectrometry like the previous editor posted.

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15y ago

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What are the methods that astronomers use to identiy the composition of distant stars?

Spectroscopy.


How does a spectroscope enable astronomers to determine the characteristics of distant stars and galaxies?

en.wikipedia.org/wiki/Spectroscopy


Why is Newton's version of Kepler's third law so useful to astronomers?

Newton's version of Kepler's third law, which relates the orbital period and distance of a celestial body to its mass, allows astronomers to calculate the mass of celestial objects such as planets, moons, and stars. This is crucial for understanding the dynamics of the solar system and other celestial systems. Additionally, it provides a framework for studying gravitational interactions between celestial bodies.


Why astronomers have difficulty looking at distant stars except?

Astronomers have difficulty looking at distant stars because while we have highly specialized telescopes, they are in constant contention with various other celestial bodies. In addition to this, the light of distant stars takes hundreds of thousands of years to reach us, making it impossible to get a current look at a distant star.


How can astronomers tell what a distant object is made of?

Astronomers are able to identify chemicals in distant space with the use of spectral analysis. This breaks the light apart into a spectrum and find either emission lines or absorption lines and identifies which elements are present.


How can astronomers infer approximately how long the universe has been expanded?

Astronomers can determine the expansion of the universe by observing the cosmic background radiation, and the red- or blue-shifting of distant objects.


How does the light that astronomers see from distant stars and galaxies tell htem that the same atoms with the same properties exist throughout the universe?

We determine the types of elements contained in the star or within the corona by analyzing the spectrum of the light we receive. Each element will radiate at a set of specific discreet frequencies, and the frequencies they radiate tell us what the element is, and how deeply ionized it is. The spectral analysis is exact; we can even determine the proportions of the elements that we see by the relative brilliance of their light. But there IS one thing that the spectrum cannot tell us; is this a normal matter star, or an anti-matter star?


Quasar in a sentence?

Astronomers have detected a quasar in a distant galaxy.


Why might astronomer would most likely use the principles of chemistry?

An astronomer would use the principles of chemistry to determine the chemical components of distant planets and stars. The most useful discipline is that of spectral analysis. This is the identification of chemical compounds by their actions on various wavelengths of light.


What is the quasar method?

The quasar method is a technique used in astrophysics to estimate the distances to distant celestial objects. It involves observing the spectra of quasars, which are extremely bright and distant objects, to determine the redshift caused by the expansion of the universe. By comparing the redshift of a quasar with known properties to that of a target object, astronomers can infer the distance to the target object.


What is the rotational period of the Celestial Sphere in hours and how would you determine that?

The rotational period of the celestial sphere is simply the reflection of Earth's rotation; therefore, it rotates once every 23 hours and 56 minutes. You can determine that by observing the apparent movement of distant stars.


What information can we determine from the light of distance objects?

From the light of distant objects, we can determine properties such as their distance, composition, temperature, and motion. By analyzing the light's spectrum, astronomers can infer the chemical elements present in the object and its velocity towards or away from us (Doppler effect). Additionally, the brightness of the object's light can provide clues about its size and luminosity.