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.
A spectral line refers to the distinct lines in a spectrum that correspond to specific wavelengths of light emitted or absorbed by atoms or molecules. For example, astronomers analyze the spectral lines of distant stars to determine their composition and temperature.
Astronomers have detected a quasar in a distant galaxy.
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.
The instrument used to see distant objects is called a telescope. Telescopes collect and magnify light from distant celestial bodies, allowing astronomers to observe stars, planets, and galaxies that are far away. There are various types of telescopes, including optical, radio, and infrared, each designed for specific wavelengths of light.
Satellites and space probes provide astronomers with access to data from space that cannot be obtained from Earth, such as images in different wavelengths or information about distant objects. They also allow for exploration of distant celestial bodies and regions that are not easily accessible using ground-based telescopes. These tools help astronomers study the universe more comprehensively and advance our understanding of the cosmos.
Spectroscopy.
Astronomers primarily use telescopes to observe distant stars. These can be optical telescopes, which capture visible light, or radio telescopes that detect radio waves emitted by celestial objects. Additionally, space-based observatories like the Hubble Space Telescope provide clearer views by avoiding Earth's atmosphere, while instruments like spectrometers analyze the light from stars to determine their composition, temperature, and motion.
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.
en.wikipedia.org/wiki/Spectroscopy
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.
An instrument used to measure stars is called a spectrometer. It analyzes the light emitted or absorbed by stars, allowing astronomers to determine their composition, temperature, distance, and velocity. Another important tool is the telescope, which magnifies distant celestial objects, enabling precise observations and measurements of stars’ positions and brightness. Together, these instruments enhance our understanding of the universe.
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.
Astronomers can determine the expansion of the universe by observing the cosmic background radiation, and the red- or blue-shifting of distant objects.
A spectral line refers to the distinct lines in a spectrum that correspond to specific wavelengths of light emitted or absorbed by atoms or molecules. For example, astronomers analyze the spectral lines of distant stars to determine their composition and temperature.
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?
A crucial tool for astronomers is the telescope, which allows them to observe distant celestial objects and gather important data about their properties. Telescopes come in various types, including optical, radio, and space-based, each designed for specific wavelengths of light. By using these instruments, astronomers can study the universe's composition, structure, and evolution, leading to significant discoveries about galaxies, stars, and planets.
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.