What are emission line stars?
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What are emission line stars?
An emission-line star is a star whose spectrum exhibits emission lines in the optical spectra. Common types include: Be star. Herbig Ae/Be star. Shell star.
Do emission lines come from stars?
Emission lines are usually seen as bright lines, or lines of increased intensity, on a continuous spectrum. This is seen in galactic spectra where there is a thermal continuum from the combined light of all the stars, plus strong emission line features due to the most common elements such as hydrogen and helium.
Why do stars have emission lines?
When a hydrogen cloud gives off light, it gives off light exactly the same color as the cloud absorbs. If the cloud gives off more light than it absorbs, the spectrum at the left will have a peak instead of a valley. These peaks are called “emission lines,” because the cloud emits light.
What are the dark lines in the spectra of stars called?
Fraunhofer lines, in astronomical spectroscopy, any of the dark (absorption) lines in the spectrum of the Sun or other star, caused by selective absorption of the Sun’s or star’s radiation at specific wavelengths by the various elements existing as gases in its atmosphere.
WHAT IS a emission line?
Definition of emission line : a bright line in the emission spectrum of a gas or vapor — compare absorption line.
How are emission lines formed?
Emission lines occur when the electrons of an excited atom, element or molecule move between energy levels, returning towards the ground state. The spectral lines of a specific element or molecule at rest in a laboratory always occur at the same wavelengths.
What is an emission line?
Why do stars have dark lines in their spectra?
9) Stars have dark spectral lines because gases in the star’s atmosphere absorb specific wavelengths (colors) of light from the full spectrum of light coming from it’s surface.
How emission lines are formed?
Why are there dark lines in the spectrum of light emitted by stars?
Why are there dark spots on the spectrum of light emitted by stars? Some wavelengths of light are absorbed by the elements in the star’s outer atmosphere.
What are absorption and emission lines?
Emission lines refer to the fact that glowing hot gas emits lines of light, whereas absorption lines refer to the tendency of cool atmospheric gas to absorb the same lines of light. When light passes through gas in the atmosphere some of the light at particular wavelengths is scattered resulting in darker bands.
What are emission and absorption lines?
Do stars have an emission or absorption spectrum?
Stars have absorption line spectra. We can think of stars as a hot continuum source with a “cool” atmosphere of absorbing gas. The wavelengths that get absorbed depend on the chemical make up of the gas in the stellar atmosphere.
Why do stars have different absorption lines?
Stars have plenty of “cold” gas (atoms in their ground states). If you put some gas on the way from a light source to you, some frequencies will be less represented (dark absorption lines) than non resonance frequencies.
What is emission lines in physics?
Learn about this topic in these articles: …a pattern is called an emission, or bright-line, spectrum. When light passes through a gas or cloud at a lower temperature than the light source, the gas absorbs at its identifying wavelengths, and a dark-line, or absorption, spectrum will be formed.
What do the lines in the spectrum reveal about the stars?
From spectral lines astronomers can determine not only the element, but the temperature and density of that element in the star. The spectral line also can tell us about any magnetic field of the star. The width of the line can tell us how fast the material is moving.
Where are emission lines found?
Do stars have emission and absorption lines?
What type of spectrum do most stars emit?
The spectrum of a star is composed mainly of thermal radiation that produces a continuous spectrum. The star emits light over the entire electromagnetic spectrum, from the gamma rays to radio waves. However, stars do not emit the same amount of energy at all wavelengths.
Does stars have emission or absorption spectrum?