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What else can I help you with?
The spectral lines from distant galaxies do not match spectral lines on Earth due to?
The spectral lines from distant galaxies do not match those on Earth because of the Doppler effect, cosmic expansion, and differences in elements present in the galaxies. These factors cause the observed spectral lines to be shifted or altered compared to what we see on Earth.
How do stellar spectra provide evidence that stars are actually moving?
Stellar spectra provide evidence of star motion through the Doppler effect, which causes shifts in the wavelengths of light emitted by a star. If a star is moving towards us, its spectral lines shift towards the blue end of the spectrum (blueshift), while a star moving away from us exhibits a redshift, where spectral lines shift towards the red end. By analyzing these shifts in the spectral lines, astronomers can determine the velocity and direction of a star's movement relative to Earth. This technique has been crucial for understanding the dynamics of stars within galaxies and the expansion of the universe.
Why do stars of spectral class M not show strong lines of hydrogen in their spectra?
Stars of spectral class M have cooler temperatures compared to stars of other spectral classes, causing their hydrogen lines to weaken and be less prominent in their spectra. The lower temperature results in lower energy levels, making it more difficult for hydrogen atoms to transition between energy levels and emit or absorb light in the hydrogen spectral lines.
What diagram best represents the pattern of spectral lines from the same element when it was observed by Edwin Hubble in the light of one of the distant galaxies?
The best diagram to represent the pattern of spectral lines from the same element observed by Edwin Hubble in the light of distant galaxies is the redshift spectrum. This spectrum shows the spectral lines of elements shifted toward longer wavelengths (redshifted) due to the Doppler effect, indicating that the galaxies are moving away from us. The pattern of these lines remains consistent with the element's known absorption or emission spectrum, but the entire set of lines shifts uniformly to the red, reflecting the expansion of the universe.
What particle is responsible for spectra?
Spectra are produced by interaction of electromagnetic radiation with matter, typically atoms or molecules. The particle responsible for spectra is the photon, which carries energy and interacts with electrons in the atoms or molecules to produce the spectral lines observed in both emission and absorption spectra.
The spectra of most galaxies show redshifts this means that their spectral lines?
have wavelengths that are longer than normal:)
The spectral lines from distant galaxies do not match spectral lines on Earth due to?
The spectral lines from distant galaxies do not match those on Earth because of the Doppler effect, cosmic expansion, and differences in elements present in the galaxies. These factors cause the observed spectral lines to be shifted or altered compared to what we see on Earth.
How are elements identified fro bright line spectra?
Elements are identified from bright line spectra by comparing the observed spectral lines with known emission spectra of elements. Each element emits a unique set of spectral lines due to the characteristic energy levels of its electrons. By matching the observed lines with known patterns, scientists can determine the elements present in a sample.
How would the spectra from galaxies appear?
They have broad emission lines of highly ionized elements.
The spectral lines of elements when observed in distant galaxies show a shift towards?
The red end of the spectrum.
Why do stars of spectral class M not show strong lines of hydrogen in their spectra?
Stars of spectral class M have cooler temperatures compared to stars of other spectral classes, causing their hydrogen lines to weaken and be less prominent in their spectra. The lower temperature results in lower energy levels, making it more difficult for hydrogen atoms to transition between energy levels and emit or absorb light in the hydrogen spectral lines.
What is meant by the statement spectra lines are the fingerprints of elements?
Spectra lines are specific wavelengths of light emitted or absorbed by elements. Each element has a unique set of spectral lines, which allows scientists to identify elements present in a sample by comparing the observed spectra to known patterns, similar to how fingerprints are unique to individuals.
Who first discovered redshift?
The discovery of redshift in the spectra of light from distant galaxies was made by astronomer Vesto Melvin Slipher in the early 20th century. He noticed that many galaxies appeared to be moving away from us based on the shift of their spectral lines towards the red end of the spectrum. This laid the foundation for the theory of the expanding universe.
What is the Wavelength barium?
Barium has an atomic spectra of lines, not only one line (with one wavelength); I reccomend to consult a catalog of spectral lines. See the link below.
Why can you use line spectra to measure the speed of galaxies?
The Doppler effect changes the position of well-known lines.
Why do atomic spectra show individual lines instead of continuous spectra?
Atomic spectra show individual lines instead of continuous spectra because each line corresponds to a specific energy level transition of electrons within the atom. When electrons move between energy levels, they emit or absorb energy in the form of light at specific wavelengths, creating distinct spectral lines. This results in the observed pattern of individual lines in atomic spectra.
What particle is responsible for spectra?
Spectra are produced by interaction of electromagnetic radiation with matter, typically atoms or molecules. The particle responsible for spectra is the photon, which carries energy and interacts with electrons in the atoms or molecules to produce the spectral lines observed in both emission and absorption spectra.
