Some spectral lines are brighter than others due to variations in the intensity of light emitted or absorbed by different elements or molecules at specific wavelengths. Factors such as population levels of excited states, the abundance of the element in the source, and the conditions under which the light is emitted, such as temperature and pressure, can influence these intensities. Additionally, certain transitions may be more probable or allowed than others, leading to stronger emissions or absorptions. Consequently, this results in a spectrum where some lines appear more prominent than others.
'Appear' would become 'appeared' in the past tense so the sentence would simply be 'some stars appeared to be brighter than others'.
Because some are larger than others and some are closer than others.
Stars look brighter than others due to factors such as their size, temperature, and distance from Earth. A larger and hotter star will appear brighter, as will a star that is closer to us. The brightness of a star as seen from Earth is measured by its apparent magnitude.
If there is a star shining through the gas then some of the starlight will be absorbed by the gas to deliver spectral lines of the "stuff" making up the gas.
Stars appear brighter depending on their size, temperature, and distance from Earth. Larger and hotter stars emit more light, making them appear brighter. Additionally, stars that are closer to Earth will appear brighter than those that are farther away.
Different quantities of the materials producing the lines.Some lines are weaker because the electron transitions producing them are less likely.Some lines are stronger or weaker depending upon the temperature of the material producing the lines (a big issue in determining stellar spectral classes).Different quantities of the materials producing the lines. Some lines are weaker because the electron transitions producing MORE?The distribution of photon energies, which have a peak at a wavelength that depends on temperature (ref. 1).Also differing amounts or concentrations of the elements responsible for those lines.
Elements have several spectral lines and although some lines may be the same between different elements most lines are not and the whole spectrum for each element is indeed unique.
'Appear' would become 'appeared' in the past tense so the sentence would simply be 'some stars appeared to be brighter than others'.
Because some are larger than others and some are closer than others.
Three possibilities: It is brighter (some are brighter than others), it is bigger, or it is closer to earth.
In a spectral line from a rotating body such as a star, some of the matter emitting the line is moving toward you and has a part of its line shifted slightly to the bluer end of the spectrum, some is moving away and has a slight shift toward the red end, and the rest is moving more or less across your line of sight and the shift is normal.
Fraunhofer realised that some of these dark lines were at the same position in effect called the Zeeman effect can also cause splitting of the spectral lines.
In absolute terms, some are brighter than our Sun - in some rare cases, millions of times brighter - while others are much less bright than our Sun.
No it is not. It is less bright than some, but brighter than others.
Stars look brighter than others due to factors such as their size, temperature, and distance from Earth. A larger and hotter star will appear brighter, as will a star that is closer to us. The brightness of a star as seen from Earth is measured by its apparent magnitude.
If there is a star shining through the gas then some of the starlight will be absorbed by the gas to deliver spectral lines of the "stuff" making up the gas.
Some star characteristics that can be identified by spectral analysis include temperature, composition, mass, luminosity, and age. By analyzing the lines present in a star's spectrum, astronomers can determine these key properties and gain insights into the star's physical characteristics and evolutionary stage.