Because the bright line spectrum is generated by the transition of electrons in the atom
among higher and lower energy levels, and no other atom of any other element has less
than one electron in it.
No, an absorption spectrum and a bright line spectrum are not the same. An absorption spectrum is produced when light is absorbed by atoms or molecules, showing dark lines at specific wavelengths. On the other hand, a bright line spectrum is produced when atoms or molecules emit light at specific wavelengths, creating bright lines in the spectrum.
A bright line spectrum refers to the pattern of distinct and bright lines of different colors that are produced when an element is excited and emits light. Each element has a unique bright line spectrum that can be used to identify the element through spectroscopy.
If you shine white light through a prism, you always get the same result - a spectrum. However, if the environment is brightly lit, you may not see the spectrum as it will be too faint compared to the brightly lit background.
Red, blue, green, and violet are found in the emission spectrum of hydrogen.
The bright lines in a bright light spectrum, known as emission lines, indicate the specific wavelengths of light emitted by excited atoms or molecules when they return to a lower energy state. Each element produces a unique pattern of emission lines, allowing scientists to identify the elements present in a light source.
Emission spectra are bright-line spectra, absorption spectra are dark-line spectra. That is: an emission spectrum is a series of bright lines on a dark background. An absorption spectrum is a series of dark lines on a normal spectrum (rainbow) background.
Sunlight produced spectrum is continuous and contains a broad range of wavelengths, while hydrogen gas produced spectrum consists of discrete lines at specific wavelengths due to the unique energy levels of hydrogen atoms. Sunlight spectrum is continuous due to the various processes that produce light, whereas hydrogen gas spectrum is a result of the energy levels of hydrogen atoms emitting photons of specific wavelengths.
In a continuous spectrum, you see every color in visible light from wavelengths around 380 nm to 780 nm. The bright light spectrum has only light at specific wavelengths, forming narrow regions of lights. This is characteristic of a particular substance, emitting these lights from its unique electron configuration. Light at specific wavelengths is emitted for different substances, but not a continuous rainbow.
Dark-line spectrum is a "photo-negative" of emission spectrum. It is the gaps that appear in precisely the same location as corresponding bright lines. produced by a cool gas with a hot solid and you
There are no bright lines and no dark lines in the spectrum, incandescent light has a continuous spectrum with all visible colors present
If the enviorment is brightly lit, you may not see the spectrum as it will be too faint compared to the brightly lit background.
The range of colors that makes up white light is called the visible light spectrum. This spectrum includes all the colors of the rainbow, from red to violet. Brightness refers to the intensity of light, not to the range of colors present.