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.
The dark lines in a star's spectrum are caused by absorption of specific wavelengths of light by the elements in the star's outer atmosphere. This absorption occurs when the elements in the atmosphere absorb photons of specific energies, leading to the creation of dark absorption lines in the spectrum.
The dark lines that appear in a spectrum of light from a star are called absorption lines. These lines are caused by the absorption of specific wavelengths of light by elements in the outer atmosphere of the star. Absorption lines help astronomers identify the chemical composition of stars and other celestial objects.
No. The red shift simply means that the absorption lines of elements such as hydrogen and helium are shifted towards the red end of the spectrum. A very hot star would normally appear blue. If it were relatively near the earth and so receding relatively slowly, the spectrum would still be blueish, rather than red.
some of the light from the corona produces a continuous spectrum that lacks absorption lines. however the type is absorption spectrum
The absorption spectrum of an atom shows that the atom emits that spectrum which it absorbs.
The absorption spectrum of boron typically shows strong absorption in the ultraviolet region, with some absorption in the visible spectrum as well. Boron's absorption spectrum is characterized by a series of sharp peaks due to transitions between energy levels in its atomic structure.
In the absorption spectrum the peaks are due to preferential absorption at a definite wavelength by molecules, ions, etc.
Emission spectrum: lines emitted from an atom.Absorption spectrum: absorbed wavelengths of a molecule.
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.
An absorption spectrum shows dark lines at specific wavelengths where light has been absorbed by a substance. A continuous spectrum shows all colors/wavelengths with no gaps, like the rainbow. The main difference is that the absorption spectrum has specific dark lines while the continuous spectrum is smooth and uninterrupted.
The absorption spectrum shows the wavelengths of light that are absorbed by a substance. Each substance has a unique absorption spectrum due to its molecular structure and composition. The absorption spectrum is determined by measuring the amount of light absorbed at different wavelengths.
An absorption spectrum is a graph that shows how much light is absorbed by a substance at different wavelengths. It appears as a series of peaks and valleys. Scientists use absorption spectra to identify the chemical composition of a substance, study its properties, and understand its behavior in various conditions.
The number of lines in the emission spectrum is the same as in the absorption spectrum for a given element. The difference lies in the intensity of these lines; in emission, they represent light being emitted, while in absorption, they represent light being absorbed.
Dark lines in an absorption spectrum are called absorption lines. These lines correspond to wavelengths of light that have been absorbed by specific elements or molecules in the sample being analyzed. They appear as dips or gaps in the spectrum where less light is detected.
Absorption spectrum is a gap in the overall spectrum. It happen when light makes an electron jump to a higher orbital and light energy is absorbed. Emission spectrum is light emitted at particular wavelengths (where the absorption spectrum gaps are). It happens when an electron falls from a higher orbital and emits light energy in doing so.
An absorption edge is the boundary of a dark bad in an x-ray spectrum.