Spectroscopy 101 – How Absorption and Emission Spectra Work

Spectroscopy 101 – How Absorption and Emission Spectra Work Why do different elements have different spectral patterns? Let’s go back to simple absorption and emission spectra. We can use a star’s absorption spectrum to figure out what elements it is made of based on the colors of light it absorbs. We can use a glowing nebula’s emission spectrum to figure out what gases it is made of based on the colors it emits. We can do both of these because each element has its own unique spectrum. An element’s spectrum is like its fingerprint, its autograph, its barcode. Why is this? Let’s take a look at hydrogen, the most abundant element in the universe. Absorption of Light by Hydrogen A hydrogen atom is very simple. It consists of a single proton in the nucleus, and one electron orbiting the nucleus. When a hydrogen atom is just sitting around without much energy, its electron is at the lowest energy level. When the atom absorbs light, the electron jumps to a higher energy level (an “excited state”). It can jump one level or a few levels depending on how much energy it absorbs. The interesting thing is that the electron can move only from one energy level to another. It can’t go partway between levels. In addition, it takes a very discrete amount of energy—no more, no less—to move the electron from one particular level to another. The energy that an electron needs in order to jump up to a certain level corresponds to the wavelength of light that it absorbs. Said in another way, electrons absorb only the photons that give them exactly the right energy they need to jump levels. (Remember https://science.nasa.gov/mission/webb/science-overview/science-explainers/spectroscopy-101how-absorption-and-emission-spectra-work/ when we said that photons only carry very specific amounts of energy, and that their energy corresponds to their wavelength?) The absorption spectrum of hydrogen shows the results of this interaction. In the visible part of the spectrum, hydrogen absorbs light with wavelengths of 410 nm (violet), 434 nm (blue), 486 nm (blue-green), and 656 nm (red). Each of the absorption lines corresponds to a specific electron jump. The shortest wavelength/highest energy light (violet 410 nm) causes the electron to jump up four levels, while the longest wavelength/lowest energy light (red 656 nm) causes a jump of only one level. The relationship between a hydrogen atom and its absorption spectrum. (Left) A simple model of a hydrogen atom showing four of the many possible “jumps” the electron could make when it absorbs light. (Right) The relationship between the electron jumps and the specific wavelengths of light that the atom absorbs. An electron jumps from one energy https://science.nasa.gov/mission/webb/science-overview/science-explainers/spectroscopy-101how-absorption-and-emission-spectra-work/ level to another only when it absorbs a very specific wavelength of light (i.e., when it absorbs a photon with a specific energy). The shorter the wavelength, the higher the energy, and the higher the jump. This illustration shows a set of jumps that correspond to absorption of visible wavelengths (the Balmer Series). NASA, ESA, and L. Hustak (STScI) Emission of Light by Hydrogen Electrons can also lose energy and drop down to lower energy levels. When an electron drops down between levels, it emits photons with the same amount of energy—the same wavelength—that it would need to absorb in order to move up between those same levels. This is why hydrogen’s emission spectrum is the inverse of its absorption spectrum, with emission lines at 410 nm (violet), 434 nm (blue), 486 nm (blue-green), and 656 nm (red). The highest energy and shortest wavelength light is given off by the electrons that fall the farthest. https://science.nasa.gov/mission/webb/science-overview/science-explainers/spectroscopy-101how-absorption-and-emission-spectra-work/ The relationship between a hydrogen atom and its emission spectrum. (Left) A simple model of a hydrogen atom showing four of the many possible “drops” the electron could make when it emits light. (Right) The relationship between the electron drop and the specific wavelengths of light that the atom emits. When an electron drops down from one energy level to another, it emits a very specific wavelength of light (i.e., it emits a photon with a specific energy). The farther the drop, the shorter the wavelength and the higher the energy of the photon. This illustration shows a set of drops that correspond to emission of visible wavelengths (the Balmer Series). NASA, ESA, CSA, Leah Hustak (STScI) Other Atoms and Molecules Different elements have different spectra because they have different numbers of protons, and different numbers and arrangements of electrons. The differences in https://science.nasa.gov/mission/webb/science-overview/science-explainers/spectroscopy-101how-absorption-and-emission-spectra-work/ spectra reflect the differences in the amount of energy that the atoms absorb or give off when their electrons move between energy levels. Molecules, like water, carbon dioxide, and methane, also have distinct spectra. Although it gets a bit more complicated, the basic idea is the same. Molecules can absorb specific bands of light, corresponding to discrete changes in energy. In the case of molecules, these changes in energy can be related to electron jumps, but can also be related to rotations and vibrations of the molecules. 1.​ What causes dark lines to appear in a star’s spectrum? a.​ The star fails to produce those colors b.​ Electrons absorb specific wavelengths of light c.​ The telescope blocks some wavelengths d.​ The star has a cooler surface than other stars 2.​ Why can scientists identify elements in stars using spectroscopy? a.​ All stars emit only one color of light b.​ Each element produces a unique pattern of spectral lines c.​ Stars are always made of hydrogen and helium only d.​ Spectra show the physical size of the stars 3.​ A continuous spectrum becomes an absorption spectrum when: a.​ light passes through a cooler gas b.​ the star stops emitting light c.​ only red wavelengths are present d.​ electrons emit photons of all colors 4.​ Which type of spectrum shows bright lines on a dark background? a.​ Absorption spectrum b.​ Continuous spectrum c.​ Emission spectrum d.​ Doppler spectrum 5.​ In your own words, explain why an absorption spectrum can tell us which elements are present in a star’s atmosphere. Use evidence from the reading. The Absorption spectrum of an atom has lines which are the specific energy levels that the elements absorb due to each element having their own unique spectrum. By looking at the emission spectrums of other elements that match the lines we can determine the elements in the atmosphere of the star.