![]() It is because of this that visible light is sometimes referred to as ROY G. Dispersion of visible light produces the colors red (R), orange (O), yellow (Y), green (G), blue (B), and violet (V). For these reasons, visible light is dispersed upon passage through a prism. Each color is characteristic of a distinct wavelength and different wavelengths of light waves will bend varying amounts upon passage through a prism. The separation of visible light into its different colors is known as dispersion. Isaac Newton showed that light shining through a prism will be separated into its different wavelengths and will thus show the various colors that visible light is comprised of. That is, when light of that particular wavelength strikes the retina of our eye, we perceive that specific color sensation. This narrow band of visible light is affectionately known as ROYGBIV.Įach individual wavelength within the spectrum of visible light wavelengths is representative of a particular color. Expressed in more familiar units, the range of wavelengths extends from 7 x 10 -7 meter to 4 x 10 -7 meter. This visible light region consists of a spectrum of wavelengths that range from approximately 700 nanometers (abbreviated nm) to approximately 400 nm. In this sense, we are referring to visible light, a small spectrum from the enormous range of frequencies of electromagnetic radiation. Normally when we use the term "light," we are referring to a type of electromagnetic wave that stimulates the retina of our eyes. Since this narrow band of wavelengths is the means by which humans see, we refer to it as the visible light spectrum. Though electromagnetic waves exist in a vast range of wavelengths, our eyes are sensitive to only a very narrow band. The focus of Lesson 2 will be upon the visible light region - the very narrow band of wavelengths located to the right of the infrared region and to the left of the ultraviolet region. You are undoubtedly familiar with some of the other regions of the electromagnetic spectrum. Two very narrow regions within the spectrum are the visible light region and the X-ray region. The longer wavelength, lower frequency regions are located on the far left of the spectrum and the shorter wavelength, higher frequency regions are on the far right. The diagram below depicts the electromagnetic spectrum and its various regions. The subdividing of the entire spectrum into smaller spectra is done mostly on the basis of how each region of electromagnetic waves interacts with matter. The entire range of the spectrum is often broken into specific regions. This continuous range of frequencies is known as the electromagnetic spectrum. Nonetheless, there are a variety of statements that can be made about such waves.Įlectromagnetic waves exist with an enormous range of frequencies. The precise nature of such electromagnetic waves is not discussed in The Physics Classroom Tutorial. Electromagnetic waves are produced by a vibrating electric charge and as such, they consist of both an electric and a magnetic component. Unlike mechanical waves that require a medium in order to transport their energy, electromagnetic waves are capable of transporting energy through the vacuum of outer space. Sources of x-rays include million-degree gas, exploded stars, and material colliding around black holes.As discussed in Unit 10 of The Physics Classroom Tutorial, electromagnetic waves are waves that are capable of traveling through a vacuum. ![]() The blue color shows Chandra's view in x-ray light. Most of this light comes from stars, and they trace the same spiral structure as the dust lanes. The yellow color is Hubble's view in visible light. It highlights the heat emitted by dust lanes in the galaxy where stars can form. ![]() The red color shows Spitzer's view in infrared light. This composite image of the spiral galaxy Messier 101 combines views from Spitzer, Hubble, and Chandra space telescopes. Credit: Mars Odyssey Thermal Emission Imaging System, NASA/JPL/ASU. Large deposits of the mineral olivine appear in this image as magenta to purple-blue. Martian Soil - This false-color infrared image from the Thermal Emission Imaging System (THEMIS) camera onboard the Mars Odyssey spacecraft reveals the differences in the mineralogy, chemical composition, and structure of the Martian surface.
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