Reading The Colors of the Spectrum
Did you ever wonder how scientists can tell us so much about distant stars, for example, the surface temperature or chemical makeup of a star, light years away from Earth? Scientists can only use what the star sends our way -- its radiation, and specifically radiation in the form of light that travels through space and reaches us. The branch of science that analyzes this radiation is called spectroscopy.
Spectroscopy uses a common principle of light, the fact that white light can be broken into different and distinct colors by shining it through a prism, creating a spectrum. A spectrum is nothing more than a representation of light at different frequencies. Our Sun breaks light into the familiar colors of the rainbow. But what does a spectrum tell us about such things as the chemical composition or the temperature of our Sun and other stars?
The answer lies in another aspect of how the spectrum is affected by different gases. An absorption spectrum, also called a black line spectrum exposes black lines amid the colors. These black lines coincide with the absorption of light of particular wave lengths by gases. By examining the black lines on the spectrum scientists can tell what elements are affecting the spectrum and hence what elements are contained in the star. And by adding Wien's law, which is a formula that uses the wavelength of a star to plot its temperature, scientists can figure out quite a lot about objects millions and millions of miles away.
About the Author
Gene Mascoli, JD
Gene Mascoli is a founder and publisher of ScienceIQ.com. He holds a J.D. degree from the University of Santa Clara and a B.A. in English. In 1997 Gene launched ScienceMaster.com, an online science education portal where he brought together his love of writing with his interest in the sciences. Gene collaborated with David Gamon on the popular digital book “The Internet Guide to NASA on the Net” and has also produced two popular science CD-ROMs on astronomy and space science.