FIGURE 29.2 Examples of spectra in the visible wavelength range 400-700 nm. Hydrogen Mercury Neon 400 nm 500 nm 600 nm 700 nm Violet Blue Green Yellow Orange Red Figure 29.2 shows that the atomic spectra of hydrogen, mercury, and neon look very different from one another. In fact, every element in the periodic table has its own, unique discrete spectrum. The fact that each element emits a unique spectrum means that atomic spectra can be used as “fingerprints" to identify elements. Conse- quently, atomic spectroscopy is the basis of many contemporary technologies for analyzing the composition of unknown materials, monitoring air pollutants, and studying the atmospheres of the earth and other planets. TABLE 29.1 Wavelengths of visible lines in the hy drogen spectrum 656 nm 486 nm 434 nm 410 nm

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As shown the wavelengths of the first four lines in the visible spectrum of hydrogen.
a. Determine the Balmer formula n and m values for these wavelengths.
b. Predict the wavelength of the fifth line in the spectrum.

FIGURE 29.2 Examples of spectra in the visible wavelength range 400-700 nm.
Hydrogen
Mercury
Neon
400 nm
500 nm
600 nm
700 nm
Violet
Blue
Green
Yellow Orange
Red
Figure 29.2 shows that the atomic spectra of hydrogen, mercury, and neon look
very different from one another. In fact, every element in the periodic table has its
own, unique discrete spectrum. The fact that each element emits a unique spectrum
means that atomic spectra can be used as “fingerprints" to identify elements. Conse-
quently, atomic spectroscopy is the basis of many contemporary technologies for
analyzing the composition of unknown materials, monitoring air pollutants, and
studying the atmospheres of the earth and other planets.
Transcribed Image Text:FIGURE 29.2 Examples of spectra in the visible wavelength range 400-700 nm. Hydrogen Mercury Neon 400 nm 500 nm 600 nm 700 nm Violet Blue Green Yellow Orange Red Figure 29.2 shows that the atomic spectra of hydrogen, mercury, and neon look very different from one another. In fact, every element in the periodic table has its own, unique discrete spectrum. The fact that each element emits a unique spectrum means that atomic spectra can be used as “fingerprints" to identify elements. Conse- quently, atomic spectroscopy is the basis of many contemporary technologies for analyzing the composition of unknown materials, monitoring air pollutants, and studying the atmospheres of the earth and other planets.
TABLE 29.1 Wavelengths of visible lines
in the hy drogen spectrum
656 nm
486 nm
434 nm
410 nm
Transcribed Image Text:TABLE 29.1 Wavelengths of visible lines in the hy drogen spectrum 656 nm 486 nm 434 nm 410 nm
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