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Spectra - Introduction Astronomy II - Laboratory 10 | ASTR 1402, Lab Reports of Astronomy

Material Type: Lab; Class: Intro Astronomy II; Subject: Astronomy; University: University of Texas - Pan American; Term: Unknown 1989;

Typology: Lab Reports

2009/2010

Uploaded on 02/24/2010

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Astronomy 1402
Department of Physics and Geology Spectra
Equipment Needed Qty Equipment Needed Qty
Spectroscope 1 Set of Colors 1
Gas Spectral Lamps 13 Ruler 1
Background
When an atom is excited, electrons change their energy levels to higher ones. When electrons from
higher energy levels drop back down to lower energy levels, energy is released in the form of light as
shown in the figure 1. The frequency of the emitted light depends directly on the energy between the
two orbits and this determines the color of the light. Every element has a unique spectrum of light
composed of a set number of different frequencies. If materials are heated, the elemental composition
can be determined by resolving those unique spectrums from the emitted light.
Figure 1. A photon may be emitted when the electron drops from high energy level to low energy level.
White light contains all frequencies of visible light. When white light passes through a prism or a
diffraction grating, its component colors are separated and one can distinguish the colors (like in a
rainbow). A device specifically designed to separate the components of light and atomic spectra is the
spectroscope. A spectroscope contains a narrow slit on one end, a long body, and a diffraction grating at
the other end, as shown in Figure 2. When we look at the spectroscope, we see a strong line from the
light source in the middle. On both sides of the strong line, we will see relatively weaker spectra. The
spectrum is same for both sides but in reverse order. In order to observe the spectrum with your eye,
you may look at the spectrum on one side (left or right side). Figure 3 shows an example of a spectrum
from a Helium gas spectral tube.
Figure 2. Simple diagram of a spectroscope Figure 3. Helium spectrum
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Astronomy 1402

Department of Physics and Geology

Spectra

Equipment Needed Qty Equipment Needed Qty

Spectroscope 1 Set of Colors 1

Gas Spectral Lamps 13 Ruler 1

Background

When an atom is excited, electrons change their energy levels to higher ones. When electrons from

higher energy levels drop back down to lower energy levels, energy is released in the form of light as

shown in the figure 1. The frequency of the emitted light depends directly on the energy between the

two orbits and this determines the color of the light. Every element has a unique spectrum of light

composed of a set number of different frequencies. If materials are heated, the elemental composition

can be determined by resolving those unique spectrums from the emitted light.

Figure 1. A photon may be emitted when the electron drops from high energy level to low energy level.

White light contains all frequencies of visible light. When white light passes through a prism or a

diffraction grating, its component colors are separated and one can distinguish the colors (like in a

rainbow). A device specifically designed to separate the components of light and atomic spectra is the

spectroscope. A spectroscope contains a narrow slit on one end, a long body, and a diffraction grating at

the other end, as shown in Figure 2. When we look at the spectroscope, we see a strong line from the

light source in the middle. On both sides of the strong line, we will see relatively weaker spectra. The

spectrum is same for both sides but in reverse order. In order to observe the spectrum with your eye,

you may look at the spectrum on one side (left or right side). Figure 3 shows an example of a spectrum

from a Helium gas spectral tube.

Figure 2. Simple diagram of a spectroscope Figure 3. Helium spectrum

By observing the spectra of heated materials using the spectroscope, we can identify the chemical

compositions of the materials. In fact, this method is commonly used to study the chemical environment

of distant stars or planets. In this lab, we study atomic spectra by observing light from gas spectral tubes.

SAFETY REMINDER

• Follow the directions for using the equipment

• Do not touch light sources.

For You To Do

The purpose of this laboratory activity is to examine the atomic spectra given off from excited gases

using a spectroscope and identify an element by its spectra.

PART I: Gas Spectral Tubes

Using a spectroscope, observe the spectra from various light sources. Sketch the spectra in the box

below. Use crayons to draw the spectral lines

PART II: Identification of the spectra of an element

1. Calibrate the Spectra of the Color Plate. Use a ruler to mark off a linear wavelength scale across

the bottom of the color plate such that the experimental wavelengths of the mercury spectrum

correlate with those in the table. Extend the linear wavelength scale perpendicularly and upward

across spectra on the color plate, thus creating the same wavelength scale for all of the emission

spectra.

2. Your instructor will assign to you two emission spectra from the color plate. Analyze each

spectrum by locating the most intense wavelengths in the assigned emission spectrum.

3. Compare the wavelengths of the most intense lines with the data in Table 1.

4. Identify the element having the shown spectrum.

Record your results in the Lab Report section.

Mercury Spectrum

Violet 404.7 nm

Violet 407.8 nm

Blue 435.8 nm

Yellow 546.1 nm

Orange 577.0 nm

Orange 579.1 nm