* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Download Lab 11: Atomic Spectra
Survey
Document related concepts
Super-resolution microscopy wikipedia , lookup
Rotational–vibrational spectroscopy wikipedia , lookup
Gaseous detection device wikipedia , lookup
Photomultiplier wikipedia , lookup
Gamma spectroscopy wikipedia , lookup
Rutherford backscattering spectrometry wikipedia , lookup
Mössbauer spectroscopy wikipedia , lookup
Auger electron spectroscopy wikipedia , lookup
Diffraction grating wikipedia , lookup
Upconverting nanoparticles wikipedia , lookup
Photonic laser thruster wikipedia , lookup
Ultraviolet–visible spectroscopy wikipedia , lookup
Population inversion wikipedia , lookup
Ultrafast laser spectroscopy wikipedia , lookup
Laser pumping wikipedia , lookup
Transcript
LAB 11 Atomic Spectra and Fluorescence OBJECTIVES 1. Observe and study the bright line spectra produced by hydrogen in the Balmer series. 2. Predict the wavelengths of the photons in the Balmer series. 3. Measure the wavelengths and correlate them with photon energies and electron energy level diagrams. EQUIPMENT Diffraction gratings, laser, gas lamps, and spectrometers. THEORY The hydrogen atom is of particular theoretical interest because it is the simplest of all atoms: one electron and one proton. The hydrogen atom is observed to have spectral lines as a result of photons being emitted by electron transitions between different atomic energy levels. From solving the three-dimensional Schrodinger’s Equation for the hydrogen atom, it is found that the energy of an electron with principle quantum number n is given by: 4 me 1 1 En = − 2 2 2 = ( −13.6 eV) 2 8e 0 h n n When an electron jumps from an excited state (n >1) to a lower energy state, it emits a photon whose energy is equal to the difference in energy between the two different states. The wavelengths of these photons (or spectral lines) are given theoretically by = λ hc / ∆E . The Balmer series produces a line spectrum in the visible region when the electron transitions have a final state n f = 2 as seen below: PROCEDURE Part 1: The Atomic Spectrum of Fluorescent Lights a. Look at the fluorescent lights with the blue spectrometers. Write down the wavelengths of the most prominent lines you can see, along with their colors. (Some will be smeared so just do the best you can). b. Using the jpg image of the spectra of different gases, (i) identify the wavelengths you observed and determine what gas (es) are in the fluorescent bulbs. You might not find all the lines in the list of gases - if not, discuss where these lines might come from. (ii) Which ones (color and wavelength) were not found among the list of gases? Part 2: Light Spectra of Other Gases As stated above, each element can only emit specific frequencies of light. Astronomers use this fact to determine what a star is composed of (i.e. H, He, C, …) by observing the spectrum of light emitted by the star. In this part of the lab, you will play astronomer and determine what type of gas is contained in each of three gas lamps. (a) Use a diffraction grating to observe the spectra of each of the three different gas lamps. (b) Sketch the spectra for each of the three different gas lamps. (c) Using the chart of different line spectra, identify what kind of gas is in each of the three lamps. Part 3: Hydrogen Gas Spectra a. Using the hydrogen energy levels, create an Excel table that predicts all of the visible photon wavelengths for all jumps for the first 5 electron energy jumps. Setup the columns of n, m, λ(nm), Spectrum, and Color. b. Which visible wavelengths are observable in the hydrogen atomic spectrum? c. Use the calibrated blue spectrometers to identify the color and measure the wavelengths of the observed atomic spectrum of hydrogen. d. Compare the measured and predicted wavelengths using a percent difference. How do they compare? Part 4: Fluorescence Fluorescence occurs when an atom absorbs light at one frequency but then emits light at lower frequencies. For example, an atom can absorb a UV photon and jump to a higher energy state. Rather then jumping directly back to the initial energy state (and emitting the same energy UV photon), the atom can make several smaller jumps and emit lower energy photons (such as visible light). This is how black lights work. In this station, you will observe the light emitted by different fluorescent paints that are illuminated by different frequency lasers. (1) Shine the red laser onto each of the three different color fluorescent paints (green, red, and yellow). Use a diffraction grating to observe the spectra emitted by each paint. (2) Shine the green laser onto each of the three different color fluorescent paints (green, red, and yellow). Use a diffraction grating to observe the spectra emitted by each paint. (3) Shine the blue laser onto each of the three different color fluorescent paints (green, red, and yellow). Use a diffraction grating to observe the spectra emitted by each paint. (4) Which color paints does the red laser cause to fluoresce? Which color paints does the green laser cause to fluoresce? Which color paints does the blue laser cause to fluoresce? (5) Can you come up with a general rule for which color laser will cause which colors of paint to fluoresce? Explain your reasoning in terms of fluorescence and photon energies.