UV Mini Lesson Spring 2011. I. Introduction What is UV light? UV stands for Ultraviolet, a portion of the light spectrum that is beyond the violet light.

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Presentation transcript:

UV Mini Lesson Spring 2011

I. Introduction What is UV light? UV stands for Ultraviolet, a portion of the light spectrum that is beyond the violet light that we can see with our eyes. Humans cannot see UV light. Humans have ways to make UV light. We will use the LED black light to emit UV light. Where does UV light come from? Ultraviolet light is produced by the sun, and most UV radiation is absorbed by the atmosphere or reflected back into space. UV waves have higher energy than visible light. Since we cannot see ultraviolet light, how can it be detected? Some chemicals absorb UV light and then re-emit the energy as visible light.

II. How is UV light useful? How Can UV light be Useful? Ultraviolet lights are used by forensic scientists to detect bodily fluids. They can be used to kill bacteria, and bug zappers use UV light to attract insects. They are used to detect fake dollar bills ($5 and up). This strip can be seen in visible light, but fluoresces only under UV light. Bills of different denominations have strips that fluoresce different colors and are at different positions on the bill. The $1 bill does not have a strip. How is UV light dangerous? Ultraviolet light can damage DNA. This affects the function of the cells, and sometimes this makes the cells grow uncontrollably, a condition called cancer. UVB light also damages the tissue in our eyes and can cause cataracts. We should block as much UV light from our bodies as is possible. How do you know if your skin has received too much UV light? – It turns red and becomes tender, i.e., you get a sunburn. What are some ways to block UV light? – There are many ways to block UV light. They include: sunscreen, long sleeves and pants, wide brimmed hats, sunglasses, and staying in the shade. Glass in windows transmits less than 10% of sun-burning UV light

How do you know how well a sunscreen blocks UV light? – All sunscreen is labeled with an SPF (Sun Protection Factor) number that indicates how well it absorbs UV light. – For example, an SPF of 15 means that it should take 15 times as long for skin damage to occur as it would on unprotected skin. – Doctors recommend that everyone (even those with dark skin) wear a sunscreen with an SPF of at least 15 whenever they are in the sun. – Show the students the picture of the different sunscreens and point out the SPF caption. Who should wear sunscreen? Everyone! Although darkly pigmented persons develop skin cancer on sun-exposed sites at lower rates than lightly pigmented persons, UV exposure will still increase their risk for developing skin cancer.”

III. Testing UV Blocking Materials Explain that this color change is due to the presence of UV light. The beads contain a chemical that absorbs the UV light and reemits it as colored visible light. Point out the purple beads in the necklace and tell the students that they will be using just the purple beads for this experiment because these change to a more intense color than the others. Show the students a necklace of UV detecting beads. Point out that all the beads are white. Expose the necklace to the 8 inch UV light, until the beads have turned color. Part A: How UV beads work

III. Testing UV Blocking Materials Part B: Testing UV blockers Make sure that the students hold the UV light 9 inches above the beads, not directly on top of them! 9 inches Correct: Incorrect:

III. Testing UV Blocking Materials Place 2 beads on the observation sheet. Leave the first bead exposed. This is the control bead. Put the lens of a sunglass upside down over the 2 nd bead so that it is covered. Hold the UV light 9 inches above the two beads and turn it on for 8 seconds. Turn the UV light off, remove the lens and compare the color of the beads. Record the results. Repeat the set-up, using 2 new beads. Put the piece of T-shirt over one bead and repeat step 3. Repeat the set-up, using 2 new beads. Distribute a piece of sunscreen-smeared acetate to each group and place the acetate on top of one bead. Part B: Testing UV blockers

III. Testing UV Blocking Materials Part B: Testing UV blockers Using the T-shirt as a UV blocker:

III. Testing UV Blocking Materials Part B: Testing UV blockers Using the sunscreen as a UV blocker: Spread the sunscreen thickly on the acetate

IV. Discuss and Review Does sunscreen really work? Was there any difference in the effect of SPF 8 or 45 sunscreen? Do sunglasses block UV? – You may want to elaborate that these sunglasses were cheap. The cheapest we could buy. Expensive glasses may provide even more UV protection than these. Does clothing protect you from UV light?

V. Making a UV-sensitive bead bracelet Give each student a cup of 3 UV beads and 1 piece of braid. Tell the students to string the beads onto the braid. After they have finished stringing the beads, they should make a bracelet by putting the untied end through the hole in the bead on the tied-off end and tie a knot. When they are finished, they should shine their black light on the beads. Tell the students they get to keep the bracelet and should use it to measure the amount of UV radiation on sunny days. They could keep a diary of their results – trying different times of the day and different times of the year – summer vs. winter.

VI. Discussion on Ozone Depletion How is the earth’s atmosphere is protected from too much UV radiation? A layer of ozone in the upper atmosphere screens out dangerous UV rays. Ozone is an essentially colorless gas (pale blue at high concentrations) that has a distinctively sharp and unpleasant smell. Ozone is naturally formed in the atmosphere when UV rays react with O 2. In the upper atmosphere, ozone is a “good” gas, since it screens out dangerous UV rays. But close to ground ozone is a pollutant and can act as a greenhouse gas.

VI. Discussion on Ozone Depletion In the mid-1970s researchers discovered that the ozone layer was being depleted by chlorine contained in chlorofluorocarbons (CFCs). It will be at least 2050 before the ozone level reverts to that present before depletion began. The amount of ozone layer depletion depends on the latitude, and is much greater at the highest southern latitudes. An ozone hole forms over Antarctica every spring (this has happened since the late 1970s). Ozone loss in the polar regions during the winter and spring can be as great as 50% of what is normally present. Although the ozone layer recovers from these seasonal losses, the average decrease of global ozone since 1980 is 4%. The decrease in the ozone layer has caused an increase in UV rays reaching the earth’s surface. This increase correlates with an increase in the “UV Index”, a measure of the peak sunburning UV times at a particular location. (UV Indexes are often part of the daily weather report.)