Module 49 Stratospheric Ozone Depletion

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Presentation transcript:

Module 49 Stratospheric Ozone Depletion After reading this module, you should be able to Explain the benefits of stratospheric ozone and how it forms. Describe the depletion of stratospheric ozone. Explain efforts to reduce ozone depletion.

Stratospheric ozone is beneficial to life on Earth The stratospheric ozone layer exists roughly 45- 60 kilometers above Earth. Ozone has the ability to absorb ultraviolet radiation and protect life on Earth. The ultraviolet (UV) spectrum is made up of three increasingly energetic ranges: UV-A, UV-B, and UV-C.

Formation of Stratospheric Ozone UV-C radiation breaks the molecular bond holding an oxygen molecule together: O2 + UV-C → O + O   A free oxygen atom (O) produced in the first reaction encounters an oxygen molecule, and they form ozone. O + O2 → O3   Both UV-B and UV-C radiation can break a bond in this new ozone molecule:  O3 + UV-B or UV-C → O2 + O

Breakdown of Stratospheric Ozone   When chlorine is present (from CFCs), it can attach to an oxygen atom in an ozone molecule to form chlorine monoxide (ClO) and O2:  O3 + Cl → ClO + O2   The chlorine monoxide molecule reacts with a free oxygen atom, which pulls the oxygen from the ClO to produce free chlorine again: ClO + O → Cl + O2

Breakdown of Stratospheric Ozone A single chlorine atom can catalyze the breakdown of as many as 100,000 ozone molecules until finally one chlorine atom finds another and the process is stopped. In the process, the ozone molecules are no longer available to absorb incoming UV-B radiation. As a result, the UV-B radiation can reach Earth’s surface and cause harm to biological organisms. Ozone Hole

Depletion of the Ozone Layer Stratospheric ozone concentration. This data for one area of Switzerland shows a generally decreasing trend from1970 to 2011.