Wandering Ozone Hole in November 2009

Wandering Ozone Hole in November 2009
  • Credit:

    NASA image courtesy Ozone Hole Watch. Animation by Jesse Allen. Caption by Michael Carlowicz.

The annual hole in the ozone layer over the South Pole is not static, nor is it necessarily symmetrical or circular. But in November 2009, the hole contorted and stretched itself for three weeks in such a way as to give South Americans an extra dose of ultraviolet (UV) radiation.

This image—assembled from data from the Ozone Monitoring Instrument (OMI) on NASA’s Aura satellite—shows the Antarctic ozone hole as it appeared on November 13, 2009; the downloadable movie shows the entire month of November. The hole stretched into an oblong shape and persistently extended over the southern reaches of South America from November 11 to 30.

Using measurements from ground stations and from satellites such as Aura, researchers led by Jos de Laat of the Royal Netherlands Meteorological Institute found that the ozone hole was centered just off the southern tip of Chile and Argentina for three weeks in November 2009, rather than its usual center over Antarctica.

According to atmospheric scientist Paul Newman of NASA’s Goddard Space Flight Center, it is not necessarily the first time scientists have observed a hole stretching so far north or taking such an oblong shape. Variability in the shape, size, and duration of the annual ozone hole are determined mostly by temperature and wind patterns in the stratosphere. But the northward-shifted hole was unusually persistent in 2009, and it was the first time such a phenomenon has affected South America, according to de Laat et al. The event gave citizens of Tierra del Fuego and nearby regions nearly twice the normal dose of UV radiation for the area.

The ozone layer is Earth’s natural sunscreen, absorbing and blocking most of the incoming UV radiation from the Sun and protecting life from DNA-damaging radiation. Ozone gas is naturally created and replenished by a chemical reaction in the upper atmosphere, where UV rays break oxygen molecules (O2) into individual atoms that then recombine into three-part molecules (O3). As it is moved around the globe by upper level winds, ozone is slowly depleted by naturally occurring atmospheric gases.

If you want to see how this year’s ozone hole is evolving—it is now shrinking and breaking up as southern spring sunlight returns—visit NASA’s Ozone Hole Watch page.

  1. References

  2. de Laat, A.T.J., et al (2010). Extreme sunbathing: Three weeks of small total O3 columns and high UV radiation over the southern tip of South America during the 2009 Antarctic O3 hole season. Geophysical Research Letters. Vol. 37, L14805, 6 pp.
  3. NASA (n.d.) Ozone Hole Watch. Accessed November 1, 2010.
  4. NASA Earth Observatory (n.d) World of Change: Antarctic Ozone Hole. Accessed November 1, 2010.
  5. NASA Earth Observatory (2009, May 13) The World We Avoided by Protecting the Ozone Layer. Accessed November 1, 2010.

Images & Animations


File Dimensions

  • 720x720
  • JPEG
  • 720x37
  • JPEG
  • QuickTime 4 MB

Note: Often times, due to the size, browsers have a difficult time opening and displaying images. If you experiece an error when clicking on an image link, please try directly downloading the image (using a right click, save as method) to view it locally.


  • Data Date:

    November 13, 2009
  • Visualization Date:

    November 1, 2010
  • Sensor(s):

    Aura - OMI


NASA - National Aeronautics and Space Administration