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Report - School of Physics

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SOFIA: SOFIA (Stratospheric Observatory for Infrared Astronomy) is a joint endeavour<br />

<strong>of</strong> NASA and the German DLR (http://www.s<strong>of</strong>ia.arc.nasa.gov/). A modified<br />

Boeing 747SP carrying a 2.7-m telescope will operate at an altitude <strong>of</strong> about<br />

12 km. The first call for proposals will be issued in August 2005 for the first observing<br />

cycle starting in January 2006. A total <strong>of</strong> nine instrument have been selected,<br />

providing imaging and spectroscopy in the range 1–600 µm. Operating out <strong>of</strong> NASA<br />

Ames Research Center, the facility is to observe three or four nights a week for at<br />

least twenty years. Its location above the bulk <strong>of</strong> Earth’s atmosphere will provide<br />

access to the mid-infrared region without the limitations <strong>of</strong> observatories on the<br />

ground. Its long projected lifetime will make it possible to conduct muli-epoch<br />

observations for variable or evolving objects and the ability to easily exchange instruments<br />

will ensure that the latest technology can be incorporated as it becomes<br />

available.<br />

The science with SOFIA will revolve around cold matter in our solar system, the<br />

interstellar medium, stars and galaxies. Similar to Spitzer, SOFIA is not expected<br />

to contribute directly to the discovery <strong>of</strong> extra-solar planets, but it will enhance<br />

understanding <strong>of</strong> planet formation by studying circumstellar disks. Furthermore it<br />

will provide interesting information on the infrared spectra <strong>of</strong> solar system bodies<br />

including the chemistry <strong>of</strong> atmospheres.<br />

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